Understanding what processes govern atmospheric escape and the loss of planetary water is of paramount importance for understanding how life in the universe can exist. One mechanism thought to be important at all planets is an ambipolar electric field that helps ions overcome gravity. We report the discovery and first quantitative extraterrestrial measurements of such a field at the planet Venus. Unexpectedly, despite comparable gravity, we show the field to be five times stronger than in Earths similar ionosphere. Contrary to our understanding, Venus would still lose heavy ions (including oxygen and all water-group species) to space, even if there were no stripping by the solar wind. We therefore find that it is possible for planets to los...
Both particle and electromagnetic energy flow into the Earth’s high latitude ionosphere. This energy...
Strong ultraviolet radiation from the Sun ionizes the upper atmosphere of Venus, creating a dense i...
The solar-planetary interaction is unique for non-magnetic planets, since the solar wind interacts d...
International audienceUnderstanding what processes govern atmospheric escape and the loss of planeta...
As an Earth-like planet Venus probably had a primordial dipole field for several million years after...
The present‐day Venusian atmosphere is dry, yet, in its earlier history a significant amount of wate...
Magnetometer measurements on the Pioneer Venus Orbiter (PVO) have shown that Venus is a non-magnetic...
Venus, unlike Earth, is an extremely dry planet although both began with similar masses, distances f...
The purpose of this dissertation is to expand our understanding of oxygen ion escape to space from V...
International audienceIn order for the Parker Solar Probe (PSP) mission to study the solar corona, i...
The solar wind interacts with the non-magnetic planet Venus by processes within the mantle region, l...
International audienceThe present atmosphere of Venus contains almost no water, but recent measureme...
The present atmosphere of Venus contains almost no water, but recent measurements indicate that in i...
AbstractVenus is gradually losing some of its atmosphere in the form of ions through its induced mag...
Atmospheric escape from the upper atmosphere of Venus is mainly influenced by the loss of hydrogen a...
Both particle and electromagnetic energy flow into the Earth’s high latitude ionosphere. This energy...
Strong ultraviolet radiation from the Sun ionizes the upper atmosphere of Venus, creating a dense i...
The solar-planetary interaction is unique for non-magnetic planets, since the solar wind interacts d...
International audienceUnderstanding what processes govern atmospheric escape and the loss of planeta...
As an Earth-like planet Venus probably had a primordial dipole field for several million years after...
The present‐day Venusian atmosphere is dry, yet, in its earlier history a significant amount of wate...
Magnetometer measurements on the Pioneer Venus Orbiter (PVO) have shown that Venus is a non-magnetic...
Venus, unlike Earth, is an extremely dry planet although both began with similar masses, distances f...
The purpose of this dissertation is to expand our understanding of oxygen ion escape to space from V...
International audienceIn order for the Parker Solar Probe (PSP) mission to study the solar corona, i...
The solar wind interacts with the non-magnetic planet Venus by processes within the mantle region, l...
International audienceThe present atmosphere of Venus contains almost no water, but recent measureme...
The present atmosphere of Venus contains almost no water, but recent measurements indicate that in i...
AbstractVenus is gradually losing some of its atmosphere in the form of ions through its induced mag...
Atmospheric escape from the upper atmosphere of Venus is mainly influenced by the loss of hydrogen a...
Both particle and electromagnetic energy flow into the Earth’s high latitude ionosphere. This energy...
Strong ultraviolet radiation from the Sun ionizes the upper atmosphere of Venus, creating a dense i...
The solar-planetary interaction is unique for non-magnetic planets, since the solar wind interacts d...