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12-15-2018 Precaspian Isthmus Emergence Triggered the Early Sakmarian Glaciation (Paleontologic, Sedimentologic and Geochemical Proxies) Vladimir I. Davydov Boise State University
Publication Information Davydov, Vladimir I. (2018). "Precaspian Isthmus Emergence Triggered the Early Sakmarian Glaciation (Paleontologic, Sedimentologic and Geochemical Proxies)". Palaeogeography, Palaeoclimatology, Palaeoecology, 511, 403-418. http://dx.doi.org/ 10.1016/j.palaeo.2018.09.007
This is an author-produced, peer-reviewed version of this article. © 2018, Elsevier. Licensed under the Creative Commons Attribution- NonCommercial-NoDerivatives 4.0 license. The final, definitive version of this document can be found online at Palaeogeography, Palaeoclimatology, Palaeoecology, doi: 10.1016/j.palaeo.2018.09.007 Precise timing of the Precaspian- Tethys Seaway closure (Precaspian Isthmus) is established
The emergence of the Isthmus occurs at the Asselian-Sakmarian transition
The biotic and sedimentological evidences support the emergence of the Isthmus
The event changed the global oceanic circulation and is the major driver of the glaciation 295-290 Ma ? 310-295 Ma Uralian Foredeep ? 11 12 11 10 10 8 8 5 12 7 9 6-7 5 9 6 4 4 2
3 1 2 Center of originations
1 Center of originations
WWBF Realms: Tethyan Boreal North American Direction of oceanic currents 1 Precaspian Isthmus emergence triggered the Early Sakmarian glaciation
2 (paleontologic, sedimentologic and geochemical proxies)
3 Vladimir I. Davydov a,b,с,*
4 a Permian Research Institute, Boise State University, 1910 University Drive, Boise, ID, 83725,
5 USA
6 b Kazan Federal University, Kremlevskaya St., 4/5, Kazan’, Tatarstan Republic, Russia
7 c North-East Interdisciplinary Scientific Research Institute n. a. N.A. Shilo Far East Branch of the
8 Russian Academy of Sciences, Magadan.
9 * Corresponding author: [email protected]
10ABSTRACT
11 The sub-meridional seaway that connected Paleo-Arctic and Paleo-Tethys basins was one of the
12 most important geographical attributes of the Late Paleozoic Pangea landscape,
13 paleogeography and paleoclimate. Existing models about the timing of the disconnection of
14 the Paleo-Arctic and the Paleo-Tethyan oceans is very controversial and poorly documented.
15 Warm-water benthic foraminifera (WWBF) were utilized to establish the precise timing of the
16 closure of the Urals-Precaspian-Paleo-Tethys Seaway (UPTS) during Cisuralian time. The WWBF
17 of Paleo-Tethys and those of the Ural—Precaspian Basins during the Gzhelian-Asselian, display a
18 considerably high level of similarity. Beginning from the Sakmarian, the faunas of these two
19 regions became dissimilar, suggesting a break in the connection between the Paleo-Tethys and
20 Ural-Precaspian Basins. The sedimentological evidence (olistostromes and seismites) of the final
21 collision of the Eastern Ural, Kazakhstania, Scythian-Turan plates with the southeastern part of
22 the Russian Platform during Late Paleozoic also support the emergence of the Precaspian
23 Isthmus at the Asselian-Sakmarian transition. The oceanic currents in the Precaspian and the
24 Southern Ural Basins before the Sakmarian were directed northward and later changed to the 25 south. These biotic and physical changes are consistent with the proposed timing of the cutoff
26 of the UPTS. The biotic and sedimentologic features clearly suggest the UPTS closure and the
27 origination of Precaspian Isthmus during the Asselian-Sakmarian transition. The abrupt changes
28 in the oceanic circulation triggered changes in atmospheric CO2, atmospheric circulation and,
29 possibly, albedo feedback. The emergence of the Precaspian Isthmus induced an increase in the
30 poleward salt and heat transport towards mid- to lower latitude Gondwana and Cathasia
31 margins. The warm water currents and moisture along the margins of Gondwana caused a rapid
32 increase in the precipitation necessary to build significant ice sheets during the early-middle
33 Sakmarian.
34 Keywords: Oceanic gateway; Isthmus; Late Paleozoic glaciation; benthic foraminifera;
35 continents configuration.
36 1. Introduction
37 The Late Paleozoic glaciation is a very intriguing and controversial matter and is the penultimate
38 icehouse-greenhouse transition on Earth (Crowell, 1999; Montanez and Poulsen, 2013; Smith and
39 Read, 2000). Our understanding of the processes associated with the glaciation, and particularly
40 the factors that caused the icehouse to greenhouse transition, may help us better understand the
41 changes to recent climate perturbations. The level of atmospheric CO 2 is considered the major
42 factor that drives climate change along with the other less important, such as tectonics,
43 continents configuration, variations of the orbital and spin axis of the Earth and other
44 extraterrestrial events (Montanez and Poulsen, 2013; Smith and Read, 2000). However, the
45 factors behind CO2 fluctuations in the past are unclear. The role of paleogeographic configuration
46 and solar irradiation is considered of secondary importance (Lowry et al., 2014).
47 The sub-meridional seaway that connected Paleo-Arctic and Paleo-Tethys basins was
48 one of the most important geographical attributes of the Late Paleozoic Pangea landscape,
49 paleogeography and paleoclimate (Scotese, 2015). The seaway which connected the shelves
50 along the East-European Craton, the Ural and the Paleo-Tethys was the major oceanic gateway
51 between the oceans in the Paleo-Tethys and Paleo-Arctic (Fig. 1). The final collision of
52 Kazakhstania and Siberian continents with the sutured Laurentia and Gondwana is usually
53 considered to have caused the closure of the Uralian foredeep and UPTS sometime in latest
54 Cisuralian time (Puchkov, 2010). Most tectonic models of the development of the Ural and the
55 surrounding areas during Paleozoic-Mesozoic time imply the existence of the UPTS until the
56 Kungurian because of the early Permian marine sedimentation in the Precaspian and the
57 Southern Ural. According to these models, the end of the marine sedimentation and the
58 accumulation of thick sabkha evaporites in the Precaspian and along the Ural during the
59 Kungurian denote the complete closure of the UPTS (Brown et al., 1997; Cocks and Torsvik,
60 2007; Golonka, 2007; Nikishin et al., 1996; Puchkov, 1997, 2009, 2010; Snyder et al., 1994;
61 Ziegler, 1989; Zonenshain et al., 1990). Nevertheless, some paleogeographic models suggest
62 the existence of the seaway between the Paleo-Arctic and the Paleo -Tethys until the Triassic
63 (Blakey, 2013; Chumakov and Zharkov, 2002; Domeier and Torsvik, 2014 Kaz'min and and
64 Natapov, 1998; Scotese, 2015). Other models suggest that the closing of the Uralian—Paleo-
65 Tethys connection happened in the Moscovian (Lawver et al., 2011) or sometime within the
66 Bashkirian - Kasimovian (Cavazza et al., 2004; Stampfli et al., 2013). Golonka (2011) proposed
67 that the seaway was closed in the Asselian-Artinskian and reopened in the Guadalupian. A
68 somewhat exotic idea by Sengor and Atayaman (2009) proposed that the Paleo-Arctic—Tethys
69 was connected through the hypothetical Carapelit rift during latest Kungurian-Wuchiapingian
70 time.
71 Existing models about the timing of the disconnection of the Paleo-Arctic and the Paleo-
72 Tethyan oceans is very controversial and poorly documented and one of the goals of this study
73 was to establish the precise timing of the event. The exceptionally accurate, quantitative
74 biostratigraphic and radioisotopic calibration of the Pennsylvanian–early Permian global time
75 scale, developed in the type sections in the Southern Ural was employed to establish the
76 precise timing of the geological events in the Late Paleozoic, including those in the Ural-
77 Precaspian regions ( Davydov et al., 2012; Davydov and Cozar, 2018, in press; Schmitz and
78 Davydov, 2012). The tropical-subtropical paleogeographic distribution and the well-known
79 sensitivity of WWBF to paleoenvironments, coupled with their application in development of
80 high-resolution spatial and temporal framework, provides the basis for the study presented
81 here. The taxonomic changes and the evolutionary divergence of the foraminifera in the Uralian
82 and West Tethyan oceans through the Pennsylvanian and early Permian time definitively
83 indicate the emergence of the Precaspian Isthmus and the closure of the connection between
84 the Uralian and Paleo-Tethys oceans on both the northern and mid-east sides of Pangea (Fig. 1).
85 The mid-late Artinskian closure of the connection between the Uralian--Paleo-Tethyan
86 oceans utilizing fusulinids data has been proposed previously (Chuvashov, 1998; Leven, 2004;
87 Ross, 1967b;). Shi and Waterhouse (2010) interpreted this as a significant event that enhanced
88 the cooling of the paleo-Arctic ocean which had already been occurring due to Pangaea's
89 northward drift throughout the Permian. However, this closure was considered insignificant in
90 paleoclimatic models because of the lack of the temporal connection with any known climatic
91 event ( Lowry et al., 2014; Montanez and Poulsen, 2013). In this paper we propose and discuss
92 the causal link between the development of the Precaspian Isthmus in-between the Uralian and
93 West Tethyan basins, the profound biotic transformations in the oceans, sea-level changes, the
94 decline of the atmospheric CO2 concentration, and the expansion of the Gondwanan ice sheet
95 during the early-middle Sakmarian.
96 2. Data
97 In this study the foraminiferal data was compiled from 252 literature sources (see supplemental
98 references list) covering the regions along the Ural ocean and the northern margins of the
99 Paleo-Tethys ocean (Fig. 1). The data from the author’s foraminifera collections was also used.
100 Taxonomy was carefully considered and publications with paleontological plates were
101 evaluated. Some publications without plates were also included in the database where the
102 taxonomy appeared reliable. The main goal of the taxonomic evaluation was to develop the
103 database with internally consistent taxonomy for each analyzed region and chronostratigraphic
104 time slice.
105 The data at species level and at generic level was analyzed separately. Foraminifera are
106 very sensitive to environmental changes, particularly at species level. The cutoff of the Ural-
107 Tethys passage would undoubtedly have been expressed in the dramatic changes of the
108 environments and therefore WWBF taxonomy (Davydov and Cozar, 2018, in press). At genus
109 level, those changes are not that apparent as many genera existed at that time and were
110 evolving independently in completely isolated basins for a long time (Collins et al., 1996;
111 Davydov, 2014; Mamet, 1977; Ross, 1995;).
112 Although some of the paleogeographic models suggest a very early UPTS closure in
113 Early-Middle Pennsylvanian time (Lawver et al., 2011; Stampfli et al., 2013), we started to
114 compile the data from the late Gzhelian-Asselian to the Kungurian, as the Bashkirian-Gzhelian
115 fusulinids within the UPTS regions are clearly very similar (Davydov and Cozar, 2018, in press).
