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Artigos de revistas sobre o tema "Atmospheric tides"

Autor: Grafiati

Publicado: 4 de junho de 2021

Última modificação: 25 de julho de 2025

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1

Palumbo, A. "Atmospheric tides." Journal of Atmospheric and Solar-Terrestrial Physics 60, no. 3 (1998): 279–87. http://dx.doi.org/10.1016/s1364-6826(97)00078-3.

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2

Auclair-Desrotour, P., S. Mathis, and J. Laskar. "Atmospheric thermal tides and planetary spin." Astronomy & Astrophysics 609 (January 2018): A118. http://dx.doi.org/10.1051/0004-6361/201731540.

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Context. Thermal atmospheric tides can torque telluric planets away from spin-orbit synchronous rotation, as observed in the case of Venus. They thus participate in determining the possible climates and general circulations of the atmospheres of these planets. Aims. The thermal tidal torque exerted on an atmosphere depends on its internal structure and rotation and on the tidal frequency. Particularly, it strongly varies with the convective stability of the entropy stratification. This dependence has to be characterized to constrain and predict the rotational properties of observed telluric ex

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3

Auclair-Desrotour, P., J. Laskar, and S. Mathis. "Atmospheric tides in Earth-like planets." Astronomy & Astrophysics 603 (July 2017): A107. http://dx.doi.org/10.1051/0004-6361/201628252.

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Context. Atmospheric tides can strongly affect the rotational dynamics of planets. In the family of Earth-like planets, which includes Venus, this physical mechanism coupled with solid tides makes the angular velocity evolve over long timescales and determines the equilibrium configurations of their spin. Aims. Unlike the solid core, the atmosphere of a planet is subject to both tidal gravitational potential and insolation flux coming from the star. The complex response of the gas is intrinsically linked to its physical properties. This dependence has to be characterized and quantified for app

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4

Navarro, Thomas, Timothy M. Merlis, Nicolas B. Cowan, and Natalya Gomez. "Atmospheric Gravitational Tides of Earth-like Planets Orbiting Low-mass Stars." Planetary Science Journal 3, no. 7 (2022): 162. http://dx.doi.org/10.3847/psj/ac76cd.

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Abstract Temperate terrestrial planets orbiting low-mass stars are subject to strong tidal forces. The effects of gravitational tides on the solid planet and that of atmospheric thermal tides have been studied, but the direct impact of gravitational tides on the atmosphere itself has so far been ignored. We first develop a simplified analytic theory of tides acting on the atmosphere of a planet. We then implement gravitational tides into a general circulation model of a static-ocean planet in a short-period orbit around a low-mass star—the results agree with our analytic theory. Because atmosp

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5

Auclair-Desrotour, P., J. Laskar, and S. Mathis. "Atmospheric tides and their consequences on the rotational dynamics of terrestrial planets." EAS Publications Series 82 (2019): 81–90. http://dx.doi.org/10.1051/eas/1982008.

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Atmospheric tides can have a strong impact on the rotational dynamics of planets. They are of most importance for terrestrial planets located in the habitable zone of their host star, where their competition with solid tides is likely to drive the body towards non-synchronized rotation states of equilibrium, as observed in the case of Venus. Contrary to other planetary layers, the atmosphere is sensitive to both gravitational and thermal forcings, through a complex dynamical coupling involving the effects of Coriolis acceleration and characteristics of the atmospheric structure. These key phys

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6

Brahde, R. "Lunisolar Atmospheric Tides. II." Australian Journal of Physics 42, no. 4 (1989): 439. http://dx.doi.org/10.1071/ph890439.

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In an earlier paper (Brahde 1988) it was shown that series of measurements of the atmospheric pressure in Oslo contained information about a one�day oscillation with mean amplitude 0�17 mb. The data consisted of measurements every second hour during the years 1957-67, 1969 and 1977. In the present paper the intervening years plus 1978 and 1979 have been included, increasing the basis from 13 to 23 years. In addition the phase shift occurring when the Moon crosses the celestial equator has been defined precisely, thus making it possible to include all the data.

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7

Brahde, R. "Lunisolar Atmospheric Tides. III." Australian Journal of Physics 44, no. 1 (1991): 87. http://dx.doi.org/10.1071/ph910087.

