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The Floodwaters of Mars 7 June 2013
The floodwaters of Mars 7 June 2013 erosive power of the fast-flowing water, this hardier outcrop has stood the test of time. Slightly further downstream, the flood waters did their best to erase the 100 km-wide Sharonov crater, crumpling its southern rim. Around Sharonov, many small streamlined islands form teardrop shapes rising from the riverbed, carved as water swept around these natural obstacles. Kasei Valles. (Phys.org) —Dramatic flood events carved this impressive channel system on Mars covering 1.55 million square kilometres, shown here in a stunning new mosaic from ESA's Mars Express. The mosaic, which features the spectacular Kasei Valles, comprises 67 images taken with the spacecraft's high-resolution stereo camera and is released during the week of the 10th anniversary of the spacecraft's launch to the Red Planet. Kasei Valles is one of the largest outflow channel systems on Mars – from source to sink, it extends Kasei Valles in context. some 3000 km and descends by 3 km in altitude. The scene covered in the mosaic spans 987 km north–south (19–36°N) and 1550 km east–west (280–310°E). The region between Sacra Mensa and Sharonov is seen in close-up detail in the perspective view The channel originates beyond the southern edge below, looking downstream from the northern flank of this image near Valles Marineris, and empties of Kasai Valles. into the vast plains of Chryse Planitia to the east (right). Zooming into the valley floor reveals small craters with bright dust 'tails' seemingly flowing in the Kasei Valles splits into two main branches that hug opposite direction to the movement of water. -
La Doppia Edizione De Le Lagrime Di San Pietro Di Luigi Tansillo Tra Censura E Manipolazione
Università degli Studi di Napoli Federico II Dottorato di ricerca in Filologia moderna Coordinatore: Prof. Costanzo Di Girolamo Tesi di dottorato Ciclo XXIII La doppia edizione de Le lagrime di San Pietro di Luigi Tansillo tra censura e manipolazione Candidato: Dott. Luca Torre Tutore: Prof. Tobia R. Toscano Cotutore: Prof. Corrado Calenda Napoli 2010 INDICE Introduzione .......................................................................................... p. 3 1. La tradizione de Le lagrime di San Pietro..................................... » 4 2. Lo sfondo culturale e l’inventio tansilliana.................................... » 16 3. Giovan Battista Attendolo e la censura ecclesiastica..................... » 27 4. La vis polemica di Tommaso Costo: la stampa del 1606............... » 43 5. Conclusioni minime....................................................................... » 51 6. La presente edizione: criteri e struttura.......................................... » 56 Criteri di trascrizione.............................................................................. » 58 Testi ....................................................................................................... » 61 Pianto primo....................................................................................... » 63 Pianto secondo................................................................................... » 86 Pianto terzo........................................................................................ » 100 Pianto quarto..................................................................................... -
Analysis of Polarimetric Mini-SAR and Mini-RF Datasets for Surface Characterization and Crater Delineation on Moon †
Proceeding Paper Analysis of Polarimetric Mini-SAR and Mini-RF Datasets for Surface Characterization and Crater Delineation on Moon † Himanshu Kumari and Ashutosh Bhardwaj * Photogrammetry and Remote Sensing Department, Indian Institute of Remote Sensing, Dehradun 248001, India; [email protected] * Correspondence: [email protected]; Tel.: +91-9410319433 † Presented at the 3rd International Electronic Conference on Atmospheric Sciences, 16–30 November 2020; Available online: https://ecas2020.sciforum.net/. Abstract: The hybrid polarimetric architecture of Mini-SAR and Mini-RF onboard Indian Chan- drayaan-1 and LRO missions were the first to acquire shadowed polar images of the Lunar surface. This study aimed to characterize the surface properties of Lunar polar and non-polar regions con- taining