P2.152 Spring-Neap Tidal Patterns in North Atlantic

Total Page:16

File Type:pdf, Size:1020Kb

P2.152 Spring-Neap Tidal Patterns in North Atlantic P2.152 SPRING-NEAP TIDAL PATTERNS IN NORTH ATLANTIC TROPICAL CYCLONES Peter H. Yaukey* University of New Orleans, New Orleans, USA ABSTRACT spring-neap tidal cycle. Tropical cyclones are hypothesized to Atlantic best-track observations from reduce their own intensity by mixing of cool 1950-2007 displayed a pronounced peak of water upward, locally reducing the warmth of both hurricane occurrence and mean cyclone the sea surface. Little is known about how wind speed half way between the new and temperature variations in subsurface waters full moon. These patterns were consistent might moderate their influence on cyclones over time, being correlated between the first over sub-seasonal time scales. For instance, (1950-1978) and second (1979-2007) halves cold water might be mixed upward to depths of the study period. This pattern of hurricane accessible to storms by internal tidal waves occurrence was similar east and west of (bores) propagated along the thermocline. I 550W and in the Gulf of Mexico/Caribbean explored the possible influence of tidal mixing Sea, but appeared phase shifted by ~7 d on near-surface ocean temperature profiles north of 350N. Initiation dates of rapid and tropical cyclones by analyzing patterns of intensification events (≥15 kt increase in 24 h) cyclone frequency and intensity, and of were distributed non-uniformly across the subsurface water temperatures, across the synodic cycle, and showed peaks more ___________________________________ directly centered on the new (major peak) *Corresponding author address: Department and full moon (minor). of Geography, University of New Orleans, Water temperatures at 35-150m depth at New Orleans, LA, USA, 70148; e-mail: three long term moorings between 120N and [email protected]. 320N were each dominated by a peak near 1 the new moon, matching the timing of tracks, with especially large errors in the intensification events, although they varied in realm of rapid intensification (Rappaport et other details. Within 500 km of the 120N and al., 2009). The National Hurricane Center 150N moorings, cyclones that passed while has elevated improvements in intensity rapidly intensifying appeared to be associated forecasting to their top priority for tropical with warmer 35-150m waters than were other meteorology research. Intensification of passing cyclones. Evidence less consistent hurricanes is widely recognized to be affected with tidal influence include the presence of a by a variety of factors, including vertical wind relatively strong lunar pattern in hurricane shear, humidity, vorticity, and upper-level occurrence in the Gulf of Mexico and divergence. Ocean temperature is critical to Caribbean Sea where tides are weak, the storm intensification, including not just limited amplitude of spring-neap temperature surface temperature but also the depth of the variations (only 0.1-0.20C) and their surface layer of warm water (Hong et al., inconsistency across years at two of the 2000; Mao et al., 2000; Shay et al., 2000; mooring sites. Gino and Trinanes, 2003). The heat content of the uppermost KEY WORDS: Tropical cyclone; hurricane; ocean and variation of water temperature with rapid intensification; tidal; spring-neap. depth near the surface depend upon several factors, such as the presence and depth of 1. INTRODUCTION warm ocean currents and eddies, radiant Forecasting of hurricane intensity remains an fluxes, and wind. In recent years important challenge for tropical cyclone oceanographers have also become aware researchers. Accurate intensity forecasting is that much more tidal energy dissipation critical to warning coastal communities of the occurs away from the continental shelves level of threat posed by approaching storms, than was previously thought (Egbert and Ray, yet advances in forecasting intensity have not 2000; Garrett, 2003; Jayne, 2005; Thorpe, kept pace with those in predicting of storm 2005). The ability of tidal movements to 2 induce mixing of water near the ocean variations in the occurrence and intensity of surface is still not well understood, but mixing tropical cyclones across the spring-neap in the upper ocean has been reported from cycle. I then examine temperature modeling and empirical studies both far from fluctuations