Study: Simulation of planetary atmospheres
, 2020 This thesis analyzes different ways of simulating planetary atmospheres to reproduce the observed phenomena and further understand its dynamics. To do so, a two dimensional Shallow Water model in ellipsoidal coordinates will be used in order to start capturing part of the dynamics that occur at large scales in the atmospheres of gas giant planets. Then,
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Multi-wavelength global maps of Jupiter and Saturn using Cassini imaging system data. [PDF]
Sci DataWang X, Li L, Jiang X, West RA.
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Radiation Driven Atmospheres of O-type stars: Constraints on the Mass–Luminosity Relation of Central Stars of Planetary Nebulae [PDF]
, 2003 A. W. A. Pauldrach +2 more
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Ripples formed in low-pressure wind tunnels suggest Mars's large windblown ripples are not impact ripples. [PDF]
Nat CommunAlvarez CA +3 more
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Planetary transport processes in the upper atmosphere. Annual progress report
, 1974 Reginald E. Newell
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Evolution of the Solar Magnetic Activity over Time and Effects on Planetary Atmospheres [PDF]
, 2004 E. F. Guinan, I. Ribas
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The erosion of large primary atmospheres typically leaves behind substantial secondary atmospheres on temperate rocky planets. [PDF]
Nat CommunKrissansen-Totton J +3 more
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Transonic Hydrodynamic Escape of Hydrogen from Extrasolar Planetary Atmospheres [PDF]
, 2005 Feng Tian +3 more
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Perspectives on Mars Sample Return: A critical resource for planetary science and exploration. [PDF]
Proc Natl Acad Sci U S AMcSween HY, Hamilton VE, Farley KA.
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Contributions of a multimoment multispecies approach in modeling planetary atmospheres: Example of Mars [PDF]
, 2005 V. Boqueho, Pierre‐Louis Blelly
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