Add to ORKGIonization of thermal and non-thermal oxygen atoms above the plasmapause on Venus supplies an escape flux for O averaging 6 × 106atoms cm ²sec−1. Hydrogen and oxygen atoms escape with stoichiometry characteristic of water. It is argued that escape of H is controlled by the oxidation state of the atmosphere, regulated by escape of O
Venus is free of molecular oxygen but it is thought to have contained a primordial water ocean. Pres...
Decades of research have sought to understand the similarities and differences between Venus and Ea...
The present‐day Venusian atmosphere is dry, yet, in its earlier history a significant amount of wate...
Ionization of thermal and non-thermal oxygen atoms above the plasmapause on Venus supplies an escape...
Venus, unlike Earth, is an extremely dry planet although both began with similar masses, distances f...
Atmospheric escape from the upper atmosphere of Venus is mainly influenced by the loss of hydrogen a...
International audienceThe present atmosphere of Venus contains almost no water, but recent measureme...
International audienceA fundamental question for the atmospheric evolution of Venus is how much wate...
A fundamental question for the atmospheric evolution of Venus is how much water-related material esc...
The present atmosphere of Venus contains almost no water, but recent measurements indicate that in i...
International audienceA time dependent model of hydrogen hydrodynamic escape powered by solar EUV fl...
Recombination of O(2)(+) represents a source of fast oxygen atoms in Venus' exosphere, and subsequen...
As an Earth-like planet Venus probably had a primordial dipole field for several million years after...
Charge exchange between H and H+ and momentum transfer between fast O and H provide comparable sourc...
Venus is free of molecular oxygen but it is thought to have contained a primordial water ocean. Pres...
Decades of research have sought to understand the similarities and differences between Venus and Ea...
The present‐day Venusian atmosphere is dry, yet, in its earlier history a significant amount of wate...
Ionization of thermal and non-thermal oxygen atoms above the plasmapause on Venus supplies an escape...
Venus, unlike Earth, is an extremely dry planet although both began with similar masses, distances f...
Atmospheric escape from the upper atmosphere of Venus is mainly influenced by the loss of hydrogen a...
International audienceThe present atmosphere of Venus contains almost no water, but recent measureme...
International audienceA fundamental question for the atmospheric evolution of Venus is how much wate...
A fundamental question for the atmospheric evolution of Venus is how much water-related material esc...
The present atmosphere of Venus contains almost no water, but recent measurements indicate that in i...
International audienceA time dependent model of hydrogen hydrodynamic escape powered by solar EUV fl...
Recombination of O(2)(+) represents a source of fast oxygen atoms in Venus' exosphere, and subsequen...
As an Earth-like planet Venus probably had a primordial dipole field for several million years after...
Charge exchange between H and H+ and momentum transfer between fast O and H provide comparable sourc...
Venus is free of molecular oxygen but it is thought to have contained a primordial water ocean. Pres...
Decades of research have sought to understand the similarities and differences between Venus and Ea...
The present‐day Venusian atmosphere is dry, yet, in its earlier history a significant amount of wate...