down to 150m at three long term (e.g., Martin, 2007; Schiller and Fiedler, moorings in the Atlantic, to assess whether 2007) and along continental shelves (e.g., sub-surface temperatures vary in a pattern Creswell and Badcock, 2000; Sharples et al., consistent with patterns exhibited by the 2006). Deep ocean tidal mixing is thought to cyclones. I focus on the Atlantic basin, where be generated at seafloor topographic the most complete and precise historical features, and it is not clear how far tidal database of storm wind speeds is available. energy can spread from these. One possible mechanism of spread is via movements of 2. METHODS internal waves along the thermocline. Such 2.1 Tropical cyclone records internal waves create predictable upwelling I obtained tropical cyclone records at 6 h and surface cooling with fortnightly intervals from June-November between 1950 periodicity, at least at several locations on the and 2007 from the best track analyses of the Pacific Coast of North America (Pineda 1991, National Hurricane Center’s North Atlantic 1995). At present, tidal variations in Hurricane Database (HURDAT, subsurface water temperatures are not http://www.nhc.noaa.gov/pastatll.shtml). incorporated into cyclone forecasting. Records prior to 1950 were excluded The purpose of this paper is investigate because most lacked data from the early whether the subsurface waters within reach (tropical depression) phase of storm of wind-induced mixing by passing cyclones development, and observations made north exhibit meaningful temporal variation on the of 500N or coded as “extratropical” were spring-neap tidal cycle, which might indicate omitted. The onset of rapid intensification the potential to influence cyclone was identified for storms that experienced a intensification. I begin by examining Rapid Intensification Event (RIE) of ≥15 knots 3 (7.7 ms-1) over 24 h. Intensification individual storm accounts in the National calculations did not begin until a storm was Hurricane Center online archives, and storm classified as a tropical or subtropical system track maps on the UNISYS website of at least depression strength, and (www.weather.unisys.com/hurricane). consecutive (beginning 6 h after another ended) or overlapping RIE were considered a 2.2 Ocean temperature single event. When a storm had more than Three moorings that have especially one RIE, that with the largest total wind lengthy records of sub-surface temperatures speed increase was used; maximum 6 h in cyclone-prone areas of the Atlantic were increase within the RIE was the second tie selected for analysis (Fig. 1). Two were breaker. To exclude RIEs caused merely by adjacent components of the PIRATA array landfall-weakened storms intensifying as they located at 12.00N 38.00N and 15.00N 38.00N, returned to sea, post-landfall RIE did not 333 km apart (available at begin until storms had regained their pre- http://www.pmel.noaa.gov/tao/data_deliv/deli landfall strength. If this happened in between v-nojava-pir.html). Daily temperature observations, the storm was assumed to readings were available from these moorings have regained it at the midpoint in between back to 1999 and 1998 respectively, at 20 m those observations. Pre-landfall wind speed depth intervals down to 140 m and at 180m. was taken from the last observation before For days that were missing data from a single the official track came ashore. For purposes depth or two adjacent depths that were other than RIE, observations within 3 d after bounded by measurements 20m above and being over land (coded as 10 x 10 blocks that below, missing temperatures were filled in by intersected land) were excluded. For all interpolation between the next deeper and purposes, only contacts with a continental shallower values, based simply on the mean mainland or Greater Antillean island relative magnitude of the missing depth’s constituted landfall. Identification of RIE and temperature between its two bounding depths landfalls in HURDAT was assisted by 4 in the overall data set. Days with more HURDAT observations posed challenges for missing data were omitted testing for statistical significance. I dealt with The third mooring, the Bermuda Testbed this problem in two ways. First, I compared site (31.70N 64.20W), has been operating patterns of cyclone occurrence and wind since 1994 (data available at http://www.opl. speed or ocean water