The THEMIS fluxgate magnetometer
Abstract The THEMIS Fluxgate Magnetometer (FGM) measures the background magnetic
field and its low frequency fluctuations (up to 64 Hz) in the near-Earth space. The FGM is …
field and its low frequency fluctuations (up to 64 Hz) in the near-Earth space. The FGM is …
The BepiColombo planetary magnetometer MPO-MAG: what can we learn from the Hermean magnetic field?
D Heyner, HU Auster, KH Fornaçon, C Carr… - Space Science …, 2021 - Springer
The magnetometer instrument MPO-MAG on-board the Mercury Planetary Orbiter (MPO) of
the BepiColombo mission en-route to Mercury is introduced, with its instrument design, its …
the BepiColombo mission en-route to Mercury is introduced, with its instrument design, its …
Observation-based modelling of magnetised coronal mass ejections with EUHFORIA
C Scolini, L Rodriguez, M Mierla, J Pomoell… - Astronomy & …, 2019 - aanda.org
Context. Coronal mass ejections (CMEs) are the primary source of strong space weather
disturbances at Earth. Their geo-effectiveness is largely determined by their dynamic …
disturbances at Earth. Their geo-effectiveness is largely determined by their dynamic …
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 …
The analyser of space plasmas and energetic atoms (ASPERA-4) for the Venus Express mission
The general scientific objective of the ASPERA-4 (Analyser of Space Plasmas and Energetic
Atoms) experiment is to study the solar wind–atmosphere interaction and characterise the …
Atoms) experiment is to study the solar wind–atmosphere interaction and characterise the …
Radial Evolution of Coronal Mass Ejections Between MESSENGER, Venus Express, STEREO, and L1: Catalog and Analysis
Our knowledge of the properties of coronal mass ejections (CMEs) in the inner heliosphere
is constrained by the relative lack of plasma observations between the Sun and 1 AU. In this …
is constrained by the relative lack of plasma observations between the Sun and 1 AU. In this …
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 …
Generic magnetic field intensity profiles of interplanetary coronal mass ejections at Mercury, Venus, and Earth from superposed epoch analyses
M Janvier, RM Winslow, S Good… - Journal of …, 2019 - Wiley Online Library
We study interplanetary coronal mass ejections (ICMEs) measured by probes at different
heliocentric distances (0.3–1 AU) to investigate the propagation of ICMEs in the inner …
heliocentric distances (0.3–1 AU) to investigate the propagation of ICMEs in the inner …
Magnetic structure and propagation of two interacting CMEs from the Sun to Saturn
E Palmerio, T Nieves‐Chinchilla… - Journal of …, 2021 - Wiley Online Library
One of the grand challenges in heliophysics is the characterization of coronal mass ejection
(CME) magnetic structure and evolution from eruption at the Sun through heliospheric …
(CME) magnetic structure and evolution from eruption at the Sun through heliospheric …
The loss of ions from Venus through the plasma wake
Venus, unlike Earth, is an extremely dry planet although both began with similar masses,
distances from the Sun, and presumably water inventories. The high deuterium-to-hydrogen …
distances from the Sun, and presumably water inventories. The high deuterium-to-hydrogen …