Haworth, Nobile, Gioja, an unnamed crater, Arago, and Moltke craters and delineate the crater boundaries using a newly emerged approach. The Terrain Mapping Camera (TMC) data of Chandrayaan-1 was found useful for the detection and extraction of precise boundaries of the cra- ters using the ArcGIS Crater tool. The Stokes child parameters estimated from radar backscatter like the degree of polarization (m), the relative phase (δ), Poincare ellipticity (χ) along with the Circular Polarization Ratio (CPR), and decomposition techniques, were used to study the surface attributes of craters. The Eigenvectors and Eigenvalues used to measure entropy and mean alpha showed distinct types of scattering, thus its comparison with m-δ, m-χ gave a profound conclusion to the lunar surface. The dominance of surface scattering confirmed the roughness of rugged material. The results showed the CPR associated with the presence of water ice as well as a dihedral reflection inside the polar craters. -
I Quaderni Del Castello
Gruppo Amici della Storia Locale “Giuseppe Gerosa Brichetto” I QUADERNI DEL CASTELLO NUMERO 3 CONFERENZE AL CASTELLO DI PESCHIERA BORROMEO MAGGIO 2012 PRESENTAZIONE Ed eccoci al terzo appuntamento, con i Quaderni del Castello. In quanto tale, che questo numero 3 della Rivista sia “perfetto”, non osiamo crederlo, in ogni caso il giudizio complessivo spetta ai lettori, che ci auguriamo benevoli. Di certo, noi ce l’abbiamo messa tutta, per confezionarlo meglio che possiamo. Riguardo ai contenuti, la valutazione spetta appunto a chi legge; sulle caratteristiche tecniche, crediamo però non possano esserci dubbi, il progresso si vede subito: difatti, se fino all’anno scorso la pubblicazione veniva prodotta “in casa”, utilizzando personal computer e stampanti casalinghe, le presenti pagine sortiscono da una tipografia in piena regola, mentre per la fase di pre-stampa ci siamo avvalsi della competenza e della preziosa collaborazione dell’amico Roberto Casetta, che generosamente ha preparato il tutto, cosa di cui lo ringraziamo di cuore. Siamo grati altresì ai Conti Franco e Filippo Borromeo, che ci onorano del loro sostegno e con squisita cortesia ci ospitano una volta ancora nella splendida cornice del Castello di Peschiera Borromeo, per la presentazione in anteprima della pubblicazione, sotto forma di conferenze dei singoli Autori, i quali anticipano i testi di seguito riportati integralmente. Tra il Gruppo Amici della Storia Locale e la Famiglia Borromeo si è da tempo stabilita una virtuosa “corrispondenza d’amorosi sensi” che ha reso possibile, oltre che questa Rivista, l’organizzazione di memorabili giornate di visite al Castello, soddisfacendo la sete di bellezza di centinaia e centinaia di persone del Circondario, le quali hanno potuto così ammirare da vicino i tesori d’arte e di storia custoditi nella nobile dimora. -
THE PHILOSOPHER and the VOLCANO on the ANTIQUE SOURCES of NIETZSCHE's UBERMENSCH Babette Babich
Fordham University Masthead Logo DigitalResearch@Fordham Articles and Chapters in Academic Book Philosophy Collections Fall 2011 The hiP losopher and the Volcano Babette Babich Fordham University, [email protected] Follow this and additional works at: https://fordham.bepress.com/phil_babich Part of the Classical Literature and Philology Commons, Continental Philosophy Commons, German Language and Literature Commons, and the History of Philosophy Commons Recommended Citation Babich, Babette, "The hiP losopher and the Volcano" (2011). Articles and Chapters in Academic Book Collections. 43. https://fordham.bepress.com/phil_babich/43 This Article is brought to you for free and open access by the Philosophy at DigitalResearch@Fordham. It has been accepted for inclusion in Articles and Chapters in Academic Book Collections by an authorized administrator of DigitalResearch@Fordham. For more information, please contact [email protected]. THE PHILOSOPHER AND THE VOLCANO ON THE ANTIQUE SOURCES OF NIETZSCHE'S UBERMENSCH Babette Babich Happy and blessed one, you shall be a god Hence and in order to get to Empedocles, I ar instead of a mortal. gue that it is necessary to read Nietzsche's Thus Empedocles Spoke Zarathustra as an overtly Menippean sat It has traditionally been observed that the fig ire as Nietzsche refers to this tradition. Inasmuch ure of Empedocles is key to Nietzsche's as the satires attributed to the cynic Menippus of Zarathustra. But the nature of this significance is Gadara happen to be lost, I read Nietzsche's Thus less commonly detailed: in part this is Nietz Spoke Zarathustra via the second century AD sche's fault, as and although he includes Lucian's "high" or serious, i.e., truth-purposing Empedocles in his notes for the Pre-Platonic (as the ancients described it) kind of parody 1 Philosophers, Nietzsche excludes Empedocles where Lucian relates to Menippus, at least in from his Philosophy in the Tragic Age of the some part, as Plato does to Socrates. -