temperature on the ucsb.edu/btm.html). Sensor depths here lunar cycle between the years in the first and have shifted over time and this analysis will second halves of the study period (1950- focus on the four depths that offer the 1978, 1979-2007 for cyclones) using simple greatest number of observations since the correlation; correlated patterns were mooring began: 3, 35, 70, and 150 m. The considered unlikely to be spurious. For this sensor depths used actually varied around purpose, each synodic cycle was partitioned each of these targets by as much as 1m (for into 30 equal “days” (cf. mean length of 29.53 the 3m depth), 5m (for 35m and 70m), or 9m d) and the frequency of hurricane (for 150m). When more than one sensor was observations, mean wind speed, or mean available at a given depth, only one was water temperature was calculated for each used- generally the Tidbit sensor because of
Recommended publications
  • Atmospheric Tidal Waves in the Troposphere and Lower Stratosphere Observed by Wuhan MST Radar
    2nd URSI AT-RASC, Gran Canaria, 28 May – 1 June 2018 Atmospheric tidal waves in the troposphere and lower stratosphere observed by Wuhan MST radar Haiyin Qing School of Physics and Electronic Engineering, Leshan Normal University, 614000, China Abstract 2. Data and Method In this paper, the observation data of the Wuhan MST radar in the whole 2012 are used making a statistical analysis on This paper mainly deals with the observation data of the low stratospheric and troposphere tidal waves. The Wuhan MST radar in 2012. The months of 12, 1, 2 are results show that: (1) the diurnal tide is the strongest and divided into winter; the months of 3, 4, 5 are divided into most of the time at low levels of Sunday tide is stronger spring; the months of 6, 7, 8 are divided into summer; and than the high tide of Sunday. (2) the amplitude of the tidal the months of 9,10,11 are divided into autumn. Then wave is not modulated by the fluctuation with a smaller choose the most complete data in the strength of 50 days to time scale than their periods, and only these waves with a carry out different tidal wave components in the four longer time scale than their periods can affect the variation seasons. The time resolution of the data is 0.5 h, and the of the amplitude of the tidal waves. slip time length is 4 days. Fitting time series of wind field data in time window by least square method, the fitting Keywords: MST radar; Atmospheric tidal waves; model is as follows: troposphere; stratosphere; planetary waves (1) 2 () =0+( +) 1.
    [Show full text]
  • Tidal Wind Oscillations in the Tropical Lower Atmosphere As Observed by Indian MST Radar
    Annales Geophysicae (2001) 19: 991–999 c European Geophysical Society 2001 Annales Geophysicae Tidal wind oscillations in the tropical lower atmosphere as observed by Indian MST Radar M. N. Sasi, G. Ramkumar, and V. Deepa Space Physics Laboratory Vikram Sarabhai Space Centre, Trivandrum 695 022, India Received: 7 November 2000 – Revised: 17 May 2001 – Accepted: 18 May 2001 Abstract. Diurnal tidal components in horizontal winds marised the salient features of the classical theory of tides measured by MST radar in the troposphere and lower strato- under various simplifying assumptions, such as motionless sphere over a tropical station Gadanki (13.5◦ N, 79.2◦ E) are atmosphere, zonal symmetry of the heat sources, etc. and presented for the autumn equinox, winter, vernal equinox and this classical theory is successful in explaining the major summer seasons. For this purpose radar data obtained over features of tidal oscillations in the upper atmosphere. How- many diurnal cycles from September 1995 to August 1996 ever, if the water vapour and ozone distribution have zonal are used. The results obtained show that although the sea- asymmetry, solar thermal excitation of these constituents will sonal variation of the diurnal tidal amplitudes in zonal and generate tidal modes with zonal wave numbers not equal to meridional winds is not strong, vertical phase propagation 1. This means that solar thermal excitation will not be able characteristics show significant seasonal variation. An at- to follow the apparent westward motion of the Sun. These tempt is made to simulate the diurnal tidal amplitudes and Sun-asynchronous tidal modes are known as nonmigrating phases in the lower atmosphere over Gadanki using classical modes.
