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 …

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 …

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 …

Several models of the martian ionosphere have been developed in the last years. In this
paper, a new empirical model for the dayside electron density of the martian ionosphere …

We use electron density profiles measured by the Mars Advanced Radar for Subsurface and
Ionosphere Sounding instrument on board the Mars Express spacecraft to investigate the …

Spacecraft observations around Mars show that ionospheric irregularities occur frequently in
the Martian ionosphere. In this study, Mars Atmosphere and Volatile Evolution data (the …

This paper is a phenomenological description of the ionospheric plasma and induced
magnetospheric boundary (IMB) response to two different types of upstream solar wind …

Abstract The Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS)
onboard the European Space Agency's Mars Express (MEX) spacecraft routinely detects …

The total electron content (TEC) is one of the most useful parameters to evaluate the
behavior of the Martian ionosphere because it contains information on the total amount of …

Solar cycle variations in solar radiation create density changes in any planetary ionosphere,
which are well established in the Earth's case. At Mars, however, the ionospheric response …