The induced magnetospheres of Mars, Venus, and Titan
This article summarizes and aims at comparing the main features of the induced
magnetospheres of Mars, Venus and Titan. All three objects form a well-defined induced …
magnetospheres of Mars, Venus and Titan. All three objects form a well-defined induced …
Structure, dynamics, and seasonal variability of the Mars‐solar wind interaction: MAVEN Solar Wind Ion Analyzer in‐flight performance and science results
We report on the in‐flight performance of the Solar Wind Ion Analyzer (SWIA) and
observations of the Mars‐solar wind interaction made during the Mars Atmosphere and …
observations of the Mars‐solar wind interaction made during the Mars Atmosphere and …
Space plasma physics: A review
BT Tsurutani, GP Zank, VJ Sterken… - … on Plasma Science, 2022 - ieeexplore.ieee.org
Owing to the ever-present solar wind, our vast solar system is full of plasmas. The turbulent
solar wind, together with sporadic solar eruptions, introduces various space plasma …
solar wind, together with sporadic solar eruptions, introduces various space plasma …
Martian shock and magnetic pile-up boundary positions and shapes determined from the Phobos 2 and Mars Global Surveyor data sets
JG Trotignon, C Mazelle, C Bertucci… - Planetary and Space …, 2006 - Elsevier
A great many Martian bow shock and magnetic pile-up boundary crossings have been
identified in the Phobos 2 and Mars Global Surveyor, MGS, data. From these observations …
identified in the Phobos 2 and Mars Global Surveyor, MGS, data. From these observations …
The Magnetometer instrument on MESSENGER
BJ Anderson, MH Acuña, DA Lohr, J Scheifele… - … MESSENGER mission to …, 2007 - Springer
The Magnetometer (MAG) on the MErcury Surface, Space ENvironment, GEochemistry, and
Ranging (MESSENGER) mission is a low-noise, tri-axial, fluxgate instrument with its sensor …
Ranging (MESSENGER) mission is a low-noise, tri-axial, fluxgate instrument with its sensor …
Ion energization and escape on Mars and Venus
Mars and Venus do not have a global magnetic field and as a result solar wind interacts
directly with their ionospheres and upper atmospheres. Neutral atoms ionized by solar UV …
directly with their ionospheres and upper atmospheres. Neutral atoms ionized by solar UV …
First results of the MAVEN magnetic field investigation
JEP Connerney, JR Espley… - Geophysical …, 2015 - Wiley Online Library
Abstract Two Mars Atmosphere and Volatile EvolutioN magnetic field sensors sample the
ambient magnetic field at the outer edge of each solar array. We characterized relatively …
ambient magnetic field at the outer edge of each solar array. We characterized relatively …
Flows, fields, and forces in the Mars‐solar wind interaction
We utilize suprathermal ion and magnetic field measurements from the Mars Atmosphere
and Volatile EvolutioN (MAVEN) mission, organized by the upstream magnetic field, to …
and Volatile EvolutioN (MAVEN) mission, organized by the upstream magnetic field, to …
A MAVEN case study of radial IMF at Mars: Impacts on the dayside ionosphere
The solar wind interaction with Mars controls the transfer of energy and momentum from the
solar wind into the magnetosphere, ionosphere and atmosphere, driving structure, and …
solar wind into the magnetosphere, ionosphere and atmosphere, driving structure, and …
Influence of the solar EUV flux on the Martian plasma environment
R Modolo, GM Chanteur, E Dubinin… - Annales …, 2005 - angeo.copernicus.org
The interaction of the solar wind with the Martian atmosphere and ionosphere is investigated
by using three-dimensional, global and multi-species hybrid simulations. In the present work …
by using three-dimensional, global and multi-species hybrid simulations. In the present work …