    [Show full text]
  • 2021 Girls Spring Season
    2021 GIRLS' SPRING PROGRAM SEASON INFORMATION PACKET LAST UPDATED: WEDNESDAY, APRIL 7TH @ 10:00PM 2020-21 RETURN TO PLAY - MAKING YOUR SAFETY A PRIORITY C R E A T E D B Y V C U N I T E D S T A F F U S I N G R E S T O R E I L L I N O I S A N D J V A / U S A V / A A U V O L L E Y B A L L G U I D E L I N E S 2021 SPRING TRYOUTS 2020-21 Seaon - Return To Play - Making Your Safety Our Priority GET READY FOR THE 2021 SPRING SEASON WHY TRYOUTS? Even though we anticipate that the Pre-TRryouEt Cl-iniTcs aRre a gYreatO way Uto prTepar eC for tLhe uIpNcomiIngC club season early sessions will be in-house leagues, or simply keep your skills sharp during the year. Each session will focus on a we need to accomplish two goals with range of skills and include drills to sharpen your overall game and build our tryouts. First, to create a competitive training environment with your confidence as you prepare for the spring club season. players of similar ability and objectives. Second, is to be in a position to quickly U17 U16 U15 move to teams/tournament play when SATURDAY, APRIL 17 SATURDAY, APRIL 17 SATURDAY, APRIL 17 Illinois determines it is safe to do so. 9A-11A OR 1P-3P 9A-11A OR 1P-3P 9A-11A OR 1P-3P COST: $30 COST: $30 COST: $30 AGE GROUPS USA Volleyball and AAU Volleyball have U14 U13 U12-U11 changed the birthdate cutoff starting SATURDAY, APRIL 17 SATURDAY, APRIL 17 SATURDAY, APRIL 17 with the upcoming season.
    [Show full text]
  • Increasing Day-Length Induces Spring Flushing of Tropical Dry Forest Trees in the Absence of Rain
    Trees (2002) 16:445–456 DOI 10.1007/s00468-002-0185-3 ORIGINAL ARTICLE Guillermo Rivera · Stephen Elliott · Linda S. Caldas Guillermo Nicolossi · Vera T. R. Coradin Rolf Borchert Increasing day-length induces spring flushing of tropical dry forest trees in the absence of rain Received: 10 September 2001 / Accepted: 26 March 2002 / Published online: 20 July 2002 © Springer-Verlag 2002 Abstract In many conspecific trees of >50 species high- synthetic gain in tropical forests with a relatively short ly synchronous bud break with low inter-annual varia- growing season. tion was observed during the late dry season, around the spring equinox, in semideciduous tropical forests of Keywords Bud break · Phenology · Photoperiodic Argentina, Costa Rica, Java and Thailand and in tropical control · Tropical semideciduous forests savannas of Central Brazil. Bud break was 6 months out of phase between the northern and southern hemispheres and started about 1 month earlier in the subtropics than Introduction at lower latitudes. These observations indicate that “spring flushing”, i.e., synchronous bud break around the In cold-temperate forests, vegetative phenology of all spring equinox and weeks before the first rains of the broad-leaved trees is strongly synchronized by winter wet season, is induced by an increase in photoperiod of cold. In contrast, severe seasonal drought does not syn- 30 min or less. Spring flushing is common in semidecid- chronize vegetative phenology in tropical semideciduous uous forests characterized by a 4–6 month dry season forests with a dry season of 4–6 months and annual rain- and annual rainfall of 800–1,500 mm, but rare in neo- fall between 800 and 1,500 mm.
    [Show full text]
  • ESSENTIALS of METEOROLOGY (7Th Ed.) GLOSSARY
    ESSENTIALS OF METEOROLOGY (7th ed.) GLOSSARY Chapter 1 Aerosols Tiny suspended solid particles (dust, smoke, etc.) or liquid droplets that enter the atmosphere from either natural or human (anthropogenic) sources, such as the burning of fossil fuels. Sulfur-containing fossil fuels, such as coal, produce sulfate aerosols. Air density The ratio of the mass of a substance to the volume occupied by it. Air density is usually expressed as g/cm3 or kg/m3. Also See Density. Air pressure The pressure exerted by the mass of air above a given point, usually expressed in millibars (mb), inches of (atmospheric mercury (Hg) or in hectopascals (hPa). pressure) Atmosphere The envelope of gases that surround a planet and are held to it by the planet's gravitational attraction. The earth's atmosphere is mainly nitrogen and oxygen. Carbon dioxide (CO2) A colorless, odorless gas whose concentration is about 0.039 percent (390 ppm) in a volume of air near sea level. It is a selective absorber of infrared radiation and, consequently, it is important in the earth's atmospheric greenhouse effect. Solid CO2 is called dry ice. Climate The accumulation of daily and seasonal weather events over a long period of time. Front The transition zone between two distinct air masses. Hurricane A tropical cyclone having winds in excess of 64 knots (74 mi/hr). Ionosphere An electrified region of the upper atmosphere where fairly large concentrations of ions and free electrons exist. Lapse rate The rate at which an atmospheric variable (usually temperature) decreases with height. (See Environmental lapse rate.) Mesosphere The atmospheric layer between the stratosphere and the thermosphere.