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In two earlier papers (Brahde 1988, 1989) the atmospheric tide in Oslo (Norway) was studied using pressure data for 23 continuous years. In the present paper a similar study based on pressure data from Batavia (now Jakarta in Indonesia, latitude 6�08'S, longitude 106�45'E) is presented. The result is that the tidal wave caused by the lunisolar tide is represented by a one-day and a half-day oscillation with mean amplitudes of 0 �11 and 0�33 mb respectively. The amplitude spectrum reveals amplitudes of up to 1 mb of dynamiC origin. The 'thermal' tide is also studied and the connection between t

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8

FORBES, Jeffrey M. "Middle Atmosphere Tides and Coupling between Atmospheric Regions." Journal of geomagnetism and geoelectricity 43, Supplement2 (1991): 597–609. http://dx.doi.org/10.5636/jgg.43.supplement2_597.

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9

Salazar, Andrea M., and Robin Wordsworth. "The Feasibility of Asynchronous Rotation via Thermal Tides for Diverse Atmospheric Compositions." Planetary Science Journal 5, no. 10 (2024): 218. http://dx.doi.org/10.3847/psj/ad74ef.

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Abstract The equilibrium rotation rate of a planet is determined by the sum of torques acting on its solid body. For planets with atmospheres, the dominant torques are usually the gravitational tide, which acts to slow the planet’s rotation rate, and the atmospheric thermal tide, which acts to spin up the planet. Previous work demonstrated that rocky planets with thick atmospheres may produce strong enough thermal tides to avoid tidal locking, but a study of how the strength of the thermal tide depends on atmospheric properties has not been done. In this work, we use a combination of simulatio

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10

Biagi, P. F., R. Piccolo, V. Capozzi, A. Ermini, S. Martellucci, and C. Bellecci. "Exalting in atmospheric tides as earthquake precursor." Natural Hazards and Earth System Sciences 3, no. 3/4 (2003): 197–201. http://dx.doi.org/10.5194/nhess-3-197-2003.

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Abstract. During February–March 1998, we observed a significant increase (6–8 dB) in the electric field of the CZE (f = 270 kHz, Czech Republic) broadcasting station at a site named AS and located in central Italy. On 13 March 1998 an earthquake (M = 5.2) occurred in Slovenia, starting a strong seismic crisis (M = 6.0 on 12 April, M = 5.1 on 6 May). The distances of the epicentres from the radio receiver were over 400 km, but the epicentres are located in a zone that is in the middle of the CZE-AS path. Previously, we advanced the hypothesis that the increase of radio-signal electric field det

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11

Forbes, Jeffrey M., and Gerald V. Groves. "Atmospheric tides below 80 km." Advances in Space Research 10, no. 12 (1990): 119–25. http://dx.doi.org/10.1016/0273-1177(90)90391-c.

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12

Cunha, Diana, Alexandre C. M. Correia, and Jacques Laskar. "Spin evolution of Earth-sized exoplanets, including atmospheric tides and core–mantle friction." International Journal of Astrobiology 14, no. 2 (2014): 233–54. http://dx.doi.org/10.1017/s1473550414000226.

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AbstractPlanets with masses between 0.1 and 10 M⊕ are believed to host dense atmospheres. These atmospheres can play an important role on the planet's spin evolution, since thermal atmospheric tides, driven by the host star, may counterbalance gravitational tides. In this work, we study the long-term spin evolution of Earth-sized exoplanets. We generalize previous works by including the effect of eccentric orbits and obliquity. We show that under the effect of tides and core–mantle friction, the obliquity of the planets evolves either to 0° or 180°. The rotation of these planets is also expect

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13

Hagen, Jonas, Klemens Hocke, Gunter Stober, Simon Pfreundschuh, Axel Murk, and Niklaus Kämpfer. "First measurements of tides in the stratosphere and lower mesosphere by ground-based Doppler microwave wind radiometry." Atmospheric Chemistry and Physics 20, no. 4 (2020): 2367–86. http://dx.doi.org/10.5194/acp-20-2367-2020.

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Abstract. Atmospheric tides are important for vertical coupling in the atmosphere, from the stratosphere down to the troposphere and up to the thermosphere. They are planetary-scale gravity waves with well-known periods that are integer fractions of a day and can be observed in the temperature or wind fields in the atmosphere. Most lidar techniques and satellites measure atmospheric tides only in the temperature field and continuous measurements of the tides in the wind field of the stratosphere and lower mesosphere are rare, even though, with modern lidars, they would be feasible. In this stu

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14

Krochin, Witali, Axel Murk, and Gunter Stober. "Thermal tides in the middle atmosphere at mid-latitudes measured with a ground-based microwave radiometer." Atmospheric Measurement Techniques 17, no. 17 (2024): 5015–28. http://dx.doi.org/10.5194/amt-17-5015-2024.