116 Most of the existing models propose the UPTS closure during the Kungurian. Some
117 paleogeographic models show the existence of a permanent UPTS during the entire Permian
118 (Blakey, 2013; Domeier and Torsvik, 2014; Golonka, 2011; Scotese, 2015;). These regions during
119 Cisuralian were located within the tropics—subtropics (Blakey, 2013; Davydov, 2014; Domeier
120 and Torsvik, 2014; Golonka, 2011; Scotese, 2015). However, no typical warm-water
121 foraminifera such as fusulinids have ever been found in Kungurian and Roadian seas in the
122 Precaspian, in the Southern Ural, and in the Russian Platform ( Filimonova et al., 2015; Gorsky
123 and Kalmykova, 1986; Sukhov, 2003). The youngest WWBF in these regions are known only
124 from the lower Kungurian in the north-central Preural, where they are rare and of very low
125 diversity (Zolotova and Baryshnikov, 1978).
126 The WWBF data have been compiled along the Ural-Tethyan passage (Fig. 1) which
127 includes the Carnic Alps (CA) (1), Taurids (2), Donets Basin (3), Darvaz (4), South Tian-Shan’ and
128 the northern margin of Tarim microcontinent (5), northern and eastern Precaspian (6-7), the
129 Southern Ural (8), Russian Platform (9), the Central Ural (10) and the Timan-Pechora Basin (11).
130 3. Methods
131 The Late Paleozoic foraminifera FODs (first occurrence datum) and LODs (last occurrence
132 datum) were calibrated using the exceptionally accurate, quantitative biostratigraphic and
133 radioisotopic scale that has been developed in the Ural and surrounding regions (Schmitz and
134 Davydov, 2012). Therefore, the accurate timing of the taxonomic changes associated with the
135 acme of the Precaspian Isthmus closure can be established. All the regions involved in the
136 analyses, occur within the paleo-tropics sub-tropics and therefore the latitudinal differences
137 played no role or minor role in controlling of the distribution of foraminifera in the studied
138 regions. The highest plausible resolution to resolve the time calibration of the foraminiferal
139 events has been employed in this study. The author is confident that the position of the stages
140 and zonal boundaries are constrained with a 0.1-0.2 Myr resolution. The number and precision
141 of the radiometric ages, the number of the bioevents in the composite section (CONOP9), and a
142 direct link to an eccentricity-tuned cyclostratigraphy result in a ca. 0.1–Myr resolution for the
143 chronostratigraphic model through most of this time period (Schmitz and Davydov, 2012).
144 The foraminiferal taxonomic data was analyzed using the PAST v.3.0 software (Hammer
145 et al., 2001). The binary (i.e., presence/absence) matrices for each region include two types: 1)
146 species only; 2) genera only. Probabilistic Raup-Crick similarity/dissimilarity indices were used
147 to calculate the matrices (Hammer and Harper, 2006). More details on the advantages and
148 disadvantages of these different types of the indices applied to WWBF can be found in an
149 earlier published paper (Davydov and Cozar, 2018, in press).
150 4. Results
151 Results of the Raup and Crick probabilistic similarity index (PSI) at species level are given in
152 Table 1, and the data at genus level can be found in supplementary Table 2.
153 The PSI is sensitive to the lack of taxa in any of compared regions and thus, taxa that are
154 geographically widespread do not have a disproportionate effect on the measurement of
155 similarity. The PSI provides the opportunity to measure statistically significant similarity and
156 dissimilarity at the 95% confidence level and is less affected by sampling bias.
157 Two clusters are recognized among WWBF at both species and genus levels during the
158 early-middle Asselian (Figs. 2-4, Tables 1-2). The Paleo-Arctic cluster (Boreal Realm) includes the
159 Russian Platform (9), the central and northern Ural (10) and Timan-Pechora region (11). The
160 Tethyan cluster is comprised of the Carnic Alps (1), Taurids (2), Donets Basin (3), Darvaz (4),
161 South Tian-Shan (5), Precaspian (6-7) and the Southern Ural (8). The Donets Basin was involved
162 in the analyses only for early-middle and late Asselian time-slices. By the early Sakmarian, the
163 Precaspian and the Southern Ural regions became part of the Paleo-Arctic cluster.
164 In the early-middle Asselian the PSI of Paleo-Arctic and Tethyan clusters at species level
165 is 0.2 and increases up to 0.45-0.48 in the late Asselian (Fig. 5). Beginning with the early
166 Sakmarian, the PSI between the Boreal and Tethyan clusters at species level is zero, i.e. the
167 WWBF of these clusters are dissimilar in the post-Asselian time (Fig. 5). The PSI at genus level
168 shows similar tendencies, except the absolute values of the PSI are significantly higher. During
169 early-middle Asselian the PSI at genus level is 0.48, during the late Asselian it increases to 0.7-
170 0.72 (Table 2). Starting in the early Sakmarian the PSI drops drastically to 0.25 and after that,
171 the PSI progressively goes down from 0.25 in the early Sakmarian to 0.1 towards the end of the
172 Artinskian (Fig. 5). Some similarity between the two clusters at genus level can be explained by
173 the fact that the genera ranges are much more prolonged than the ranges of species.
174 Beginning in the early Sakmarian, the Precaspian and the Southern Ural regions became
175 a part of the Paleo-Arctic cluster, the PSI of the latter and the rest of the Paleo-Arctic regions
176 reaching 1.0 (Fig. 5, table1-2). The PSI value remains the same during the entire Sakmarian-
177 Artinskian time.
178 5. Discussion
179 5.1. Paleo-Tethys—Paleo-Arctic Seaway closure
180 5.1.1 Dynamics of taxonomic similarity changes in Paleo-Tethyan and Paleo-Arctic through the
181 Cisuralian time.
182 Four major realms are recognized in the Carboniferous-Permian within the distribution pattern
183 of the Late Paleozoic foraminifera (Ross, 1995) (Fig. 1). The largest realm is the Tethyan, which
184 extended from the tropics in the China blocks to the tropics of the eastern margin of Pangea
185 and the northern margin of Gondwana. The second realm, Boreal or Ural-Franklinian, embraces
186 the subtropics in the northern margins of Pangea. The third realm, commonly called ‘North
187 American’ or ‘Midcontinent-Andean’, is positioned in the tropics and subtropics along the
188 western margin of Pangea. The fourth realm, named ‘Panthalassan’ or ‘Sonomia’, is not well
189 defined. It includes a series of terranes and sea-mounts within Paleo-Pacific, i.e. parts of Japan,
190 the Russian Far East, Cache-Creek, British Columbia, Koryakia, New Zealand, and S. Peru (Fig. 1).
191 The main purpose of this study is the comparison of the Boreal and Tethyan realms. The
192 taxonomic composition of these realms was quite similar during most of the Late Paleozoic, due
193 to the free connection of Paleo-Arctic and Paleo-Tethys oceans (Fig. 6). Although, the WWBF of
194 Russian Platform, the Ural and Timan Pechora formed a separate cluster (Figs. 2-4), they reveal
195 considerable similarity with the WWBF of the Tethyan realm regions during Asselian time,
196 especially at genus level (Figs. 3,5). At that time the WWBF in the Donets Basin, the Precaspian
197 and the Southern Ural belonged to the faunas of Tethyan affinity. The taxonomic diversity of
198 the WWBF within the Gzhelian-Asselian transition reached the maximum recorded for the
199 entire Late Paleozoic and remained very high during the Asselian, except for a small decrease in
200 the diversity in the middle Asselian (Fig. 7) (Davydov, 2014; Groves and Wang, 2009).
201 The major event that drastically changed the similarity among the analyzed regions over
202 an interval of less than 0.5 Myr occurred within the Asselian-Sakmarian transition (Fig. 7). These
203 changes were reported earlier in the Russian literature and some Russian scientists (Bensh,
204 1962; Rauser-Chernousova, 1965) considered the position of the Carboniferous-Permian
205 boundary at the base of the Sakmarian because of these severe changes. Marine
206 sedimentation ceased in the Donets Basin at the end of the Asselian.
207 During the Sakmarian and through the end of the Artinskian the species and genera of
208 the WWBF of the Precaspian and the Southern Ural had a high degree of similarity with those of
209 the Central Ural, Russian Platform and Timan Pechora (Fig. 5). At the same time, the similarity
210 between the WWBF of the Tethyan and Boreal realms dropped twice at genus level and almost
211 to zero at species level (Fig. 5). At the Asselian-Sakmarian transition the global diversity of
212 WWBF at both species and genus levels dropped threefold (Davydov, 2014; Groves and Wang,
213 2009). During the Sakmarian and Artinskian, the similarity between the Tethyan and Boreal
214 WWBF at species level remained close to zero. At genus level, the similarity index had been
215 progressively falling from 0.25 to 0.1 through Sakmarian-Artinskian boundary, and towards the
216 end of the Artinskian dropped below 0.1 (Fig. 5).
217 It is obvious from the discussion above that the distribution of the WWBF throughout
218 the Asselian within the Paleo-Artic and the Ural-Precaspian shelves was not limited by any
219 physical or climatic factors. Starting in the Sakmarian, the WWBF of the Paleo-Tethys shelves
220 were isolated from those of the Paleo-Artic and the faunas of Paleo-Artic and the Ural-
221 Precaspian, developed as a single unified biome. Such a sudden event in the separation of the
222 Paleo-Arctic and Paleo-Tethyan faunas in the subtropics was evidently caused by the
223 appearance of the physical barrier between the Precaspian Basin, the southernmost region of
224 the Paleo-Arctic, and the Paleo-Tethys regions. The presence of this physical barrier is well
225 expressed in the records of the WWBF from the regions closest to the Precaspian-Southern
226 Ural, such as Darvaz, S. Tian-Shan’ and Taurides (Figs. 1, 6). The data from Turan Platform,
227 which was a part of the Precaspian Basin until the late Asselian, is consistent with this
228 observation (Akramkhodjaev et al., 1981; Uzakov, 1996; Dronov et al., 1997; Pronin et al., 2011;
229 Volozh et al., 2011, 2011).
230 5.2 Evolutionary and ecological proxies of the WWBF of the Uralian-Tethyan passage
231 closure.
232 The UPTS passage was the only way for the exchange of the WWBF between the Paleo-
233 Arctic and Paleo-Tethys during the Late Paleozoic (Fig. 1A). Thus, the timing of the
234 disappearance of the Tethyan taxa in the Precaspian and in the Ural and the shift in the
235 provinciality from the Tethyan affinity to the Boreal would be the signs of the emergence of the
236 Precaspian Isthmus (Fig. 6)
237 The migration of the WWBF between the Paleo-Tethyan and Paleo-Arctic oceans
238 occurred in only one direction, from south to north. This is consistent with the distribution of
239 the marine faunas along the temperature latitudinal gradient from the high-diversity
240 assemblages in the Paleo-Tethys to the low-diversity assemblages in the shelves of higher
241 latitudes (Davydov, 1997; Davydov and Arefifard, 2013; Jablonski et al., 2006). Most of the
242 fusulinid genera and many species, which dispersed into the Paleo-Arctic ocean, originated in
243 the Paleo-Tethys (Davydov, 1986; Davydov et al., 2001; Izotova, 1985; Izotova and Vevel, 1998;
244 Nilsson and Davydov, 1997). The distribution and provincialism of the WWBF were largely
245 controlled by climate along the temperature latitudinal gradient (Davydov, 2014; Rind, 1998).