    [Show full text]
  • Spring Winter Summer Autumn
    • Always drive on good, properly inflated issouri is a state of four seasons tires. and each season has its own unique road conditions. Missouri driving • Know and obey all traffic laws. cannot be categorized entirely into spring, summer, autumn, or winter. Nature some- • Be ready to adjust your speed to be ap- times mixes our four seasons together, and propriate for constantly changing driving this can cause problems when we travel. conditions. This brochure has been prepared to give you some tips on how to handle our Finally, let’s all work together, so fewer many varied driving conditions. people will become traffic crash statistics on Missouri’s highways. Spring Buckle Up Missouri! • Never drive when you have been drink- ing alcoholic beverages. Summer • Never ride with someone who has been drinking. • If medication directions indicate you should not drive after taking it, don’t do Feel free to call the it. Road Condition Report Hotline at: Produced by: Public Information and Education Division • Have a good attitude when you drive. Be Published by: Autumn patient with others. 1-888-275-6636 Missouri State Highway Patrol 1510 East Elm Street • Give driving your full attention. Behind Or, check the Patrol’s Jefferson City, MO 65101 the wheel is no place to read, put on 573-751-3313 makeup, or talk on the cell phone. web site at: V/TDD 573-751-3313 email: [email protected] • How about those eyes? Don’t be vain. If www.mshp.dps.mo.gov www.mshp.dps.mo.gov Winter you need glasses, wear them.
    [Show full text]
  • Excitations of the Earth and Mars' Variable Rotations by Surficial Fluids
    Excitations of the Earth and Mars’ Variable Rotations by Surficial Fluids YH Zhou1, XQ Xu1, CC Xu1, JL Chen2, D Salstein3 1Shanghai Astronomical Observatory, CAS, China 2Center for Space Research, UT Austin, USA 3Atmospheric and Environmental Research, USA Outline Earth’s variable rotation Differences between NCEP/NCAR and ECMWF atmospheric excitation functions Atmospheric excitation of Mars’ rotation Mars’ semidiurnal LOD amplitude and the dust cycles during the Martian Years 24-31 Summary and discussion Earth rotation and Geophysical excitation function LOD change (Axial component, 풎ퟑ) Earth rotation vector (3-Dimentional) Polar motion (Equatorial components, 풎 = 풎ퟏ + 풊풎ퟐ) Axial term Geophysical excitation function Equatorial terms Atmospheric excitation of Earth’s variable rotation Atmospheric activity is the most important source for exciting the Earth’s short-period variations. Wind term (due to atmospheric wind) Atmospheric excitation function dominant source to LOD Change Pressure Term (due to change of air pressure) main source to Polar motion The AEF is archived and updated in IERS SBA website. Atmospheric Circulations Atmospheric GCM US:NCEP/NCAR Europe:ECMWF JMA:JMA China:LASG How large are Differences between NCEP/NCAR and ECMWF? NCEP/NCAR VS ECMWF Temporal resolution:6 hours Spatial resolution ퟐ. ퟓ° × ퟐ. ퟓ° 0.75° × 0.75° NCEP/NCAR VS ECMWF Pressure field: Similar AEF Differences: 3% AEF of ECMWF correlates slightly better with Earth rotation than that of NCEP/NCAR Wind field 37 levels 1 hPa 2 hPa 3 hPa 10-1 5 hPa 17 levels hPa 7 hPa 10 hPa 10 hPa 20 hPa 20 hPa 30 hPa 30 hPa • •• •• • 850 hPa 850 hPa 875 hPa 900 hPa 925 hPa 925 hPa 950 hPa 975 hPa 1000 hPa 1000 hPa Earth vs.