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Abstract. In recent decades, theoretical studies and numerical models of thermal tides have gained attention. It has been recognized that tides have a significant influence on the dynamics of the middle and upper atmosphere; as they grow in amplitude and propagate upward, they transport energy and momentum from the lower to the upper atmosphere, contributing to the vertical coupling between atmospheric layers. The superposition of tides with other atmospheric waves leads to non-linear wave–wave interactions. However, direct measurements of thermal tides in the middle atmosphere are challenging

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15

Lindzen, Richard S. "Richard J. Reed and Atmospheric Tides." Meteorological Monographs 53 (December 1, 2003): 85–89. http://dx.doi.org/10.1175/0065-9401-31.53.85.

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16

Palumbo, A. "Reply to comments on "Atmospheric Tides"." Journal of Atmospheric and Solar-Terrestrial Physics 60, no. 18 (1998): 1793. http://dx.doi.org/10.1016/s1364-6826(98)00148-5.

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17

Price, Colin, Ron Maor, and Hofit Shachaf. "Using smartphones for monitoring atmospheric tides." Journal of Atmospheric and Solar-Terrestrial Physics 174 (September 2018): 1–4. http://dx.doi.org/10.1016/j.jastp.2018.04.015.

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18

Brahde, R. "Lunisolar Atmospheric Tides: A New Approach." Australian Journal of Physics 41, no. 6 (1988): 807. http://dx.doi.org/10.1071/ph880807.

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In records of the atmospheric pressure in Oslo, at 60' latitude, a one-day oscillation caused by the lunisolar tide has been detected. The amplitude has a mean value of O� 17 mb. This oscillation appears during intervals when the declination of the Moon has high numerical values. When the Moon passes through the equator, the one-day oscillation disappears and only the half-day mode continues. If a maximum coincides with upper culmination, it reappears during the next fortnight at lower culmination. This means that the phase changes approximately 180' or 12h every time the Moon crosses the equa

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19

French, Richard G., Anthony D. Toigo, Peter J. Gierasch, et al. "Seasonal variations in Pluto’s atmospheric tides." Icarus 246 (January 2015): 247–67. http://dx.doi.org/10.1016/j.icarus.2014.05.017.

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20

Guzewich, Scott D., C. E. Newman, M. de la Torre Juárez, et al. "Atmospheric tides in Gale Crater, Mars." Icarus 268 (April 2016): 37–49. http://dx.doi.org/10.1016/j.icarus.2015.12.028.

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21

Wergen, W. "Normal mode initialization and atmospheric tides." Quarterly Journal of the Royal Meteorological Society 115, no. 487 (1989): 535–45. http://dx.doi.org/10.1002/qj.49711548706.

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22

Hupe, Patrick, Lars Ceranna, and Christoph Pilger. "Using barometric time series of the IMS infrasound network for a global analysis of thermally induced atmospheric tides." Atmospheric Measurement Techniques 11, no. 4 (2018): 2027–40. http://dx.doi.org/10.5194/amt-11-2027-2018.

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Abstract. The International Monitoring System (IMS) has been established to monitor compliance with the Comprehensive Nuclear-Test-Ban Treaty and comprises four technologies, one of which is infrasound. When fully established, the IMS infrasound network consists of 60 sites uniformly distributed around the globe. Besides its primary purpose of determining explosions in the atmosphere, the recorded data reveal information on other anthropogenic and natural infrasound sources. Furthermore, the almost continuous multi-year recordings of differential and absolute air pressure allow for analysing t

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23

Tokioka, Tatsushi, and Isamu Yagai. "Atmospheric Tides Appearing in a Global Atmospheric General Circulation Model." Journal of the Meteorological Society of Japan. Ser. II 65, no. 3 (1987): 423–38. http://dx.doi.org/10.2151/jmsj1965.65.3_423.