246 WWBF provide a particularly sensitive index of climate changes within the marginal conditions
247 at the transition from subtropics to temperate mid-latitudes, such as the shelves of the Paleo-
248 Arctic ocean (Davydov and Arefifard, 2013). During the Late Paleozoic there were several waves
249 of change in the biodiversity and provinciality of the WWBF, associated with global climate
250 fluctuations (Fig. 7). During episodes of global warming (climatic optimums), the WWBF for the
251 given latitude and depth reached their maximum diversity and world-wide distribution, with
252 tropical taxa migrating to the higher latitudes. For example, Eofusulina originated in the
253 Vereiyan (the early Moscovian) in the Paleo-Tethys and migrated into the Paleo-Arctic
254 (Greenland, Canadian Arctic) during the Kashirian (the late early Moscovian). The late Gzhelian-
255 early Asselian Likharevites and Asselian Sphaeroschwagerina and Biwaella migrated in the late
256 Asselian as far as Spitsbergen, North Greenland and the Canadian Arctic (Nilsson and Davydov,
257 1992, 1997; Rui Lin et al., 1994); and personal data of the author). By contrast, global cooling
258 led to the disappearance of the foraminiferal fauna starting at higher and moving to lower
259 latitudes, their stepwise extinction, increasing provincialism, and to the preferential survival of
260 euryfacial faunas (Davydov and Arefifard, 2013).
261 During the Moscovian-Gzhelian and the entire Asselian the WWBF in the Precaspian,
262 Donets Basin and the Southern Ural were generally of Tethyan affinity with many common
263 species and genera known from the other Tethyan regions ( Akhmetshina et al., 2013; Davydov,
264 1986, 1992; Izotova, 1985; Nikolaev, 2011; Leven and Scherbovich, 1978; Scherbovich, 1969).
265 The WWBF taxa of the Boreal affinity in the Precaspian, Donets Basin and the Southern Ural
266 were very rare during this time. From the beginning of the Sakmarian, the fauna of the Boreal
267 affinity predominated in the Precaspian and the Southern Ural. Only a small number of species
268 of Tethyan affinity, i.e., few species of Sakmarella, Darvasites and Rugosofusulina, described
269 from Darvaz (Leven and Shcherbovich, 1980), were found only in the earliest Sakmarian in the
270 very southern part of the Southern Ural (Davydov, 1986). The Tethyan Sakmarella, Darvasites
271 and Rugosofusulina were found in only one (the lowermost) horizon of the Sakmarian, in the
272 Southern Ural (Davydov, 1986). From the beginning of Sakmarian the WWBF of the Precaspian
273 and southern Ural were exclusively of Boreal affinity. And again, these sharp changes in
274 biogeography signify the physical separation of the Precaspian and Southern Ural regions from
275 the Tethyan shelves at the Asselian-Sakmarian transition.
276 5.3 Olistostrome and seismite deposits and the oceanic currents within the Late Paleozoic in
277 the Southern Ural.
278 Olistostromes and seismites occur widely in ancient orogenic belts and in exhumed subduction–
279 accretion complexes. In latter type of orogenic belt, the temporal and spatial distribution of
280 different types of olistostromes commonly indicate different tectonic stages over period of 10+
281 Myrs from the early rift–drift to the later subduction, collision, and orogenic exhumation
282 (Ettensohn et al., 2002; Festa et al., 2016). Generally, olistostromes are the fundamental
283 markers of tectonic events and their study is a powerful tool for the basin analysis at various
284 scales (Festa et al., 2016). Hence, the evaluation of distribution of the olistostromes and
285 seismites in the area of the Precaspian Isthmus may help in understanding of the dynamics of
286 the closure. Unfortunately, only one area, i.e., Southern Ural, is available for this evaluation.
287 The scarсe published records of the lithostratigraphy from the subsurface of the Precaspian
288 have prevented the analyses of the olistostromes there. The regions immediately to the south
289 from the Precaspian Isthmus are either not exposed or occur far from the collision area
290 (Figs.1,6,8).
291 An olistostrome is a sedimentary deposit composed of a chaotic mass of heterogeneous
292 material, such as blocks of consolidated and unconsolidated sediments with siliciclastic or
293 carbonate matrix mud, that accumulates as a semifluid body by submarine gravity sliding or
294 slumping of the unconsolidated sediments. Olistostromes are well preserved in paleo-active
295 margins such as Southern Ural foredeep. Causative mechanisms for gravitational instability in
296 collisional and intra-collisional settings are mostly seismic shocks originating from thrust
297 faulting (Festa et al., 2016). The seismite, as opposed to olistostromes, referred only to
298 stratigraphic units containing sedimentary structures produced by seismic shaking and is an in
299 situ breccia (Ettensohn et al., 2002; McCalpin, 2009). Thus, the occurrence of olistostromes and
300 seismites is indicative of the seismic activity and dynamic orogeny that are concomitant to the
301 collision processes in the Southern Ural and could be projected to the Precaspian Basin (Mizens,
302 1997; Puchkov, 2010).
303 The olistostromes are broadly distributed and well known in the Southern Ural, where
304 they have been thoroughly studied and described (Keller, 1949; Khvorova, 1961; Mizens, 1997,
305 2002). Two types of the olistostromes are designated in the Southern Ural. The first one occurs
306 as proximal facies of the poorly sorted mass of consolidated, sharp or poorly rounded boulders
307 and blocks up to 100-150 meters in size, conglomerate-breccia and conglomerates. These clasts
308 consisting of shallow-water limestone touch each other. A small amount of the silty-
309 carbonaceous matrix fills the space between the clasts (Khvorova, 1961; Mizens, 1997). This
310 type of olistostrome lacks fossils in the matrix and, perhaps, belongs to the olistostromal carpet
311 in the classification of Festa et al (2016). More distal olistostromes consist of matrix-supported,
312 unconsolidated carbonate and siliciclastics material with very large to small, sharp to rounded
313 blocks, pebbles, and unconsolidated carbonate or siliciclastic clasts of different sizes. The matrix
314 and clasts are generally of the same composition and both contain abundance of fossils of the
315 same taxa (Khvorova, 1961). This type of olistostrome belongs to the category of precursory
316 olistostromes (Festa et al., 2016).
317 Horizons of both precursory olistostromes and olistostromal carpet are unevenly
318 distributed within the Late Paleozoic succession in the Southern Ural (Fig. 7). The olistostromes
319 first appear there in the upper Moscovian (Khvorova, 1961), which is consistent with the initial
320 stage of rigid (hard) collision of Kazakhstania and the Ural and the initiation of the Uralian
321 orogeny (Puchkov, 2010). The olistostromes are frequent and sometimes thick in the upper
322 Moscovian, Kasimovian and early-middle Gzhelian (Khvorova, 1961; Mizens, 1997). The
323 uppermost horizon of the precursory olistostrome in the Carboniferous is recorded at the
324 beginning of the Orenburgian stage (the late Gzhelian in the International Scale) (Davydov,
325 1986; Khvorova, 1961). This late Gzhelian horizon can be traced in the distance of over 600 km
326 from Aidaralash Creek in Aqtobe region in Kazakhstan to Usolka river in the northern part of the
327 Southern Ural in Bashkortostan (Mizens, 1997). The end of the Gzhelian and early-middle
328 Asselian was quiet, with no olistostromes recorded. The beginning of the late Asselian is again
329 associates with the massive deposition of olistostromes, which were especially abundant in the
330 southernmost exposed part of the Southern Ural (Khvorova, 1961; Mizens, 1997). In
331 Kondurovsky section, which is the type of the Sakmarian Stage, two horizons of specific
332 sediments, named Kurmaya breccia, are described in many publications (Keller, 1949;
333 Khvorova, 1961; Mizens, 2002). These distal facies formed from the micritic limestone matrix
334 with the submerged clasts of micritic limestone (1-5 cm in size) of different color from very dark
335 to light-grey (Fig. 8). This type of rock, perhaps, could be interpreted as seismites, as both the
336 matrix and clasts are of the local origin and of same composition (Ettensohn et al., 2002). The
337 occurrence of tsunami deposits in the Late Paleozoic of Zalair Zone of the Ural has been
338 proposed as well (Keller, 1949; Khvorova, 1961).
339 During the Sakmarian and through the Artinskian and Kungurian, no olistostromes have
340 been recognized in the Southern Ural (Khvorova, 1961; Mizens, 1997). The olistostromes of this
341 age were documented only in the Central and Northern Ural, which is consistent with the
342 observed diachronous shift in the granitic magmatism and the collision area of Kazakhstania
343 and the Ural towards the north (Puchkov, 2010). In the southern periphery of the Precaspian
344 Basin, in the Tengiz-Karaton Dom structure and other micro-platforms, the carbonate and
345 mixed carbonate-siliciclastic succession extended up to the Bashkirian. In the surrounding
346 platforms areas the successions extended up to the Asselian (Abilkhasimov, 2016). In the very
347 south of the Emba zone (Buzachi Peninsula) marine sedimentation ended in the late Asselian
348 (Pronin et al., 1997). Pyroclastic material and volcanic tuffs are recognized and widely
349 distributed in the lower Permian there (Abilkhasimov, 2016). From the beginning of the
350 Sakmarian neither seismic activities nor orogeny occur in the area of the Southern Ural and
351 Emba zone in the southern periphery of the Precaspian Basin (Fig. 6) (Abilkhasimov, 2016).
352 Beginning in the Artinskian in the southern periphery of the Precaspian Basins, fluvial fan
353 deposits are documented (Bakirov et al., 1978; Fedorenko and Miletenko, 2002; Rogova and
354 and Pugacheva, 1983), suggesting the development of the weak orogeny along the border
355 between the southern Precaspian Basin and Scythian-Turan plates (Fig. 6).
356 The pattern of oceanic currents in the Southern Ural and Precaspian Basin may also help
357 clarify when the emergence of the Precaspian Isthmus occurred. The northern direction of the
358 oceanic currents in the Southern Ural has been reported in several publications (Bezhaev, 1968;
359 Keller, 1949; Khvorova, 1961; Mizens, 1997, 2002). During the Late Paleozoic, the clastic
360 sources in the Preuralian foredeep were to the east (in the present day coordinates) from the
361 Uraltau and Magnitogorsk Arc (Mizens, 1997; Puchkov, 2010). This material was delivered into
362 the foredeep by a series of paleo-rivers (Khvorova, 1961). The submarine deltaic fan deposits
363 along the mountains are supposedly oriented perpendicular to the mountains. In the Ural this
364 type of the submarine fan conglomerates in the shallow part are oriented perpendicular to the
365 mountains, i.e. from east to west (in the present day coordinates), but in the deeper part of the
366 foredeep they curve and are oriented towards the north-western and northern direction (in the
367 present day coordinates) (Fig. 6) (Khvorova, 1961; Mizens, 1997). Besides, the data on the
368 orientation of the deep-water currents in the foredeep has been obtained from the analyses of
369 the shape and distribution of the ocean paleocurrents features, such as small-scale cross-
370 bedding and ripples in the Late Paleozoic flysh successions. The cross-bedding and ripples also
371 suggest the northern direction of the oceanic currents (in the present day coordinates) during
372 Moscovian-Asselian time ( Bezhaev, 1968; Keller, 1949; Khvorova, 1961; Mizens, 1997).
373 However, beginning in the Sakmarian time the orientation of the ripples and cross-bedded
374 lamination of the sediments suggest southern direction of the oceanic currents within the
375 Uralian foredeep (Mizens, 1997)
376 5.4 The Precaspian and Scythian-Turan plate paleotectonics
377 According to the majority of publications (Cocks and Torsvik, 2007; Golonka, 2007; Nikishin et
378 al., 1996; Puchkov, 2000, 2010; Ziegler, 1989; Zonenshain et al., 1990), the Paleo-Tethys—
379 Paleo-Arctic active passage was closed in Kungurian. The other model suggests that a shallow-
380 water connection existed throughout the entire Permian (Blakey, 2013; Domeier and Torsvik,
381 2014; Chumakov and Semikhatov, 2004; Fedorenko and Miletenko, 2002; Kaz'min and and
382 Natapov, 1998; Scotese, 2015;). The biota the WWBF in the Paleo-Tethys, and Paleo-Arctic
383 basins and key sedimentological features in the Southern Ural suggest that the Paleo-Tethys-
384 Paleo-Arctic connection through the Uralian foredeep lasted through the Asselian with the
385 cutoff of the connection during the Asselian-Sakmarian transition.
