Observations and modeling of Martian auroras
Observations of planetary auroras form a new area of planetary exploration from space,
especially for nonmagnetic planets since various kinds of auroras like Discrete, Proton and …
especially for nonmagnetic planets since various kinds of auroras like Discrete, Proton and …
The impact of energetic particles on the Martian ionosphere during a full solar cycle of radar observations: Radar blackouts
We present the first long‐term characterization of ionization layers in the lower ionosphere of
Mars (below∼ 90 km), a region inaccessible to orbital in‐situ observations, based on an …
Mars (below∼ 90 km), a region inaccessible to orbital in‐situ observations, based on an …
Annual variations in the Martian bow shock location as observed by the Mars Express mission
The Martian bow shock distance has previously been shown to be anticorrelated with solar
wind dynamic pressure but correlated with solar extreme ultraviolet (EUV) irradiance. Since …
wind dynamic pressure but correlated with solar extreme ultraviolet (EUV) irradiance. Since …
Sources of ionospheric variability at Mars
M Mendillo, C Narvaez, MF Vogt… - Journal of …, 2017 - Wiley Online Library
Abstract During the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission's deep‐dip#
2 campaign of 17–22 April 2015, spacecraft instruments observed all of the physical …
2 campaign of 17–22 April 2015, spacecraft instruments observed all of the physical …
Mars' plasma system. Scientific potential of coordinated multipoint missions:“The next generation”
The objective of this White Paper, submitted to ESA's Voyage 2050 call, is to get a more
holistic knowledge of the dynamics of the Martian plasma system, from its surface up to the …
holistic knowledge of the dynamics of the Martian plasma system, from its surface up to the …
Solar cycle variations in the ionosphere of Mars as seen by multiple Mars Express data sets
The response of the Martian ionosphere to solar activity is analyzed by taking into account
variations in a range of parameters during four phases of the solar cycle throughout 2005 …
variations in a range of parameters during four phases of the solar cycle throughout 2005 …
Origin of the extended Mars radar blackout of September 2017
Abstract The Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS)
onboard Mars Express, which operates between 0.1 and 5.5 MHz, suffered from a complete …
onboard Mars Express, which operates between 0.1 and 5.5 MHz, suffered from a complete …
The influence of crustal magnetic fields on the Martian bow shock location: A statistical analysis of MAVEN and Mars Express observations
Previous missions underlined the complex influence of the crustal magnetic fields on the
Martian environment, including the plasma boundaries. Their influence on the bow shock is …
Martian environment, including the plasma boundaries. Their influence on the bow shock is …
Radar signal propagation through the ionosphere of Europa
We review the current state of knowledge of the Europan plasma environment, its effects on
radio wave propagation, and its impact on the performance and design of future radar …
radio wave propagation, and its impact on the performance and design of future radar …
Mars plasma system response to solar wind disturbances during solar minimum
This paper is a phenomenological description of the ionospheric plasma and induced
magnetospheric boundary (IMB) response to two different types of upstream solar wind …
magnetospheric boundary (IMB) response to two different types of upstream solar wind …