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Interaction with Atmosphere
Contrary to longer-pulsed laser irradiation, ultrashort laser pulses in the femto- and low picosecond-pulse duration domains are expected to be too...
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Upper Atmosphere of Mars
Mars’ atmosphere above 100 km is designated as the upper atmosphere where molecular diffusion dominates (McElroy et al., Science 194:1295–1298,...
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Lower Atmosphere of Mars
The lower atmosphere of Mars exists below 100 km, where gases are mixed and eddy diffusion is dominant. It is characterized by a strong coupling...
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Experimental sensing quantum atmosphere of a single spin
Understanding symmetry-breaking states of materials is a major challenge in the modern physical sciences. Quantum atmosphere proposed recently sheds...
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Trace Gases of Mars Atmosphere
The atmosphere of Mars is primarily composed of CO2 (~ 95%) with small amounts of N2 (~ 2.6%), Ar (~ 1.9%, O2 (0.16%) and CO (~ 0.06%). The O3, H2O,...
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A New Source of Sulfates in the Atmosphere
AbstractMonitoring data on sulfates in atmospheric haze particles over Bei**g in winter 2016 are considered. It is found that the source of sulfates...
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Aeronomy Missions: Exploration to Mars Atmosphere
Mars’ upper atmosphere has been observed by Mariners 6, 7, 9; Mars 2, 3, 4, 5; Viking 1 and 2, MGS, MEX, MAVEN, Mangalyaan, EMM, and ExoMars but...
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The Plumes and Atmosphere of Io
The current state of knowledge of Io’s atmosphere and plumes is summarized, with an emphasis on research conducted since the Galileo era. While the...
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Possible Effects of Volcanic Eruptions on the Modern Atmosphere of Venus
This work reviews possible signatures and potential detectability of present-day volcanically emitted material in the atmosphere of Venus. We first...
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Thermal Conductivity of Multilayer Insulation in the Martian Atmosphere
AbstractThe experimental results of measurements of the thermal conductivity of standard multilayer insulation (MLI) in vacuum and under conditions...
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Develo** the Models of Acoustic-Gravity Waves in the Upper Atmosphere (Review)
AbstractThe results of the authors’ studies of acoustic-gravity waves (AGW) in the upper Earth’s atmosphere for recent years are presented. The work...
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Reflectionless Acoustic Waves in an Inhomogeneous Atmosphere
We study the vertical propagation of acoustic waves in a strongly inhomogeneous atmosphere. The class of monotonically varying profiles for the sound...
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Impact Structures on Venus as a Result of Asteroid Destruction in the Atmosphere
Abstract —Venus’ thick atmosphere is capable of destroying kilometer-sized bodies such as asteroids, creating various types of traces on the surface....
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Photochemical depletion of heavy CO isotopes in the Martian atmosphere
The atmosphere of Mars is enriched in heavy isotopes with respect to Earth as a result of the escape of the atmosphere to space over billions of...
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8 Water Cycle in the Atmosphere and Shallow Subsurface
The global water cycle on Earth constitutes one of the most relevant components of the terrestrial ecosystem. While the vast majority of terrestrial...