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24

Covey, Curt, Aiguo Dai, Dan Marsh, and Richard S. Lindzen. "The Surface-Pressure Signature of Atmospheric Tides in Modern Climate Models." Journal of the Atmospheric Sciences 68, no. 3 (2011): 495–514. http://dx.doi.org/10.1175/2010jas3560.1.

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Abstract Although atmospheric tides driven by solar heating are readily detectable at the earth’s surface as variations in air pressure, their simulations in current coupled global climate models have not been fully examined. This work examines near-surface-pressure tides in climate models that contributed to the Fourth Assessment Report of the Intergovernmental Panel on Climate Change (IPCC); it compares them with tides both from observations and from the Whole Atmosphere Community Climate Model (WACCM), which extends from the earth’s surface to the thermosphere. Surprising consistency is fou

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25

Charnay, B., G. Tobie, S. Lebonnois, and R. D. Lorenz. "Gravitational atmospheric tides as a probe of Titan’s interior: Application to Dragonfly." Astronomy & Astrophysics 658 (February 2022): A108. http://dx.doi.org/10.1051/0004-6361/202141898.

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Context. Saturn’s massive gravity is expected to causes a tide in Titan’s atmosphere, producing a surface pressure variation through the orbit of Titan and tidal winds in the troposphere. The future Dragonfly mission could analyse this exotic meteorological phenomenon. Aims. We aim to analyse the effect of Saturn’s tides on Titan’s atmosphere and interior to determine how pressure measurements by Dragonfly could constrain Titan’s interior. Methods. We model atmospheric tides with analytical calculations and with a 3D global climate model (the IPSL-Titan GCM), including the tidal response of th

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26

Griffith, Matthew J., and Nicholas J. Mitchell. "Analysis of migrating and non-migrating tides of the Extended Unified Model in the mesosphere and lower thermosphere." Annales Geophysicae 40, no. 3 (2022): 327–58. http://dx.doi.org/10.5194/angeo-40-327-2022.

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Abstract. Atmospheric tides play a key role in coupling the lower, middle, and upper atmosphere/ionosphere. The tides reach large amplitudes in the mesosphere and lower thermosphere (MLT), where they can have significant fluxes of energy and momentum, and so strongly influence the coupling and dynamics. The tides must therefore be accurately represented in general circulation models (GCMs) that seek to model the coupling of atmospheric layers and impacts on the ionosphere. The tides consist of both migrating (sun-following) and non-migrating (not sun-following) components, both of which have i

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27

Braswell, William D., and Richard S. Lindzen. "Anomalous short wave absorption and atmospheric tides." Geophysical Research Letters 25, no. 9 (1998): 1293–96. http://dx.doi.org/10.1029/98gl01031.

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28

Andruk, V., G. Butenko, V. Kostyuchenko, and L. Svachij. "The relation between extinction and atmospheric tides." Journal of Physical Studies 11, no. 4 (2007): 432–37. http://dx.doi.org/10.30970/jps.11.432.

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29

Arabelos, D., G. Asteriadis, M. E. Contadakis, S. D. Spatalas, and H. Sachsamanoglou. "Atmospheric tides in the area of Thessaloniki." Journal of Geodynamics 23, no. 1 (1997): 65–75. http://dx.doi.org/10.1016/s0264-3707(96)00018-x.

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30

Zharov, V. E., and D. Gambis. "Atmospheric tides and rotation of the Earth." Journal of Geodesy 70, no. 6 (1996): 321–26. http://dx.doi.org/10.1007/bf00868183.

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31

Zharov, V. E., and D. Gambis. "Atmospheric tides and rotation of the Earth." Journal of Geodesy 70, no. 6 (1996): 321–26. http://dx.doi.org/10.1007/s001900050022.

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32

Balcerak, Ernie. "Atmospheric tides link stratosphere and ionosphere changes." Eos, Transactions American Geophysical Union 95, no. 24 (2014): 208. http://dx.doi.org/10.1002/2014eo240008.

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33

Covey, Curt, Aiguo Dai, Richard S. Lindzen, and Daniel R. Marsh. "Atmospheric Tides in the Latest Generation of Climate Models*." Journal of the Atmospheric Sciences 71, no. 6 (2014): 1905–13. http://dx.doi.org/10.1175/jas-d-13-0358.1.