386 The data of the subsurface of the areas along the transitional zone between the
387 southern periphery of Precaspian Basin and Scythian-Turan plate is very poor however some
388 assumptions can be made. Most of the models suggest the connection between the Paleo-
389 Arctic and Paleo-Tethys through the Donets—Tuarkyr and the Usturt rift systems
390 (Abilkhasimov, 2016; Afanasenkov et al., 2008; Fedorenko and Miletenko, 2002; Gavrilov, 2011;
391 Khain and Popkov, 2009; Nikishin et al., 2012;). Marine sedimentation in Donets Basin ended in
392 the latest Asselian and the remnants of the basin were filled with the thick succession of salt
393 and other evaporites (Korenevsky et al., 1968). The evaporites of the Kramatorsk formation lack
394 fossils and tentative age proposals vary from the Sakmarian to Kungurian (Volodin, 1993).
395 In the Tuarkyr and Ustyurt rift systems the Upper Paleozoic rocks have been recovered
396 only from the subsurface. The youngest known marine sediments in these regions are Asselian
397 limestone ( Akramkhodjaev et al., 1979; Akramkhodjaev et al., 1981; Maslov et al., 2016). The
398 Asselian carbonates in the region are overlain by the continental late Permian-Triassic
399 sequences (Akramkhodjaev et al., 1979; Gavrilov, 2011). In the area of the connection of the
400 Turan plate and the southern periphery of Precaspian Basin, in the Caspian Sea, the youngest
401 recorded carbonates are Asselian limestone that are unconformably overlain by Mesozoic
402 siliciclastics (Maslov et al., 2016; Pronin et al., 1997). This succession is quite similar to the one
403 in the Buzachi and South Emba regions immediately to the east of the Caspian Sea (Pronin et
404 al., 2011).
405 The most recent reconstructions of the Precaspian Basin and surrounding areas suggest
406 that a narrow rift system within the Turan plate provided a marine connection between the
407 Precaspian Basin and Paleo-Tethys until Kungurian time (Abilkhasimov, 2016) or even later
408 (Fedorenko and Miletenko, 2002). The rift system along the southern slope of the Karpinsky
409 swell that introduced carbonate sedimentation to the Pre-Caucasia and North Caucasus (Kaz'min et
410 al., 2008), emerged much later in the latest Permian time (Letavin A.I. et al., 1994). Although
411 the Precaspian, Southern Ural and the southern part of Russian Platform were still within the
412 subtropics at that time, only temperate foraminifera were found in the Kungurian and post-
413 Kungurian in these regions ( Filimonova et al., 2015; Gusev et al., 1968; Pronina, 1999; Sukhov,
414 2003). This unambiguously suggests direct connection of these regions with the temperate seas
415 of the Paleo-Arctic during the Guadalupian-Lopingian and the lack of a connection with the
416 Paleo-Tethys in post-Sakmarian time.
417 As in the case with the Alleghanian Isthmus (Davydov and Cozar, 2018, in press), the
418 closure of the Paleo-Tethys—Paleo-Arctic passage happened rather quickly, most probably,
419 during an interval of less than 0.5 Myr (Fig. 5). Some elements of the WWBF of the Tethyan
420 affinity still occurred in the earliest Tastubian in the south of the Southern Urals (Aidaralash,
421 Aktobe province) (Davydov, 1986), but rapidly disappeared almost immediately. The fauna of
422 Boreal affinity dominated in the region from Sakmarian through Kungurian and no elements of
423 Tethyan affinity are known in the Precaspian and the Southern Ural or anywhere in the Paleo-
424 Arctic (see the Results chapter for details). This conclusion in accord with the frequent
425 occurrence of olistoliths and seismites in the Uralian foredeep, which suggests the presence of
426 an active tectonic regime until the end of the Asselian in the Southern Ural and the reduction of
427 tectonic activity in the post-Asselian time (Khvorova, 1961; Mizens, 2002). Carbonate
428 sedimentation ended in the late Asselian in the areas to the south and southeast of the
429 southern periphery of the Precaspian Basin in Turan. The widely developed Artinskian
430 submarine fan deposits along the southern periphery of the Precaspian Basin (Abilkhasimov,
431 2016; Fedorenko and Miletenko, 2002) suggest the existence of the Precaspian Isthmus. In the
432 Artinskian the Isthmus was already quite high and delivered significant amount of clastic
433 material to the Precaspian basin (Fig. 6).
434 5.5 Sea-level fluctuations within the Asselian-Sakmarian transition.
435 According to the widely accepted model of the global sea-level fluctuations, the sea-
436 level at the Asselian-Sakmarian transition had dropped and the boundary coincided with a
437 global sequence boundary (Ross and Ross, 1987a). This interpretation is accepted in some
438 subsequent publications ( Golonka and Kiessling, 2002; Haq and Schutter, 2008; Rygel et al.,
439 2008). However, other authors proposed the coincidence of the Asselian-Sakmarian boundary
440 with a global flooding surface ( Boardman, Darwin R., II et al., 2009; Davydov et al., 1997a;).
441 The model of Ross and Ross (1987) was developed from the integration of the Southern
442 Ural and West Texas data based on the commonly accepted fusulinid-ammonid correlation of
443 these regions ( Furnish and Glenister, 1971; Jin et al., 1994, 1994; Ross, 1967). In this
444 correlation the middle Asselian of the Southern Ural corresponds to the Neal Ranch Formation
445 of Texas and the upper Asselian (Shikhanian) corresponds to the gap between the Neal Ranch
446 and Lenox Hill Formations of Texas. The latter formation was correlated with the entire
447 Sakmarian (Ross and Ross, 1987a). The most recent updates on the correlation of these
448 successions, involving new fusulinid and conodont biostratigraphic and taxonomic data the
449 from Ural, Nevada and Texas ( Chernykh, 2006; Chuvashov et al., 2002; Davydov et al., 1997a,
450 b; Wardlaw and Davydov, 2000;), provided a quite different correlation. The Neal Ranch
451 Formation is correlated with the upper Asselian and lower Sakmarian of the Southern Ural and
452 the Lenox Hill Formation – with the entire Artinskian, probably, including the lower Kungurian.
453 Moreover, it was clarified that the Asselian-Sakmarian boundary in both Texas and the
454 Southern Ural coincided with a flooding surface (Davydov et al., 1997a,b; Davydov et al., 2003;
455 Wardlaw and Davydov, 2000). It is now clear that the interpretation of the Kurmaya seismites
456 horizons as a conglomerate associated with sequence boundary within the Asselian-Sakmarian
457 transition at the Sakmarian type, Kondurovsky section in the Southern Ural (Ross and Ross,
458 1987), mislead the latter authors with the global correlation and sequence stratigraphy.
459 Refining the biostratigraphy of the conodonts and fusulinids in the Southern Ural and
460 the other regions provided the precise correlation of the Asselian-Sakmarian transition of the
461 Southern Ural with that of the Canadian Arctic, Iran, Nevada, New Mexico, Oklahoma, Texas,
462 Spitsbergen, Barents Sea, North and South China. The drop in global sea-level and the
463 occurrence of the associated sequence boundary occurred sometime within the early to middle
464 Tastubian (early Sakmarian) ( Beauchamp et al., 2009; Boardman, Darwin R., II et al., 2009;
465 Chernykh, 2006; Davydov, 1995, 1997a, b; Kozur and Le Mone, 1995; Leven and Gorgij, 2011;
466 Ehrenberg et al., 2000; Nilsson and Davydov, 1997; Wardlaw and Davydov, 2000).
467 The beginning of the Sakmarian was associated with a global sea level high stand. That is
468 opposite to what happened at the beginning of the Bashkirian glaciation, where the emergence
469 of the Alleghanian Isthmus corresponds with the one of the largest global sea level drops in the
470 Phanerozoic (Davydov and Cozar, 2018, in press; Ross and Ross, 1987b) Therefore, the global
471 sea-level fluctuations within the Asselian-Sakmarian transition did not coincide with the
472 emergence and development of the Precaspian Isthmus. The UPTS closure was essentially
473 caused by a tectonic event, associated with the active tectonic collisions of Kazakhstania, the
474 East Ural and Magnitogorsk Arc with the southern part of Russian Platform and Karpinsky Swell
475 at that time (Fig. 6). The event is best documented by the occurrence of the olistolith and
476 seismite horizons in the Southern Ural and by the termination of marine sedimentation at the
477 end of the Asselian in the Donets Basin and the southern periphery of the Precaspian Basin and
478 in the surrounding areas in the Turan and Scythian Platforms ( Afanasenkov et al., 2008;
479 Nikishin et al., 1996; Pronin et al., 1997). The connection between the Paleo-Tethys and the
480 Paleo-Arctic oceans during the rest of the Permian time was never re-established.
481 5.6 Seaway closure and climate
482 The chronostratigraphic constraints on the age of glacial events in the Permian are poorly
483 established and still in a state of flux. The new CA-IDTIMS data (Metcalfe et al., 2015)
484 significantly changes the chronostratigraphic framework of the Guadalupian-Lopingian glacial
485 episodes (P3 and P4 glaciations). The chronostratigraphic records from the high-latitude regions
486 of Gondwana produce quite a controversial picture concerning the glacial episodes in the
487 Gzhelian, Asselian and Sakmarian. The early Permian time is considered the apex of the late
488 Paleozoic Ice Age with the glaciations extending from the Gzhelian through the Asselian and
489 Sakmarian (Isbell et al., 2013). But the chronostratigraphy of the glacial episodes remains vague
490 given the paucity of the paleontological and geochronological constraints (Birgenheier et al.,
491 2009; Fielding et al., 2008; Mory et al., 2008). The latest paleontological and paleoecological
492 proxies link the early Permian glaciation (P1) in Australia to only the early Sakmarian (Haig et
493 al., 2014). That is consistent with the low value of the atmospheric carbon dioxide at this time
494 (Foster et al., 2017), which corresponds with the glacial episode in the early Sakmarian. The
495 significant rise of the CO2 and the corresponding global warming episode (Montanez and
496 Poulsen, 2013), occurred in the late Sakmarian (Fig. 7). The data on the carbon and oxygen
497 stable isotopes has been also obtained recently in the Southern Ural, from the type section of
498 the Sakmarian, the Kondurovsky section, and from the GGSP of the Sakmarian Stage at the
499 Usolka section (Zeng et al., 2012). The data reveals a significant shift of δ13C towards the
500 positive values in the early Sakmarian and back to the lighter isotopes in the late Sakmarian.