Crosses in the Mosaic Floors of Churches in Provincia Arabia and Nearby Territories, Against the Background of the Edict of Theodosius II II
JMR 8, 2015 33-60 Crosses in the Mosaic Floors of Churches in Provincia Arabia and Nearby Territories, Against the Background of the Edict of Theodosius II II. Theodosius’un Fermanının Arka Planına Karşı Arabistan Eyaleti ve Yakın Bölgelerdeki Kiliselerin Mozaik Tabanlarında Görülen Haçlar Lihi HABAs* (Received 23 February 2015, accepted after revision 7 November 2015) Abstract Between the 4th and 8th centuries A.D., many churches were founded in Provincia Arabia and neighbouring ter- ritories (today’s Transjordan). Most of the churches were paved with mosaics. The mosaics floors are decorated with geometric, vegetal and figurative carpets with a rich repertoire of scenes of daily life, sometimes accom- panied by personifications. The floors were also decorated with symbolic heraldic arrangements and symbolic motifs, among them crosses. This research focus on a description of the different types of cross found in Byzan- tine churches in Transjordan, their position on the mosaic floors and in the church space, and the use of parallel motifs with equivalent significance as concealed crosses. The repertoire of crosses is rich, and crosses have been found of the equal-armed Greek cross type, the Latin cross, the Maltese cross, or a geometric interlace in the form of a Greek cross. There are also crosses of the crux clipeata, crux gemmata and crux decussate type. In some places the letters ΑΩ are shown between the arms of the cross, or suspended from the vertical arm. In other places the cross is shown on a graduated mound symbolizing the hill of Golgotha. The crosses in mosaic floors decorate the vestibules of church complexes, churches, chapels attached to churches, crypts, martyrium chapels, funerary chapels, and baptisteries. -
USAFA Application
Campus Box 8208 College of Sciences 1125 Jordan Hall Department of Marine Earth & Atmospheric Sciences 2800 Faucette Drive [email protected] (704) 747-4189 Raleigh, NC 27695-8208 meas.ncsu.edu Curriculum Vitae Colonel (Ret) Julian Matthews Chesnutt Geology Ph.D. Candidate, Adjunct Professor, Lecturer and Teaching Assistant Education ● Completed all Geology Ph.D. coursework with a 4.01 GPA for a combined 3.872 Graduate work GPA ● Unconditionally passed both oral and written Geology Ph.D. qualification exams ● Graduate Certificate in Geospatial Information Science, North Carolina State University, Raleigh NC—2017 o Earned at 4.167 GPA in the GIS Graduate Certificate Program ● National Defense Fellow, Institute for the Study of Diplomacy, Georgetown University, Washington DC—2009 ● Master of Military Operational Art & Science, School of Advanced Air and Space Studies, Maxwell AFB AL—2004 ● Master of Operational Art, Air Command and Staff College, Distinguished Graduate, Maxwell AFB AL—2003 ● Master of Engineering in Materials Science, North Carolina State University, Raleigh NC—1996 ● Bachelor of Science in Space Physics, Distinguished Graduate, US Air Force Academy, Colorado Springs CO—1989 Teaching Accomplishments • Environmental Geology (GEL 230) Lecturer & Lab Adjunct Professor, Durham Technical Community College—2019 ● Planetary Geology (ERS 131, ERS 132) Course Developer, Lecturer & Lab Adjunct Professor, NC Wesleyan University—2018 ● Physical Geology (MEA 101, MEA 111) Lecturer, Lab Instructor & Teaching Assistant at NC State University—2016-2019 -
Dendrochronology 459
