Results 141 to 150 of about 6,063 (251)
Escape of hydrogen from the exosphere of Mars [PDF]
After decades of exploration, the martian neutral hydrogen exosphere has remained poorly characterized. The first measurements of this layer by Mariner 6 and 7 revealed it to be optically thick in Lyman α emission, along with a characteristic temperature
Bhattacharyya, Dolon
core
Lyα Emissions from Titan’s Atmosphere and Exosphere
From 2004 to 2017, the Cassini/UVIS instrument observed Titan’s Ly α airglow from Titan’s atmosphere and exosphere, helping to characterize Titan’s H population. Most Ly α observations remain unanalyzed. Using data from the T10 Titan flyby, we analyze Ly
Devin Hoover +5 more
doaj +1 more source
MESSENGER Observations of Planetary Ion Enhancements at Mercury's Northern Magnetospheric Cusp During Flux Transfer Event Showers. [PDF]
Sun W +13 more
europepmc +1 more source
Atmospheric escape’s potential to shape the exoplanet population motivates detailed observations of systems actively undergoing escape. AU Mic is a young and active M dwarf hosting two close-in transiting sub- to Neptune-sized planets. Atmospheric escape
Keighley E. Rockcliffe +10 more
doaj +1 more source
Soft X-ray and ENA Imaging of the Earth's Dayside Magnetosphere. [PDF]
Connor HK +18 more
europepmc +1 more source
Aerospace Environmental Challenges for Electrical Insulation and Recent Developments for Electrified Aircraft. [PDF]
Lizcano M +4 more
europepmc +1 more source
Mercury at the Dawn of a New Exploration Phase. [PDF]
Del Vecchio E +2 more
europepmc +1 more source
Energetic electron irradiations of amorphous and crystalline sulphur-bearing astrochemical ices. [PDF]
Mifsud DV +12 more
europepmc +1 more source
Exospheric Temperature of Venus
The local time dependence of the Cytherean exospheric temperature in the instantaneous heating rate model is calculated by solving the heat conduction equation. It is found that the differential heating by the solar ultraviolet radiation produces steep temperature gradients near terminator, mainly due to the low exospheric temperatures at the night ...
openaire
SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo. [PDF]
Orsini S +120 more
europepmc +1 more source