501 The data on the geographic extension of the Late Paleozoic glaciations (Isbell et al., 2012)
502 implies that the early Sakmarian glaciation was the largest within the Permian (Fielding et al.,
503 2008; Isbell et al., 2012).
504 The onset of Sakmarian P1 glaciation (Haig et al., 2014) coincided with the appearance
505 of the Precaspian Isthmus (Fig. 11). The emergence of the isthmus drastically changed the
506 pattern of the global ocean circulation similar to one that occurred after the appearance of the
507 Alleghanian Isthmus (Davydov and Cozar, 2018, in press; Saltzman, 2003). The changes
508 associated with the appearance of the Precaspian Isthmus are consistent with the scenario
509 proposed in the model of Rheic-Paleo-Tethys passage closure during the Serpukhovian-
510 Bashkirian transition (Smith and Read, 2000; Davydov and Cozar, 2018, in press; Montanez and
511 Poulsen, 2013). Evidently, the development of Precaspian Isthmus lead to the major
512 modification of the oceanic currents within the northern Paleo-Tethys, reorganization of overall
513 thermal regime of the atmosphere, the evolution of the climate and biota of the Earth.
514 The global oceanic circulation is often considered as one of the major factors controlling
515 the global climate (Rahmstorf, 2002). The final closure of the Central American Seaway and the
516 appearance of Panama Isthmus, according to some models, induced an increased poleward salt
517 and heat transport and intensified moisture supply to the northern high latitudes, which
518 resulted in the build of the Northern Hemisphere glaciation (Bartoli et al., 2011; Haug and
519 Tiedemann, 1998; Bartoli et al., 2005). The opening of the Drake Passage in the late Eocene
520 lead to the establishment of the Antarctic Circumpolar Current, that changed the ocean
521 circulation, caused water warming and enhanced precipitation in the Northern Hemisphere,
522 which in turn enhanced silicate weathering and CO2 drawdown and resulted in the
523 development of a large-scale ice sheet in Antarctica (Elsworth et al., 2017). Perhaps, the latter
524 model of the change of the ocean water circulation in the Paleo-Tethys is applicable to the case
525 of the circulation of the oceanic currents between the Paleo-Arctic and Paleo-Tethys. The
526 change of the ocean circulation in the Paleo-Arctic and Paleo-Tethys oceans would have caused
527 the re-direction of the oceanic warm currents from eastern Tethys toward the Pangea and
528 Gondwana margins. This may have enhanced precipitation and consequently silicate
529 weathering and CO2 drawdown around the Paleo-Tethys and the northern Gondwana shelves.
530 This model is consistent with the CO2 data in the Ural (Zeng et al., 2012), Nevada (Tierney et al.,
531 2008) and the global scale (Montanez et al., 2007). Starting in the Sakmarian, the global
532 biogeographic provincialism progressively increased, with the culmination at the end of the
533 Permian.
534 Recent modeling indicates that orbital forcing alone is not sufficient to cause the waxing
535 and waning of a massive Gondwanan ice sheet (Horton & Poulsen 2009, Horton et al. 2010).
536 The coincidence in the closure of the two main gateways, the Rheic-Paleo-Tethys gateway
537 during the Serpukhovian-Bashkirian transition and the Paleo-Tethys—Paleo-Arctic gateway
538 during the latest Asselian—earliest Sakmarian transition, with the onset of the two major
539 glacial events (Bashkirian and early Sakmarian) in the Late Paleozoic suggests that the closures
540 of the gateways, the appearances of the isthmus and the changes of the global oceanic currents
541 were the major drivers, along with the other less significant factors, in controlling the late
542 Paleozoic climate.
543 6. Conclusions
544 This paper has provided precise age constraints for the closure of the Paleo-Arctic—
545 Paleo-Tethys gateway by utilizing warm-water benthic foraminifera taxonomy and statistical
546 analysis. The major event, that drastically changed WWBF similarity among the analyzed
547 regions, occurred within the Asselian-Sakmarian transition during an interval of less than 0.5
548 Myr. The similarity index between the Tethyan and Boreal WWBF at the species level during the
549 Sakmarian and Artinskian time progressively decreased from 0.25 to 0.1 across the Sakmarian-
550 Artinskian boundary and was less than 0.1 towards the end of the Artinskian. From the
551 beginning of the Sakmarian, the fauna of the Boreal affinity predominated in the Precaspian
552 and the Southern Ural.
553 The temporal distribution of the olistostromes and seismites in the Southern Ural
554 suggests that major orogenic activity, and hence seismicity ceased at the Asselian-Sakmarian
555 transition in the Southern Ural and Scythian-Turan plate along the southern periphery of
556 Precaspian Basin. The fluvial fan deposits in the southern periphery of the Precaspian Basin
557 slope, suggesting the development of a weak orogeny along the border between Precaspian
558 Basin and Scythian-Turan plate.
559 The closure of the Paleo-Arctic--Paleo-Tethys seaway was caused by a tectonic event.
560 The event was associated with the collision of the southeastern part of Russian Platform,
561 Karpinsky Swell, the Southern Ural, Kazakhstania and Scythian-Turan plates along the southern
562 periphery of Precaspian Basin. The connection between the Paleo-Tethys and Paleo-Arctic
563 oceans in the post-Sakmarian time was never re-established.
564 The onset of P1 (early Sakmarian) glaciation coincided with the appearance of the
565 Precaspian Isthmus at the Asselian-Sakmarian transition (Fig. 1). The occurrence of this isthmus
566 was the second major tectonic event in the late Paleozoic, that radically changed the pattern of
567 the circulation of the global ocean, similar to one that occurred after the appearance of the
568 Alleghenian Isthmus. The development of the Precaspian Isthmus lead to the major
569 modification of the oceanic currents within the northern Paleo-Tethys, forcing changes in global
570 oceanic circulation, reorganization of the overall thermal regime of the atmosphere, and
571 consequently impacted climate and biota evolution of the Earth. The coincidence in the closure
572 of the two main gateways, the Rheic-Paleo-Tethys gateway during Serpukhovian-Bashkirian
573 transition and the Paleo-Tethys—Paleo-Arctic gateway during latest Asselian—earliest
574 Sakmarian transition, with the onset of the two major glacial events (Bashkirian and early
575 Sakmarian) in the late Paleozoic suggests that the closures of the gateways, the appearances of
576 the isthmus and the changes of the global oceanic currents were the major drivers for the
577 glaciation along with the other less significant factors controlling the Late Paleozoic climate.
578 Acknowledgments
579 The work was supported by the Ministry of Education and Science of the Russian Federation
580 contract No. 14.Y26.31.0029 in the framework of the Resolution No.220 of the Government of
581 the Russian Federation. The funds from the subsidy allocated to Kazan Federal University for
582 the state assignment #5.2192.2017/4.6 in the sphere of scientific activities and in part from the
583 subsidy of the Russian Government to support the Program of Competitive Growth of Kazan
584 Federal University among the World Leading Academic Centers are highly appreciated. I express
585 gratitude for the help of my great colleague and friend Professor Walter S. Snyder, who
586 carefully edited the text and made useful suggestions. Both W.S. Snyder and G.A. Mizens are
587 thanked for providing the photos of olistolith and seismite from the Southern Ural. The libraries
588 at Boise State University and Florida International University provided access to the literature
589 sources. The edits and suggestions of the reviewers greatly improved the manuscript.
590
591 Figures caption
592 Figure 1. Gzhelian-Asselian (A) and Sakmarian-Artinskian (B) paleogeography and foraminiferal
593 paleobiogeography (modified from Blakey, 2013). In pre-Sakmarian, warm-water benthic
594 foraminifera were freely dispersed from the Paleo-Tethys to Paleo-Arctic through the Uralian-
595 Tethyan Seaway. The emergence of the Precaspian Isthmus at the Asselian-Sakmarian
596 transition completely isolated the Boreal and the Tethyan foraminifera.
597 Figure 2. Multivariate cluster analyses with Raup-Crick probabilistic similarity index (PSI) at the
598 species level. During the early-middle Asselian and late Asselian the WWBF of Donets Basin, the
599 Precaspian and the Southern Ural belonged to the Tethyan Realm and had strong similarity with
600 the WWBF of the other Tethyan regions. From the early Sakmarian through the late Artinskian
601 the WWBF of the Precaspian and the Southern Ural belonged to Boreal affinity and got
602 dissimilar with the fauna of the Tethyan realm.
603 Figure 3. Multivariate cluster analyses performed with the Raup-Crick probabilistic similarity
604 index (PSI) at the genus level. The tendencies in the similarity/dissimilarity of the WWBF of
605 Donets Basin, the Precaspian and the Southern Ural regions and the other regions of Boreal and
606 Tethyan Realms are generally the same as for the PSI at the species level.
607 Figure 4. Non-metric multivariate ordination analysis with the Raup-Crick probabilistic
608 similarity index (PSI) at the species level. The taxonomic composition of the WWBF of the
609 Paleo-Arctic and Tethys significantly overlap during the Asselian, but the taxonomy becomes
610 completely dissimilar during the early Sakmarian through the late Artinskian time.
611 Figure 5. The summary of the similarities dynamics of the Boreal-dominated and Tethyan-
612 dominated WWBF at the species and generic levels from the late Gzhelian through Cisuralian
613 time. PSI - Raup-Creek probabilistic similarity index between Tethyan and Paleo-Arctic basins;
614 PSI A_U - Raup-Crick probabilistic similarity index between the WWBF of paleo-Arctic and Ural-
615 Precaspian. Gzhel., Gzhelian; Kung., Kungurian (part); Earl.—Midl., Early—Middle. The
616 separation of Paleo-Tethyan and Paleo-Arctic oceans occurred at the Asselian--Sakmarian
617 transition due to the collisions of Scythian and Turan microplates with southern Russian
618 Platform, Kazakhstania and the Ural. The similarity between WWBF of the Ural-Paleo-Arctic and
619 Paleo-Tethys increased through the Asselian and dropped drastically at the Asselian-Sakmarian
620 transition. After that, the WWBF of Ural-Paleo-Arctic and Paleo-Tethys oceans become
621 dissimilar. At the same time, the similarity of the WWBF of the Southern Ural--Precaspian and
622 Paleo-Arctic had been slowly increasing during the Asselian and had increased quite sharply at
623 the beginning of the Sakmarian, the fauna of these two areas became completely similar.
624 During the Kungurian the WWBF in the Southern Ural-Precaspian and Paleo-Arctic basins went
625 extinct.