DENDROCHRONOLOGY 459 Taylor, R. E. (1987). Radiocarbon Dating: An Archaeological Wintle, A. G. (1973). Anomalous fading of thermoluminescence in Perspective. Academic Press, New York. mineral samples. Nature 245, 143–144. Tuniz, C., Bird, J. R., Fink, D., and Herzog, G. F. (1998). Wohlfarth, B., Bjo¨ rck, S., Possnert, G., et al. (1993). AMS dating Accelerator Mass Spectrometry: Ultasensitive Analysis for of Swedish varved clays of the last glacial/interglacial transition Global Science. CRC Press, Boca Raton, FL. and potential difficulties of calibrating Late Weichselian ‘‘abso- Wagner, G. A. (1995). Age Determination of Young Rocks and lute’’ chronologies. Boreas 22, 113–128. Artifacts. Springer, Berlin. Zreda, M., and Phillips, F. (2000). Cosmogenic nuclide buildup in Wehmiller, J. F., and Miller, G. H. (2000). Aminostratigraphic dating surficial materials. In Quaternary Geochronology, Methods methods in Quaternary geology. In Quaternary Geochronology, and Applications (J. S. Noller et al., Eds.), pp. 61–76. Methods and Applications (J.S.Nolleret al., Eds.), pp. 187–222. American Geophysical Union, Washington, DC. American Geophysical Union, Washington, DC. Westgate, J. A., and Naeser, N. D. (1995). Tephrochronology and fission-track dating. In Dating Methods for Quaternary Relevant Website Deposits (N. W. Rutter and N. R. Catto, Eds.), pp. 15–28. Geological Survey of Canada, Ottawa. http://www.gg.rhul.ac.uk – Royal Holloway: Department of Geography. Dendroarchaeology see Plant Macrofossil Methods and Studies: Dendroarchaeology DENDROCHRONOLOGY D Smith and D Lewis, University of Victoria, Victoria, precipitation (Stallings, 1937). The first recorded Canada application of dendrochronology occurred in 1737 ª 2007 Elsevier B.V. All rights reserved. when Du Hamel and De Buffon noted a prominent frost damaged tree ring in recently felled trees that was later recorded in both Sweden and Germany Dendrochronology (Studhalter, 1955, 1956). -
Mineralogical Study of Lunar Das Impact Crater Using Chandrayaan-1- Moon Mineralogical Mapper
50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 2273.pdf MINERALOGICAL STUDY OF LUNAR DAS IMPACT CRATER USING CHANDRAYAAN-1- MOON MINERALOGICAL MAPPER. A.Karthi1, Centre for Applied Geology, The Gandhigram Rural Institute-Deemed to be University, Dindigul, Tamilnadu - 624 302, India ([email protected]) Introduction: The compositional studies and topo- graphical information will provide the best understand- ing of the lunar crust evolution [1, 2]. Optical maturity (OMAT) is key to geological marks of the Moon that closely related to its surface maturity of the space envi- ronment. The optical maturity parameter is used to derive understanding of the mature and immature index of the lunar surface (higher = immature (fresher), lower = more mature) [3, 4]. Iron and titanium are significant rock-forming elements on the moon and iron and tita- nium distributions are important for the recognition of lunar mineralogy and crustal evolution [5]. Remotely obtained spectra in the visible near-infrared (VNIR) and shortwave infrared (SWIR) wavelength regions can provide information on the mineralogy abundance of a planetary surface [6]. The present study, focused on elemental composition and spectral charaters of the Das crater in the lunar farside. Fig.1. a). Das crater 3D model with elevation meas- urement and b). Cross section of Das crater. Study Area: Das is an impact crater on the far side of the southern Moon (Fig.1 a&b). It is located in latitude Results and Discussion: of 26°36′S longitude of 136°48′W and it’s situted in northwest of the walled plain of Chebyshev. Das is Das southern and western parts show the low maturity formed in the part of the Copernican system. -
Amazonian Geologic History of the Echus Chasma and Kasei Valles System on Mars: New Data and Interpretations
Earth and Planetary Science Letters 294 (2010) 238–255 Contents lists available at ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl Amazonian geologic history of the Echus Chasma and Kasei Valles system on Mars: New data and interpretations Mary G. Chapman a,⁎, Gerhard Neukum b, Alexander Dumke b, Greg Michael b, Stephan van Gasselt b, Thomas Kneissl b, Wilhelm Zuschneid b, Ernst Hauber c, Nicolas Mangold d a Planetary Science Institute, Tucson, Arizona, USA b Institute of Geosciences, Freie Universitaet Berlin, Germany c German Aerospace Center (DLR), Berlin, Germany d LPGN, CNRS, Université Nantes, France article info abstract Article history: New high-resolution datasets have prompted a mapping-based study of the 2500-km-long Echus Chasma