    [Show full text]
  • Using Surface Pressure Variations to Study Atmospheric Disturbances Generated by Diurnal Heating
    P6M.2 Using surface pressure variations to study atmospheric disturbances generated by diurnal heating Yanping Li and Ronald B. Smith Department of Geology and Geophysics Yale University, Connecticut, USA 1. Phenomena: Our interpretation of the data is guided by the assumption Solar heating generates a diurnal cycle in temperature, winds that the diurnal signal is the sum of three parts and pressure over the Earth. The direct solar heating of the • Global atmospheric tide driven mostly by solar heating of atmosphere (e.g. absorption by ozone in the stratosphere) can the stratosphere (westward moving at about 350m/s at act everywhere (Chapman and Lindzen, 1970), whereas 40ο N ). indirect heating through surface fluxes will be • Continentally enhanced Tide driven by surface heat fluxes. inhomogeneous. Over land, the surface receives heat and • Mesoscale disturbance related to variations in the earth transports it upward by small scale convection. The Rocky surface (mountain, coast, or land cover). These Mountains is a typical area for this (Banta and Schaaf, 1987). disturbances are driven locally by surface heat flux Several responses to diurnal heating are possible, e.g. sea gradients, but they can propagate away using various breeze and mountain–plain circulation. Carbone et al. (2002), mechanisms: e.g. gravity waves, PV pulses, storm using radar composites, found eastward propagating diurnal dynamics. precipitation systems over the Great Plains and the Mid-west, We call the sum of the first and the second parts as the moving at a speed of about 20m/s. atmospheric tide, since it has the same west-propagating In some other areas, such as the Bay of Bengal, satellites speed as that of the Sun.
    [Show full text]
  • Assessment of Sun Photometer Langley Calibration at the High-Elevation Sites Mauna Loa and Izaña
    Atmos. Chem. Phys., 18, 14555–14567, 2018 https://doi.org/10.5194/acp-18-14555-2018 © Author(s) 2018. This work is distributed under the Creative Commons Attribution 4.0 License. Assessment of Sun photometer Langley calibration at the high-elevation sites Mauna Loa and Izaña Carlos Toledano1, Ramiro González1, David Fuertes1,2, Emilio Cuevas3, Thomas F. Eck4,5, Stelios Kazadzis6, Natalia Kouremeti6, Julian Gröbner6, Philippe Goloub7, Luc Blarel7, Roberto Román1, África Barreto8,3,1, Alberto Berjón1, Brent N. Holben4, and Victoria E. Cachorro1 1Group of Atmospheric Optics, University of Valladolid (GOA-UVa), Valladolid, Spain 2GRASP-SAS, Lille, France 3Izaña Atmospheric Research Center, Meteorological State Agency of Spain (AEMET), Tenerife, Spain 4NASA Goddard Space Flight Center, Greenbelt, MD, USA 5Universities Space Research Association, Columbia, MD, USA 6Physikalisch-Meteorologisches Observatorium Davos, World Radiation Centre – PMOD/WRC, Davos, Switzerland 7Laboratory of Atmospheric Optics, University of Lille, Villeneuve-d’Ascq, France 8Cimel Electronique, Paris, France Correspondence: Carlos Toledano ([email protected]) Received: 28 April 2018 – Discussion started: 14 May 2018 Revised: 21 August 2018 – Accepted: 6 September 2018 – Published: 11 October 2018 Abstract. The aim of this paper is to analyze the suitability uncertainty of ∼ 0.25–0.5 %, this uncertainty being smaller of the high-mountain stations Mauna Loa and Izaña for Lan- in the visible and near-infrared wavelengths and larger in the gley plot calibration of Sun
    [Show full text]
  • A Review of Droughts in the African Continent: a Geospatial and Long
    Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Open Access Hydrol. Earth Syst. Sci. Discuss., 11, 2679–2718, 2014 Hydrology and www.hydrol-earth-syst-sci-discuss.net/11/2679/2014/ Earth System doi:10.5194/hessd-11-2679-2014 © Author(s) 2014. CC Attribution 3.0 License. Sciences Discussions This discussion paper is/has been under review for the journal Hydrology and Earth System Sciences (HESS). Please refer to the corresponding final paper in HESS if available. A review of droughts in the African continent: a geospatial and long-term perspective I. Masih1, S. Maskey1, F. E. F. Mussá1,2, and P. Trambauer1 1UNESCO-IHE, Institute for Water Education, P.O. Box 3015, 2601 DA Delft, the Netherlands 2Eduardo Mondlane University, Faculty of Engineering, Av. de Moçambique km 1.5, C. Postal 257, Maputo, Mozambique Received: 31 January 2014 – Accepted: 3 February 2014 – Published: 6 March 2014 Correspondence to: I. Masih ([email protected]) Published by Copernicus Publications on behalf of the European Geosciences Union. 2679 Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Abstract This paper presents a comprehensive review and analysis of the available literature and information on droughts to build a continental, regional and country level perspective on geospatial and temporal variation of droughts in Africa. The study is based on 5 the review and analysis of droughts occurred during 1900–2013 as well as evidence available from past centuries based on studies on the lake sediment analysis, tree- ring chronologies and written and oral histories and future predictions from the global climate change models.