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Abstract For atmospheric tides driven by solar heating, the database of climate model output used in the most recent assessment report of the Intergovernmental Panel on Climate Change (IPCC) confirms and extends the authors’ earlier results based on the previous generation of models. Both the present study and the earlier one examine the surface pressure signature of the tides, but the new database removes a shortcoming of the earlier study in which model simulations were not strictly comparable to observations. The present study confirms an approximate consistency among observations and all m

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34

Williams, Joanne, Maialen Irazoqui Apecechea, Andrew Saulter, and Kevin J. Horsburgh. "Radiational tides: their double-counting in storm surge forecasts and contribution to the Highest Astronomical Tide." Ocean Science 14, no. 5 (2018): 1057–68. http://dx.doi.org/10.5194/os-14-1057-2018.

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Abstract. Tide predictions based on tide-gauge observations are not just the astronomical tides; they also contain radiational tides – periodic sea-level changes due to atmospheric conditions and solar forcing. This poses a problem of double-counting for operational forecasts of total water level during storm surges. In some surge forecasting, a regional model is run in two modes: tide only, with astronomic forcing alone; and tide and surge, forced additionally by surface winds and pressure. The surge residual is defined to be the difference between these configurations and is added to the loc

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35

Harris, M. J., N. F. Arnold, and A. D. Aylward. "A study into the effect of the diurnal tide on the structure of the background mesosphere and thermosphere using the new coupled middle atmosphere and thermosphere (CMAT) general circulation model." Annales Geophysicae 20, no. 2 (2002): 225–35. http://dx.doi.org/10.5194/angeo-20-225-2002.

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Abstract. A new coupled middle atmosphere and thermosphere general circulation model has been developed, and some first results are presented. An investigation into the effects of the diurnal tide upon the mean composition, dynamics and energetics was carried out for equinox conditions. Previous studies have shown that tides deplete mean atomic oxygen in the upper mesosphere-lower thermosphere due to an increased recombination in the tidal displaced air parcels. The model runs presented suggest that the mean residual circulation associated with the tidal dissipation also plays an important rol

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36

Shved, G. M., L. N. Petrova, and O. S. Polyakova. "Penetration of the Earth's free oscillations at 54 minute period into the atmosphere." Annales Geophysicae 18, no. 5 (2000): 566–72. http://dx.doi.org/10.1007/s00585-000-0566-0.

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Abstract. It is known that the fundamental spheroidal mode 0S2 of the Earth free oscillation with a period of about 54 min forces atmospheric oscillations. We present a certain phase relationship for components of the 0S2 multiplet, which is based on synchronous collocated microbarograph and seismograph observations. This relationship is both the first observational manifestation of the Pekeris mode of global atmospheric oscillations with the 54 min period and a further proof of the Earth's 0S2 mode penetrating into the atmosphere. We show that the linear non-dissipative model of steady forced

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37

Pan, Q. W., J. E. Allnutt, and C. Tsui. "Evidence of atmospheric tides from satellite beacon experiment." Electronics Letters 42, no. 12 (2006): 706. http://dx.doi.org/10.1049/el:20060408.

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38

Vial, François. "Numerical simulations of atmospheric tides for solstice conditions." Journal of Geophysical Research 91, A8 (1986): 8955. http://dx.doi.org/10.1029/ja091ia08p08955.

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39

Forbes, Jeffrey M. "Atmospheric tides between 80 km and 120 km." Advances in Space Research 10, no. 12 (1990): 127–40. http://dx.doi.org/10.1016/0273-1177(90)90392-d.

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40

Bartzokas, A., C. C. Repapis, and D. A. Metaxas. "Temporal variations of atmospheric tides over Athens, Greece." Meteorology and Atmospheric Physics 55, no. 1-2 (1995): 113–23. http://dx.doi.org/10.1007/bf01029606.

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41

Bills, Bruce G., Thomas Navarro, Gerald Schubert, Anton Ermakov, and Krzysztof M. Górski. "Gravitational signatures of atmospheric thermal tides on Venus." Icarus 340 (April 2020): 113568. http://dx.doi.org/10.1016/j.icarus.2019.113568.

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42

Palus, Shannon. "Role of lunar atmospheric tides in thermosphere density." Eos, Transactions American Geophysical Union 95, no. 47 (2014): 444. http://dx.doi.org/10.1002/2014eo470012.

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43

Livesey, Joseph R., Juliette Becker, and Susanna L. Widicus Weaver. "Tides Tighten the Hycean Habitable Zone." Astrophysical Journal Letters 987, no. 1 (2025): L8. https://doi.org/10.3847/2041-8213/ade434.