626 Figure 6. Paleogeography of the Ural-Precaspian region and surrounding areas during
627 Moscovian-Asselian and Sakmarian (modified from Fedorenko, O.A. and Miletenko, N.V., 2002).
628 Free oceanic connection between Paleotethys and Paleo-Arctic during Moscovian-Asselian
629 provides extensions of fusulinid’s Tethyan domain over the Precaspian, the Southern Ural, and
630 Donets Basins. At the Asselian-Sakmarian transition after the emergence of Precaspian Isthmus,
631 the fusulinid’s Boreal domain extended into the Southern Ural and Precaspian but were not
632 able to migrate to Tethys. Both areas in Sakmarian through Kungurian were still located within
633 the tropics. Fluvial fans deposits during Moscovian-Asselian exist only along Southern Ural
634 foldbelt and their shape indicate northern direction of the Urals oceanic currents. In Sakmarian
635 and Artinskian the fluvial fans developed along South Ural foldbelt as well as in southern
636 periphery of the Precaspian Basin along the Precaspian Isthmus.
637 Figure 7. Temporal distribution of the warming and cooling events along the North American
638 shelves for the Serpukhovian through the Artinskian, relative diversity of the WWBF of the
639 Western Tethys, sea-water surface temperature, sea-level oscillation, fluctuations of the
640 atmospheric carbon dioxide and the records of the glaciations from Eastern Australia. Green
641 arrows indicate migration events of the WWBF from Tethys to North America, which are
642 associated with the global warming events and an increase of the diversity of foraminifera. The
643 immigration of the WWBF to North America occurred rapidly and abruptly and is associated
644 with the warming events. The FOD’s of many important genera in North America are always
645 delayed in respect to the appearance of these taxa elsewhere. Global cooling events are
646 associated with the decrease of the diversity of the foraminifera, intensive sea-level
647 oscillations, and low atmospheric carbon dioxide value. P2 glacial event in Australia is divided
648 into two glacial episodes that are not recognized as separate yet. The late Artinskian warming
649 spike according to the fusulinid data from Timor and Thailand (Haig et al., 2014; Ueno et al.,
650 2015). US Midcontinent sea-level fluctuation data from (Ross and Ross, 1988). Oxygen δ18O (‰
651 V-SWOM) sea-surface temperature data from (Chen et al., 2016). The question mark in the sea-
652 surface temperature curve represents the potential break in the sedimentation at the Naqing
653 section in South China, that is recognized from fusulinids record (Anonymous, 1994).
654 Atmosphere carbon dioxide data from Foster et al., (2017).
655 The scale is calibrated with the conodont—foraminiferal zonation and U-Pb ages from
656 the Carboniferous-Permian Composite (Davydov et al., 2012). Abbreviation: Desmoin. –
657 Desmoinesian; Msr. – Missourian. Fusulinid zonation: 1, Eostaffella tenebrosa; 2,
658 Pseudoendothyra globosa-Neoarchaediscus parvus; 3, Eostaffella mirifica-Eostaffellina protvae;
659 4, Monotaxinoides transitorius- Plectostaffella acuminulata; 5, Plectostaffella bogdanovkensis;
660 6, Semistaffella variabilis; 7, Pseudostaffella antiqua; 8, Pseudostaffella praegorskyi-
661 Staffellaeformis staffellaeformis; 9, Profusulinella parva-Ozawainella pararhomboidalis; 10,
662 Verella spicata- Aljutovella tikhonovichi; 11, Aljutovella aljutovica; 12, Aljutovella priscoidea; 13,
663 Moellerites lopasnensis- Fusulinella subpulchra; 14, Fusulinella colaniae-Beedeina kamensis; 15,
664 Fusulinella bocki-Fusulina cylindrica; 16, Protriticites ovoides-Praeobsoletes burkemensis; 17,
665 Protriticites pseudomontiparus; 18, Montiparus paramontiparus; 19, Montiparus subcrassulus;
666 20, Rauserites quasiarcticus; 21, Rauserites ofive; 22, Rauserites rossicus; 23, Rauserites
667 stuckenbergi; 24, Jigulites jigulensis; 25, Daixina sokensis; 26, Ultradaixina bosbytauensis-
668 Schwagerina robusta; 27, Sphaeroschwagerina vulgaris aktjubensis; 28, Pseudoschwagerina
669 robusta; 29, Sphaeroschwagerina gigas; 30, Sakmarella moelleri; 31, Schwagerina verneuili; 32,
670 Pseudofusulina urdalensis-Ps. plicatissima; 33, Pseudofusulina concavuta-Ps. pedisequa; 34,
671 Pseudofusulina solida-Parafusulina lutugini; 35, Parafusulina solidissima-P. jenkinsi; 36,
672 Chalaroschwagerina vulgaris; 37, FAD Pamirina; 38, Misellina minor; 39, Misellina parvicostata;
673 40, Armenina pamirensis, FAD Pseudodoliolina.
674 Figure 8. The examples of olistolith and seismite from the Southern Ural.
675 Table 1. Multivariate similarity and distance indexes, Raup-Crick coefficient at species level.
676 Table 2. Multivariate similarity and distance indexes, Raup-Crick coefficient at genus level.
677 Supplementary material
678 Supplementary references used to create the database of warm-water benthic foraminifera
679 distribution.
680
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996
997
310-295 Ma Uralian Foredeep
11 ? 10 12 8 7 9 5 6 4 3
2
1 Center of originations
A
295-290 Ma Uralian Foredeep
? 12 11 10 9 8 5 6-7 4 2
1 Center of originations
B
Analyzed locations: 1, Carnic Alps; 2, Taurids, Turkey; 3, Donets Basin; 4, Darvaz, C. Asia; 5, South Tian-Shan, Central Asia; 6-7, northern and eastern Precaspian; 8, Southern Urals; 9, Russian Platform; 10, Central Urals; 11, Timan-Pechora Basin Fauna distribution Tethyan affinity Boreal affinity
WWBF Realms: Tethyan Boreal North American
Fig. 1 Davydov Cluster analyses, species Raup-Crick coefficient Late Asselian Early Sakmarian, Tastubian
Early-middle Asselian 1 8 9 4 1 5 2 6-7 10 1 1
10 9 1 6-7 8 3 4 5 2 1 100 1 9 8 3 2 4 5 1
10 1 6-7 0.96 1.0 20 100 0.96 90 0.84 0.9 0.88 0.8 0.72 0.80 0.7 100 0.60 0.72 0.6 0.48 100 0.64 Similarity Similarity
Similarity 0.5 0.36 0.56 0.4 0.24 0.48 0.3 0.12 0.40 0.2 100 100 100 0.32 0.00 Cophenetic correlation 0.86 Cophenetic correlation 0.73 Cophenetic correlation 0.95
Late Sakmarian, Sterlitamakian Early Artinskian Late Artinskian Cophenetic correlation 0.83 1 8 9 2 4 1 1 6-7 10 1 8 9 4 5 2 1 1 6-7 1 10 8 9 5 4 1 1 10 6-7 100 100 0.96 30 0.96 predominantly 0.96 100 100 0.84 Tethyan fauna 0.84 0.84 100 0.72 0.72 0.72 0.60 predominantly 0.60 0.60 Boreal fauna 0.48 0.48 Similarity
Similarity 0.48 0.36 8 the regions Similarity with the fusulinids 0.36 100 50 0.36 0.24 of Tethyan 0.24 affinity; since 0.24 0.12 90 0.12 100 Sakmarian the 0.12 0.00 fusulinids of these 100 100 0.00 Cophenetic correlation 0.998 regions belong 0.00 Cophenetic correlation 0.96 Cophenetic correlation 0.96 to Boreal affinity 1, Carnic Alps; 2, Taurids, Turkey; 3, Donets Basin; 4, Darvaz; 5, South Tian-Shan’, Central Asia; 6-7, northern and eastern Precaspian; 8, southern Urals; 9, Russian Platform; 10, Central Urals; 11, Timan-Pechora
Fig. 2 Davydov Cluster analyses (genus), Raup- Crick coefficient Early Sakmarian Early-middle Asselian Late Asselian 1 9 8 4 1 5 2 6-7 10 1 1 9 8 3 4 5 1 2 1 10 1 6-7
9 10 1 5 6-7 8 3 4 1 2 1.0 10 30 60 50 60 0.96 0.9 80 80 0.95 80 50 70 0.90 0.90 0.8 0.84 0.85 0.7 0.78 0.80 0.6 0.72 0.75 90 Similarity
Similarity 0.66 0.5 0.70 Similarity 0.60 0.4 0.65 0.54 0.60 0.3 0.48 100 100 100 0.55 Cophenetic correlation 0.71 0.2 0.42 Cophenetic correlation 0.83 Cophenetic correlation 0.90
Late Sakmarian, Sterlitamakian Early Artinskian Late Artinskian
1 predominantly 1 1 8 9 5 4 1 6-7 8 9 10 1 2 4 1 5 6-7 8 9 10 1 4 2 1 6-7 10 1 70 1.0 1.0 100 Tethyan fauna 40 20 0.96 50 90 80 0.9 0.9 0.88 70 0.8 0.8 0.80 predominantly 0.7 0.7 0.72 Boreal fauna 0.6 0.6 80 0.64 60 8 the regions 0.5 0.5 0.56 Similarity with the fusulinids Similarity 0.4 Similarity 0.4 of Tethyan 0.48 affinity; since 0.3 0.3 0.40 Sakmarian the 0.2 0.32 0.2 fusulinids of these 100 100 100 0.1 regions belong 0.24 0.1 Cophenetic correlation 0.81 Cophenetic correlation 0.95 Cophenetic correlation 0.82 to Boreal affinity 1, Carnic Alps; 2, Taurids, Turkey; 3, Donets Basin; 4, Darvaz; 5, South Tian-Shan’, Central Asia; 6-7, northern and eastern Precaspian; 8, southern Urals; 9, Russian Platform; 10, Central Urals; 11, Timan-Pechora
Fig. 3 Davydov NMMS_species, Raup-Crick coefficient
Early-middle Asselian Late Asselian Early Sakmarian, Tastubian
2 11 11 0.24 0.24 0.32 0.18 5 2 0.18 11 0.24 0.12 0.12 1 0.16 0.06 1 0.06 5 10 4 10 0.08 0.00 3 0.00 5 6-7 4 6-7 9 0.00 4 2 Coordinate 2 -0.06 10 -0.06 Coordinate 2 Coordinate 2 6-7 -0.12 -0.12 -0.08 1 9 -0.18 9 -0.18 -0.16 Precaspian Isthmus -0.24 8 -0.24 3 8 8 -0.24 -0.30 -0.30 -0.3 -0.2 -0.1 0.0 0.1 0.2 0.3 0.4 0.5 -0.24 -0.16 -0.08 0.00 0.08 0.16 0.24 0.32 -0.40 -0.32 -0.24 -0.16 -0.08 0.00 0.08 0.16 0.24 0.32 Coordinate 1 Coordinate 1 Coordinate 1
Late Sakmarian, Sterlitamakian Early Artinskian Late Artinskian predominantly 5 0.36 2 Tethyan fauna 11 0.32 0.12 4 0.30 Precaspian Isthmus 0.24 0.06 10 0.24 9 predominantly 0.16 0.00 11 8 Boreal fauna 0.18 Precaspian Isthmus -0.06 0.12 10 0.08 6-7 Precaspian Isthmus 11 -0.12 0.06 6-7 10 0.00 8 the regions Coordinate 2 Coordinate 2 Coordinate 2 4 -0.18 0.00 5 8 9 -0.08 1 with the fusulinids 4 -0.24 -0.06 of Tethyan 1 -0.16 6-7 9 2 -0.30 affinity; since -0.12 -0.24 Sakmarian the 8 -0.36 1 -0.18 fusulinids of these -0.48 -0.40 -0.32 -0.24 -0.16 -0.08 0.00 0.08 0.16 0.24 -0.40 -0.32 -0.24 -0.16 -0.08 0.00 0.08 0.16 0.24 -0.48 -0.40 -0.32 -0.24 -0.16 -0.08 0.00 0.08 0.16 0.24 regions belong Coordinate 1 Coordinate 1 Coordinate 1 to Boreal affinity 1, Carnic Alps; 2, Taurids, Turkey; 3, Donets Basin; 4, Darvaz; 5, South Tian-Shan’, Central Asia; 6-7, northern and eastern Precaspian; 8, southern Urals; 9, Russian Platform; 10, Central Urals; 11, Timan-Pechora
