Results 91 to 100 of about 1,980 (216)
Seasonal Effects of the Changing Photon Scattering Rates on Mercury’s Exospheric Structure
Emission in Mercury’s exosphere observed from the ground and by spacecraft is produced by resonant scattering of sunlight. The process of resonant scattering changes the structure of the exosphere owing to the transfer of momentum between the incident ...
Matthew H. Burger +5 more
doaj +1 more source
Search for spectroscopical signatures of transiting HD 209458b's exosphere
Following recent attempts to detect the exosphere of the extra-solar planet 51 Pegb in the infrared (Coustenis et al. [CITE], [CITE]; Rauer et al. [CITE]), we discuss here a search for optical spectroscopic signatures from a gaseous extended envelope (
A. Kaufer +6 more
core +1 more source
To better assess the role that electrons play in exosphere production on icy bodies, we measured the total and O _2 sputtering yields from H _2 O ice for electrons with energies between 0.75 and 10 keV and temperatures between 15 and 124.5 K.
Rebecca A. Carmack, Mark J. Loeffler
doaj +1 more source
Modeling Results on the Seasonal Influence at the Martian Exosphere
International audienceAnalysis of HST ACS/SBC images of Mars in the far-ultraviolet taken in Oct-Nov 2007 and May-November 2014 indicate seasonal influence as a driving factor of the hydrogen corona, as has been reported earlier. To derive the changes in
Mayyasi, Majd +4 more
core
Surface Response of Mercury’s Sulfides under Solar Wind Ion Irradiation
The MESSENGER mission revealed unexpectedly high sulfur content within Mercury’s surface, deviating from the lunar regolith, which was until recently considered a good Mercury analog.
Noah Jäggi, Catherine A. Dukes
doaj +1 more source
Observations of Mercury's Exosphere: Composition and Structure
Mercury is surrounded by a tenuous exosphere in which particles travel on ballistic trajectories under the influence of a combination of gravity and solar radiation pressure.
Cassidy, Timothy A. +5 more
core
Mercury is surrounded by a tenuous neutral exosphere composed primarily of sodium atoms, which can be continuously ionized. The production of sodium ions is concentrated on the dayside, and these ions can subsequently be transported to the magnetotail ...
Yuxi Chen, Chuanfei Dong, Weijie Sun
doaj +1 more source
Highly charged ions in the solar wind undergo charge exchange with neutral atoms in the Earth’s exosphere, particularly within the magnetosheath and cusps.
Jaewoong Jung +5 more
doaj +1 more source
A New Mechanism for Early-Time Plasmaspheric Refilling: The Role of Charge Exchange Reactions in the Transport of Energy and Mass Throughout the Ring Current-Plasmasphere System. [PDF]
Liu J, Ilie R, Borovsky JE, Liemohn MW.
europepmc +1 more source
Thermally Driven Atmospheric Escape: Transition from Diffusion-limited to Drag-off Escape
We examine the transition from diffusion-limited to drag-off escape using a direct simulation Monte Carlo (DSMC) model developed to simulate planetary atmospheres, referred to as Harrah.
Jack C. Evans +3 more
doaj +1 more source