    [Show full text]
  • The Rotation of Planets Hosting Atmospheric Tides: from Venus to Habitable Super-Earths P
    A&A 603, A108 (2017) Astronomy DOI: 10.1051/0004-6361/201628701 & c ESO 2017 Astrophysics The rotation of planets hosting atmospheric tides: from Venus to habitable super-Earths P. Auclair-Desrotour1; 2, J. Laskar1, S. Mathis2; 3, and A. C. M. Correia1; 4 1 IMCCE, Observatoire de Paris, CNRS UMR 8028, PSL, 77 Avenue Denfert-Rochereau, 75014 Paris, France e-mail: [email protected] 2 Laboratoire AIM Paris-Saclay, CEA/DRF – CNRS – Université Paris Diderot, IRFU/SAp Centre de Saclay, 91191 Gif-sur-Yvette Cedex, France e-mail: [email protected] 3 LESIA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Univ. Paris 06, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon, France 4 CIDMA, Departamento de Física, Universidade de Aveiro, Campus de Santiago, 3810-193 Aveiro, Portugal e-mail: [email protected] Received 12 April 2016 / Accepted 17 November 2016 ABSTRACT The competition between the torques induced by solid and thermal tides drives the rotational dynamics of Venus-like planets and super-Earths orbiting in the habitable zone of low-mass stars. The resulting torque determines the possible equilibrium states of the planet’s spin. Here we have computed an analytic expression for the total tidal torque exerted on a Venus-like planet. This expression is used to characterize the equilibrium rotation of the body. Close to the star, the solid tide dominates. Far from it, the thermal tide drives the rotational dynamics of the planet. The transition regime corresponds to the habitable zone, where prograde and retrograde equilibrium states appear.
    [Show full text]
  • Tide 1 Tides Are the Rise and Fall of Sea Levels Caused by the Combined
    Tide 1 Tide The Bay of Fundy at Hall's Harbour, The Bay of Fundy at Hall's Harbour, Nova Scotia during high tide Nova Scotia during low tide Tides are the rise and fall of sea levels caused by the combined effects of the gravitational forces exerted by the Moon and the Sun and the rotation of the Earth. Most places in the ocean usually experience two high tides and two low tides each day (semidiurnal tide), but some locations experience only one high and one low tide each day (diurnal tide). The times and amplitude of the tides at the coast are influenced by the alignment of the Sun and Moon, by the pattern of tides in the deep ocean (see figure 4) and by the shape of the coastline and near-shore bathymetry.[1] [2] [3] Most coastal areas experience two high and two low tides per day. The gravitational effect of the Moon on the surface of the Earth is the same when it is directly overhead as when it is directly underfoot. The Moon orbits the Earth in the same direction the Earth rotates on its axis, so it takes slightly more than a day—about 24 hours and 50 minutes—for the Moon to return to the same location in the sky. During this time, it has passed overhead once and underfoot once, so in many places the period of strongest tidal forcing is 12 hours and 25 minutes. The high tides do not necessarily occur when the Moon is overhead or underfoot, but the period of the forcing still determines the time between high tides.
    [Show full text]