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Abstract Hycean planets—exoplanets with substantial water ice layers, deep surface oceans, and hydrogen-rich atmospheres—are thought to be favorable environments for life. Due to a relative paucity of atmospheric greenhouse gases, hycean planets have been thought to have wider habitable zones (HZs) than Earth-like planets, extending down to a few times 10−3 au for those orbiting M dwarfs. In this Letter, we reconsider the hycean HZ accounting for star–planet tidal interaction. We show that for a moderately eccentric hycean planet, the surface temperature contribution from tidal heating truncat

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44

REDDY, S. JEEV ANANDA. "Lunar and solar atmospheric tides in surface winds and rainfall." MAUSAM 25, no. 3 (2022): 499–502. http://dx.doi.org/10.54302/mausam.v25i3.5264.

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Lunar and solar atmospheric tides in surface winds and rainfall data at 4 stations have been determined following Chapman-Miller method as detailed by Malin and Chapman. Using the similar results obtained by Rao and Reddy (1972) for other stations a synthesis of the lunar and solar tides in surface winds and rainfall data for Indian stations have been made.

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45

Griffith, Matthew J., Shaun M. Dempsey, David R. Jackson, Tracy Moffat-Griffin, and Nicholas J. Mitchell. "Winds and tides of the Extended Unified Model in the mesosphere and lower thermosphere validated with meteor radar observations." Annales Geophysicae 39, no. 3 (2021): 487–514. http://dx.doi.org/10.5194/angeo-39-487-2021.

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Abstract. The mesosphere and lower thermosphere (MLT) is a critical region that must be accurately reproduced in general circulation models (GCMs) that aim to include the coupling between the lower and middle atmosphere and the thermosphere. An accurate representation of the MLT is thus important for improved climate modelling and the development of a whole atmosphere model. This is because the atmospheric waves at these heights are particularly large, and so the energy and momentum they carry is an important driver of climatological phenomena through the whole atmosphere, affecting terrestria

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46

Volland, Hans. "Comments on "Atmosphereic Tides" by A.Palumbo." Journal of Atmospheric and Solar-Terrestrial Physics 60, no. 18 (1998): 1791–92. http://dx.doi.org/10.1016/s1364-6826(98)00147-3.

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47

Wilson, Ian R. G., and Nikolay S. Sidorenkov. "Long-Term Lunar Atmospheric Tides in the Southern Hemisphere." Open Atmospheric Science Journal 7, no. 1 (2013): 51–76. http://dx.doi.org/10.2174/1874282320130415001.

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The longitudinal shift-and-add method is used to show that there are N=4 standing wave-like patterns in the summer (DJF) mean sea level pressure (MSLP) and sea-surface temperature (SST) anomaly maps of the Southern Hemisphere between 1947 and 1994. The patterns in the MSLP anomaly maps circumnavigate the Earth in 36, 18, and 9 years. This indicates that they are associated with the long-term lunar atmospheric tides that are either being driven by the 18.0 year Saros cycle or the 18.6 year lunar Draconic cycle. In contrast, the N=4 standing wave-like patterns in the SST anomaly maps circumnavig

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48

RAO, K. N., and S. JEEVANANDA REDDY. "Solar and lunar atmospheric tides in rainfall at Poona." MAUSAM 23, no. 4 (2022): 535–36. http://dx.doi.org/10.54302/mausam.v23i4.5315.

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The atmospheric tides in 'the rainfall data of the monsoon season, ...e., June to September at Poona (18° 32' N; 73° 51'E), have been studied by using hourly mean values and bi-hourly mean values for the period 1949-1960. Both solar and lunar effects upto the 4th harmonic have been discussed. Study of the variation with lunar phase of the rainfall indicates a maximum fall near the phase 3 while there is no other regular variation with lunar phase.

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49

Schulz, William H., Jason W. Kean, and Gonghui Wang. "Landslide movement in southwest Colorado triggered by atmospheric tides." Nature Geoscience 2, no. 12 (2009): 863–66. http://dx.doi.org/10.1038/ngeo659.

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50

Sherwood, Steven C. "Climate signal mapping and an application to atmospheric tides." Geophysical Research Letters 27, no. 21 (2000): 3525–28. http://dx.doi.org/10.1029/2000gl011424.

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