Results 61 to 70 of about 6,063 (251)
Surface Exospheric Interactions
AbstractGas-surface interactions at the Moon, Mercury and other massive planetary bodies constitute, alongside production and escape, an essential element of the physics of their gravitationally bound exospheres. From condensation and accumulation of exospheric species onto the surface in response to diurnal and seasonal changes of surface temperature,
Teolis, Ben +11 more
openaire +2 more sources
Untangling the Origin of Molecular Hydrogen in the Lunar Exosphere
In situ experiments from the Apollo missions confirmed the presence of a tenuous exosphere on the Moon comprised of atoms and light molecular species. Of the most prominent volatiles found in the exosphere, molecular hydrogen (H2) has drawn considerable ...
P. B. Crandall +2 more
semanticscholar +1 more source
Analytical model of Europa's O2 exosphere [PDF]
The origin of the exosphere of Europa is its water ice surface. The existing exosphere models, assuming either a collisionless environment (simple Monte Carlo techniques) or a kinetic approach (Direct Monte Carlo Method) both predict that the major ...
MURA, Alessandro +7 more
core +1 more source
An ICME impact on the Martian hydrogen corona
The Martian hydrogen exosphere extends out of the bow shock, forming a "hydrogen corona". The solar wind interacts directly with the hydrogen corona. During an ICME event on 7 March 2015, the SWIA instrument onboard Mars Atmosphere and Volatile Evolution
Qi Xu +5 more
doaj +1 more source
Abstract In this study, multi‐source thermospheric observations and TIEGCM simulations were used to explore the latitudinal variations of thermospheric temperature and total mass density at equinoxes. At nighttime, temperature and density exhibit consistent latitudinal patterns, with higher values at high latitudes.
Zhongli Li +3 more
wiley +1 more source
Coronagraphic observations of the lunar sodium exosphere January–June, 2017
In order to observe the lunar sodium exosphere out to one-half degree around the Moon, we designed, built and installed a small robotically controlled coronagraph at the Winer Observatory in Sonoita, Arizona.
R. Killen +5 more
semanticscholar +1 more source
Observed variations of the exospheric hydrogen density with the exospheric temperature
Measurements of exospheric hydrogen densities at a distance of 3 RE (earth radii) are presented as a function of exospheric temperature. They imply that the density nc at the exobase level decreases with exospheric temperature Tc but not enough to keep the Jeans escape flux FJ constant.
openaire +2 more sources
Metallic Species in Mercury's Exosphere: EMMI/New Technology Telescope Observations [PDF]
International audienceWe performed high spectral resolution observations of Mercury's exosphere on 2005 October 30 and 31 using the European Southern Observatory-New Technology Telescope, La Silla, Chile.
Erard, S. +3 more
core +1 more source
Eine atomistische Deutung der Brunt-Vaisälä-Periode
In einer kurzen Notiz wird eine atomistische Deutung der Brunt-Väisälä-Periode diskutiert. Es wird gezeigt, daß an der unteren Grenze der Exosphäre, wo per definitionem die mittlere freie Weglänge und die Skalenhöhe von gleicher Größenordnung sind, die ...
A. Muschinski
doaj +1 more source
Martian Magnetotail Neutral Sheet Asymmetry Driven by Heavy Planetary Pickup Ions
Abstract In the induced magnetotail of Mars, the neutral sheet is an important channel for atmospheric ion escape, yet the role of heavy planetary pickup ions in shaping its geometry has been unclear. Using three‐dimensional hybrid simulations, we demonstrate that these ions induce a global neutral sheet asymmetry via mass loading.
Jingyi Zhou +6 more
wiley +1 more source