Accepted 19 November 2009 and Kasei Valles system that utilizes geomorphic details, stratigraphic relations, and cratering statistics Available online 29 December 2009 derived from the new datasets. Our results suggest that between the Hesperian and Amazonian Epochs on Mars (3.7 Ga to Recent), the study area was affected by at least 4 episodes of widespread volcanic activity Keywords: and 4 periods of episodic fluvio-glacial activity. This paper discusses the Amazonian (b1.8 Ga) history of the chasma study area, during which time the last of the four volcanic episodes occurred between the last two episodes valles fl fi anastomosing of uvio-glacial activity. Highlights of our new ndings from this time period include (1) evidence that dendritic suggests glaciers and near-surface ice may have persisted through Amazonian time in local areas over the permafrost entire length of Kasei Valles; (2) a new widespread platy-flow surface material that is interpreted to be 2100-km-runout flood lavas sourced from Echus Chasma; and (3) a fracture in Echus Chasma, identified to have sourced at least one late-stage flood, that may have been the origin for the platy-flow material and young north-trending Kasei flood water. -
Landscapes of Mars a VISUAL TOUR
Landscapes of Mars A VISUAL TOUR Landscapes of MarsMarsLandscapes of A VISUAL TOUR GREGORY L. VOGT © 2008 Springer Science+Business Media, LLC Printed on acid-free paper. Library of Congress Control Number: 2008933361 ISBN: 978-0-387-75467-3 e-ISBN: 978-0-387-75468-0 All rights reserved. This work may not be translated or copied in whole or in part without the written permission of the publisher (Springer Science+Business Media, LLC, 233 Spring Street, New York, NY 10013, USA) except for brief excerpts in connection with reviews or scholarly analysis. Use in connection with any form of information stor- age and retrieval, electronic adaptation, computer software, or by simi- lar or dissimilar methodology now known or hereafter developed is for- bidden. The use in this publication of trade names, trademarks, service marks, and similar terms, even if they are not identified as such, is not to be taken as an expression of opinion as to whether or not they are subject to proprietary rights. Printed in the United States of America. 9 8 7 6 5 4 3 2 1 springer.com Landscapes of Mars A VISUAL TOUR CONTENTS Introduction 9 CHAPTER 1 The Two Faces of Mars 25 CHAPTER 2 To Hellas and Back 41 CHAPTER 3 Snows of Olympus 51 CHAPTER 4 The Grandest Canyon 61 CHAPTER 5 Making an Impact on Mars 69 CHAPTER 6 Water and Wind 77 CHAPTER 7 North and South 87 CHAPTER 8 Living or Not? 93 CHAPTER 9 For a Closer Look 101 CHAPTER 10 Mars in 3D 111 APPENDIX A Topographic Terminology 131 APPENDIX B Mars vs. -
Lunar Sourcebook : a User's Guide to the Moon
REFERENCES Adams J. B. (1974) Visible and near-infrared diffuse chemistry, mineralogy and petrology of some Apollo 11 reflectance spectra of pyroxenes as applied to remote lunar samples. Proc. Apollo 11 Lunar Sci. Conf., pp. 93–128. sensing of solid objects in the solar system. J. Geophys. Ahrens T. J. and Cole D. M. (1974) Shock compression and Res., 79, 4829–4836. adiabatic release of lunar fines from Apollo 17. Proc. Lunar Adams J. B. (1975) Interpretation of visible and near-infrared Sci. Conf. 5th, pp. 2333–2345. diffuse reflectance spectra of pyroxenes and other rock Ahrens T. J. and O’Keefe J. D. (1977) Equations of state and forming minerals. In Infrared and Raman Spectroscopy of impact-induced shock-wave interaction on the Moon. In Lunar and Terrestrial Materials (C. Karr, ed.), pp. 91–116. Impact and Explosion Cratering (D. J. Roddy, R. O. Pepin, Academic, New York. and R. B. Merrill, eds.), pp. 639–656. Pergamon, New York. Adams J. B. and McCord T. B. (1973) Vitrification darkening Albee A. L. and Chodos A. A. (1970) Microprobe investigations in the lunar highlands and identification of Descartes on Apollo 11 samples. Proc. Apollo 11 Lunar Sci. Conf., pp. material at the Apollo 16 site. Proc. Lunar Sci. Conf. 4th, 135–157. pp. 163–177. Albee A. L., Chodos A. A., Gancarz A. J., Haines E. L., Adams J. B., Pieters C., and McCord T. B. (1974) Orange Papanastassiou D. A., Ray L., Tera F., Wasserburg G. J., glass: Evidence for regional deposits of pyroclastic origin and Wen T. (1972) Mineralogy, petrology, and chemistry of on the Moon.