Fig. 4 Davydov 1.0
0.9
0.8 Arctic vs Tethys 0.7 species 0.6 genera Arctic vs Urals-Precaspian 0.5 species
Similarity 0.4 collision event 0.3
0.2 WWBF extinction in Boreal Realm
0.1
0 Late Earl.-Midl. Late Early Late Early Late Early Gzhel. Asselian Sakmarian Artinskian Kung.
300 295 290 285 Age (Ma) International Geologic Time Scale Fig. 5 Davydov 38 42 48 54 60 66 72 78 84 90 96 100 28 TIC RC OA KOK 28 LE PA KHM 24 N U TPB F PBA 24 R I M TIM A E U T 20 F
20 M Russian S G A U U Z KCB N F 16 F L C Platform B K KUA N 16 MSB
M 12 P PCB C 12 UST SHB VOR 8 AMD R PA K 8 MNB K DDB C 4 UKM 4 GCM Moscovian-Asselian 0 0 1000 0 42 48 54 60 66 72 78 84 90 96
36 42 48 54 60 66 72 78 84 90 96 100 28 PA Sakmarian WAR NRM 0 1000 28 BDM JGB 24
JNF High mountains 24 KHM Mountains 20 U N F U and plateau B F R I M 20 TIM A CSB Lowland KCB T 16 KUA Lacustrine- E alluvial land U 16 F IN MSB H High salinity lagoone S 12 U STF F R A 12 P Fluvial fan conglomerates T S PCB U AMD Shallow shelf 8 CKK 8 Outer shelf PA - PaleoArctic S KP KAR 4 Bathial basins Volcanic arcs DDB GCM 4 Continental slope Intermauntain depressions UKM and foredeeps 0 ain Ocean (abyssal) basins om Oceanic currents n d 0 thya Te JGB- Junggar-Balkhash Basin NUF - North Uralian Foldbelt JNF- Junggar Forebelt PAR - Parapamiz Zone AMD - Amu-Darya Block KAR - Karabagaz Massif PBA - Pribalkhash Zone BDM - Baidara Massif KCB - Karachytyr Basin PCB - Precaspian Basin SHB - South Hissar Basin CKK - Central Karakum KHM - Khanty-Mansy Block STF - South Tian-Shan foldbelt CNA - Central Kunlun Arc KOK - Kokshetau Massif SUF - South Uralian Foldbelt CPM - Central Pamirs KPS - Karpinsky Swell CSB - Chu-Sarysu Basin KUA - Kurama Arc TIM - Timan Block DDB - Dnepr-Donets Basin MGZ - Magnitogorsk Zone TPB - Timan-Pechora Basin UFB - Uralian Foreland EUF - East-Uralian Foldbelt MNB - Mangyshlak Basin UKM - Ukrainian Shield GCM - Great Caucasus Massif MSB - Moscow Basin HIN - Hindukush Block UST - Ustyurt NKL - North Kunlun VOR - Voronezh Shield 42 48 54 60 66 72 78 84 90 96
Fig. 6 Davydov Relative species diversity Biogenic apatite geochemical record US Midcontinent Fusulinid FAD in Fusulinid FOD Atmospheric Australian Regional 18 S in West Tethys δ O (‰V-SWOM) eustatic sea-level CO (p.p.m.) Glaciation
E Tethyan and Boreal in N. America 2 I Stage magnitude (m) R Stage 10 30 50 70 90 110 Events
realms Regional Stage
E 24 23 22 21 200 0 S Fusullinid Zones 0 277.0 Yangchienia Irenian 3000 2000 1000 40 Southern Urals record Solikamian Robustoschwagerina 280 Fillipovian Kungurian 39 Yangchienia P2B N Saranian
38 Leonardian A
I Biwaella, Toriyamaia 37
L 285.0 36 Sarginian A 35 Chalaroschwagerina R Artinskian Irginian 34 Chalaroschwagerina
U P2A
Burtsevian 33 Toriyamaia S
290 I 290.0 Lenoxian
C Sterlitamakian 32 Sakmarian Robustoschwagerina Urals-Tethys Tastubian 31 ? P1 30 Eoparafusulina Eoparafusulina gateway closure 295.0 Shikhanian 29 Pseudoschwagerina Asselian Uskalykian 28
Pseudoschwagerina Nealian 250 species 298.9 Sjuranian 27 Melekhovian 26 Schellwienia 300 Noginian 25 Schellwienia
Gzhelian Pavlovoposad. 24 N
Rusavkian 23 Biwaella irgilian V A 22
I 303.7 Dorogovilovian 20-21 Triticites (s.l.) .
N Kasimovian Khamovnich. 18-19 Msr A Krevyakian 17 Eowaeringella Eowaeringella V 307.0 Peskovian 16 C4 L Triticites (s.l.)
Myachkovian 15 Y
S Podolskian 14 Bedeeina Wedekindellina 310 Wedekindellina Desmoin. C3
N Moscovian Kashirian 13
N Bedeeina 12 E Tsninian 11 P 314.7 Vereian Profusulinella
Melekesian 10 Atokan Cheremshanian 9 Pseudostaffella Bashkirian Prikamian 8 Profusulinella Monotaxinoides transitorius 320 Severokeltmian 7 Krasnopolyan. 6 Pseudostaffella Voznesenian 5 Millerella Millerella Morrowan Rheic gateway closure C2 323.2 Zapaltjubian
N 4 A
I Protvian Monotaxinoides P
P 3
I Serpukhovian Steshevian transitorius S
S Tarussian
I 2
S C1
S Venevian 1
330 I 330.0 Chesterian (part) Chesterian Ma M
The occurrence of the taxon 15 20 25 30 Climatic optimum Climatic cooling Migration event in each province (ºC) Ocean surface temperature Seismites, olistostromes
Davydov Fig. 7 Seismites at Kondurovsky Section (photo courtesy of W. S. Snyder)
Kasimovian olistolith at Zianchurino village (photo courtesy of G. Mizens)
Fig. 8 Davydov Early‐Middle Asselian Late Asselian_species Region 123456‐7891011 Region 123456‐7891011 1 1 0,9965 1,0000 1,0000 0,9960 0,8955 0,8075 0,2155 0,1425 0,0000 1 1 1,0000 0,8785 1,0000 1,0000 0,9745 0,6095 0,3365 0,5130 0,0465 2 0,9965 1 0,9990 0,9995 1,0000 1,0000 0,8005 0,6090 0,2700 0,1275 2 1,0000 1 0,9430 0,9940 1,0000 0,9835 0,4240 0,4800 0,3460 0,0435 3 1,0000 0,9990 1 1,0000 0,9910 1,0000 0,9980 0,0440 0,0635 0,0000 3 0,8785 0,9430 1 0,9905 0,9210 0,9980 0,9565 0,9230 0,6510 0,2295 4 1,0000 0,9995 1,0000 1 1,0000 1,0000 0,9610 0,0010 0,0005 0,0000 4 1,0000 0,9940 0,9905 1 1,0000 0,9560 1,0000 0,0000 0,0000 0,0000 5 0,9960 1,0000 0,9910 1,0000 1 1,0000 0,9500 0,0265 0,0000 0,0000 5 1,0000 1,0000 0,9210 1,0000 1 0,9950 0,9995 0,0005 0,0100 0,0000 6‐7 0,8955 1,0000 1,0000 1,0000 1,0000 1 1,0000 0,9480 0,8855 0,0000 6‐7 0,9745 0,9835 0,9980 0,9560 0,9950 1 1,0000 0,9995 0,9850 0,8245 8 0,8075 0,8005 0,9980 0,9610 0,9500 1,0000 1 0,7040 0,0030 0,0000 8 0,6095 0,4240 0,9565 1,0000 0,9995 1,0000 1 0,9505 0,0145 0,0000 9 0,2155 0,6090 0,0440 0,0010 0,0265 0,9480 0,7040 1 1,0000 0,3565 9 0,3365 0,4800 0,9230 0,0000 0,0005 0,9995 0,9505 1 1,0000 0,9910 10 0,1425 0,2700 0,0635 0,0005 0,0000 0,8855 0,0030 1,0000 1 0,9935 10 0,5130 0,3460 0,6510 0,0000 0,0100 0,9850 0,0145 1,0000 1 1,0000 11 0,0000 0,1275 0,0000 0,0000 0,0000 0,0000 0,0000 0,3565 0,9935 1 11 0,0465 0,0435 0,2295 0,0000 0,0000 0,8245 0,0000 0,9910 1,0000 1
Early Sakmarian_species Late Sakmarian_species Region 12456‐7891011 Region 1456‐7891011 1 1 0.9995 1 1 0.078 0000 1110.874 0.002 0 0 0 0.001 2 0.9995 1 0.9625 0.981 0.0085 0000 411100000 4 1 0.9625 1 1 0.0225 0000 50.874 1 1 0.0165 0 0 0.001 0.0065 5 1 0.981 1 1 0.109 0 0 0.0005 0 6‐7 0.002 0 0.0165 1 1 1 0.8635 0.4005 6‐7 0.078 0.0085 0.0225 0.109 1 1 1 0.9925 0.6355 80001110.9995 0.0085 800001110.9715 0 900011110.0645 9000011110.0025 10 0 0 0.001 0.8635 0.9995 1 1 0.823 10 0 0 0 0.0005 0.9925 0.9715 1 1 0.9975 11 0.001 0 0.0065 0.4005 0.0085 0.0645 0.823 1 1100000.6355 0 0.0025 0.9975 1
Early Artinskian_species Late Artinskian_species Region 12456‐7891011 Region 1246‐7891011 1 1 0.99 0.964 0.9615 00000 110.0745 0.1055 0.0195 0 0 0 0.031 2 0.99 1 0.6485 0.47 0.1845 0.02 0.037 0.0125 0.05 2 0.0745 1 0.23 0.0315 0 0 0 0.049 4 0.964 0.6485 1 0.9555 00000 40.1055 0.23 100000.006 5 0.9615 0.47 0.9555 1 0.3485 0.108 0.184 0.1075 0.2095 6‐7 0.0195 0.0315 0 1 1 1 0.984 0.82 6‐7 0 0.1845 0 0.3485 11110.6145 800011110.979 8 0 0.02 0 0.108 11110.7325 900011110.982 9 0 0.037 0 0.184 11110.8405 10 0 0 0 0.984 1 1 1 0.9945 10 0 0.0125 0 0.1075 11111 110.031 0.049 0.006 0.82 0.979 0.982 0.9945 1 11 0 0.05 0 0.2095 0.6145 0.7325 0.8405 1 1
Regions with Tethyan dominant WWBF Regions with Boreal dominant WWBF Regions with WWBF of Tethyan affinity that in Sakmarian become of Boreal affinity
For the region names see Fig. 1. Early‐Middle Asselian_genus Late Asselian_genus Region 123456‐7891011 Region 123456‐7891011 1111110.9955 0.917 0.8815 0.7735 0.022 1 1 1 0,907 1 1 0,9965 0,327 0,303 0,3575 0,013 21111110.9665 0.9805 0.8275 0.5755 2 1 1 0,8855 1 1 0,966 0,034 0,2365 0,0715 0,004 311111110.2015 0.163 0 3 0,907 0,8855 1 1 0,932 0,999 0,635 0,5495 0,0845 0,0005 41111110.9785 0.0135 0.0015 0 4 111110,9805 0,387 0 0,0005 0 51111110.983 0.325 0.0075 0 5 1 1 0,932 1 1 1 0,4905 0,012 0,02 0 6‐7 0.9955 1111110.9905 0.948 0 6‐7 0,9965 0,966 0,999 0,9805 1 1 1 0,9925 0,924 0,5185 8 0.917 0.9665 1 0.9785 0.983 1 1 0.816 0.0005 0 8 0,327 0,034 0,635 0,387 0,4905 1 1 1 0,6255 0 9 0.8815 0.9805 0.2015 0.0135 0.325 0.9905 0.816 1 1 0.777 9 0,303 0,2365 0,5495 0 0,012 0,9925 1 1 1 0,846 10 0.7735 0.8275 0.163 0.0015 0.0075 0.948 0.0005 1 1 1 10 0,3575 0,0715 0,0845 0,0005 0,02 0,924 0,6255 1 1 1 11 0.022 0.5755 000000.777 1 1 11 0,013 0,004 0,0005 0 0 0,5185 0 0,846 1 1
Early Sakmarian_genus Late Sakmarian_genus Region 12456‐7891011 Region 1 4 5 6‐7 8 9 10 11 1 11110,1475 0000 1 110,9995 0,007 0000 2 1 1 1 0,997 0,012 0000 4 1110,001 0000 4 11110,064 0000 50,9995 1 1 0,081 0 0 0,0025 0,013 5 1 0,997 1 1 0,557 0,0055 0 0,007 0 6‐7 0,007 0,001 0,081 1 1 1 0,9035 0,3075 6‐7 0,1475 0,012 0,064 0,557 11110,9215 8 00011110,022 8 0 0 0 0,0055 1 1 1 0,9585 0 9 00011110,205 9 000011110,0355 10 0 0 0,0025 0,9035 1 1 1 0,9975 10 0 0 0 0,007 1 0,9585 1 1 1 11 0 0 0,013 0,3075 0,022 0,205 0,9975 1 1100000,9215 0 0,0355 1 1
Early Artinskian_genus Late Artinskian_genus Region 12456‐78 91011 Region 1 2 4 6‐7 8 9 10 11 1 1 1 0,9995 0,945 00000 1 10,434 0,2795 0,005 0 0 0 0,0035 2 1 1 0,9985 0,414 0,029 0 0,0005 0 0,001 2 0,434 1 0,724 0,0435 0 0 0 0,0465 4 0,9995 0,9985 1 0,9085 00000 40,2795 0,724 100000,006 5 0,945 0,414 0,9085 1 0,365 0,134 0,1945 0,122 0,231 6‐7 0,005 0,0435 01110,9975 0,9485 6‐7 0 0,029 0 0,365 11110,876 8 00011110,9975 8 0 0 0 0,134 11110,858 9 00011110,9975 9 0 0,0005 0 0,1945 11110,96 10 0 0 0 0,9975 1111 10 0 0 0 0,122 11111 110,0035 0,0465 0,006 0,9485 0,9975 0,9975 1 1 11 0 0,001 0 0,231 0,876 0,858 0,96 1 1
Regions with Tethyan dominant WWBF Regions with Boreal dominant WWBF Regions with WWBF of Tethyan affinity that in Sakmarian become of Boreal affinity 1 Database References 2 3 Akhmetshina, L.Z., Kukhtinov, D.A., and Kukhtinova, L.V., 2013, Atlas of paleoontological remains of the 4 Permian deposit of northern and eastern segments of Precaspian Basin (Kazakhstan part): 242 с., 61 5 палеонт. табл., 39 ил.: Alma-Ata, Kazakhstan. 6 Akramkhodjaev, A.M., Avazkhodjaeva, K.K., and Labutina, L.I., 1979, Lithology, environments and oil-gas 7 bearing of pre-Jurassic deposits of Ustyurt.: Tashkent, Uzbekistan, Fan Publishing House. 8 Akramkhodjaev, A.M., Yuldashe, Z.Y., Avazkhodjaeva, K.K., and Labutina, L.I., 1981, Key and parametric 9 wells of Ustyurt.: Tashkent, Uzbekistan, Fan Publishing House. 10 Alekseev, A.S., Goreva, N.V., Isakova, T.N., and Kossovaya, O.L., 2009, The stratotype of the Gzhelian 11 Stage (Upper Carboniferous) in Moscow Basin, Russia, in Puchkov, V.N., ed., Carboniferous type 12 sections in Russia, potential and global stratotypes: Ufa, Institute of geology of the Ufa scientific 13 Center, p. 165. 14 Alekseev, A.S., Goreva, N.V., Isakova, T.N., and Makhlina, M.K., 2004, Biostratigraphy of the 15 Carboniferous in the Moscow Syneclise, Russia: Newsletter on Carboniferous Stratigraphy, v. 22, p. 16 28–35. 17 Alekseev, A.S., Goreva, N.V., Kulagina E.I., Kossovaya, O.L., Isakova, T.N., and Reimers, A.N., 2002, Upper 18 Carboniferous of South Urals (Bashkiria, Russia). 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99 Chuvashov, B.I., Djupina, G.V., Mizens, G.A., and Chernykh, V.V., 1990, The Key-sections of Upper 100 Carboniferous and Lower Permian in the western slope of Urals and Preurals.: Ekaterinburg, Institute 101 of Geology and geochemistry of Uralian Branch of Russian Academy of Sciences, (None), 368 p. 102 Chuvashov, B.I., and Dyupina, G.V., 1971, Verkhniy paleozoy rayona poselka Biserti. The upper Paleozoic 103 of the Bisert region: Akademiya Nauk SSSR, Ural'skiy Filial, Institut Geologii i Geokhimii, Trudy, v. 88, 104 p. 3–24. 105 Chuvashov, B.I., and Dyupina, G.V., 1978, Faunisticheskiye kompleksy i problemy korrelyatsii razno 106 fatsial'nykh otlozheniy (na primere assel'skogo yarusa zapadnogo sklona Srednogo Urala). Faunal 107 complexes and problems of the correlation of diverse facies deposits; the Asselian Stage of the 108 western slopes of the Central Urals as an example: Trudy Instituta Geologii i Geofiziki, v. 386, p. 124– 109 146. 110 Chuvashov, B.I., and Ivanova, R.M., Moskovskiye i verkhnekamennougol'nyye otlozheniya v razreze "Uly- 111 Taldyk" (Vostochnyye Mugodzhary). Moscovian and Upper Carboniferous deposits of the "Uly- 112 Taldyk" Section, eastern Mugodzhar Hills. 113 Chuvashov, B.I., and Ivanova, R.M., Sredniy karbon rek Kunary i Iseti. Middle Carboniferous of the 114 Kunara and Iset' rivers. 115 Chuvashov, B.I., and Ivanova, R.M., 1980, Middle Carboniferous of the Kunara and Iset' rivers: 116 Carboniferous stratigraphy, Fusulinidae, and miospores of the Urals. 117 Chuvashov, B.I., and Ivanova, R.M., 1980, Moscovian and Upper Carboniferous deposits of the "Uly- 118 Taldyk" Section, eastern Mugodzhar Hills: Carboniferous stratigraphy, Fusulinidae, and miospores of 119 the Urals. 120 Chuvashov, B.I., Ivanova, R.M., and Kolchina, A.N., 1979, Verkhniy paleozoy basseyna r. Sinary. The 121 upper Paleozoic basin of the Sinara River: Trudy Instituta Geologii i Geokhimii, no, no. 26, p. 95–125. 122 Chuvashov, B.I., Ivanova, R.M., and Kolchina, A.N., editors, 1984, Verkhniy paleozoy vostochnogo sklona 123 Urala; stratigrafiya i geologicheskaya istoriya. Upper Paleozoic deposits of the eastern slope of the 124 Urals; stratigraphy and geologic history: Sverdlovsk, UO AN of USSR, Papulov, G.N., 230 p. 125 Chuvashov, B.I., Leven, E.Ya.and Davydov, V.I., editor, 1986, Carboniferous/Permian Boundary beds of 126 the Urals, Pre-Urals area and Central Asia.: Moscow, Nauka Publishing House. 127 Davydov, V.I., 1981, New species of middle Carboniferous Palaeorechelina.: Paleontological Journal, no. 128 3, 120-124 (In Russian). 129 Davydov, V.I., 1984, Zonal'nye i yarusnye podrazdeleiya verkhnego karbona yu-go-vostochnogo Darvaza. 130 Fusulinid zonal subdivisions of the Upper Carboniferous of the southwestern Darvas: Bulletin of 131 Moscow Society of Natural Studies, Geological Series, v. 59, no. 3, p. 41. 132 Davydov, V.I., 1986, Fusulinids of Carboniferous-Permian boundary beds of Darvas, in B.I. Chuvashov, 133 E.Ya. Leven, and V.I. Davydov, ed., Carboniferous/Permian Boundary beds of the Urals, Pre-Urals 134 area and Central Asia.: Moscow, Nauka Publishing House, p. 103. 135 Davydov, V.I., 1986, Precise definition of the Carboniferous-Permian boundary in Donets Basin and the 136 Northern Caucasus based on paleomagnetic criteria: Soviet Geology, v. 12, p. 74–76. 137 Davydov, V.I., 1986, Upper Carboniferous and Asselian fusulinids of the Southern Urals, in Chuvashov, 138 E.Ya. Leven and V.I. Davydov, ed., Carboniferous--Permian Boundary beds of the Urals, Pre-Urals and 139 Central Asia: Moscow, Nauka Publishing House, p. 77. 140 Davydov, V.I., 1987, Fusulinid zone DAIXINA BOSBYTAUENSIS - D. ROBUSTA in South Ferghana.: Doklady 141 Akademii Nauk SSSR, v. 292, no. 1, 160-164 (In Russian). 142 Davydov, V.I., 1988, Archaediscids in the Upper Carboniferous and Lower Permian: Revue de 143 Paleobiologie, spec. v. 2, p. 39–46. 144 Davydov, V.I., 1988, The origin and evolution some "pseudofusulinids": Paleontologichesky Zhurnal, no. 145 3, p. 10.
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