Mars Express investigations of the Martian ionosphere using ASPERA-3 and new MARSIS fixed frequency modes

The plasma package Analyzer of Space Plasma and Energetic Atoms (ASPERA-3) onboard Mars Express has observed ions and electrons accelerated by the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) radar when it operates in its active ionospheric sounding mode. To better study the processes involved, new operational modes for MARSIS have been developed. In the first, a fixed frequency mode, the transmitter does not sweep over a range of frequencies, as normal, but instead transmits pulses at a fixed frequency. This frequency has been chosen to be close to the fundamental frequency of the local ionosphere around the spacecraft, which in all cases is < 350 kHz. Also, an alternating mode has been introduced, where observations in the fixed frequency mode are interleaved with observations that sweep over frequencies in order to investigate how ions are accelerated. Here we describe the new operational modes and present the results of several tests performed in the years 2020, 2021, and 2023.

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Publication Details

Journal
Advances in Space Research
Published
2025-02-07
DOI
https://doi.org/10.1016/j.asr.2025.02.005
Citations
3
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
3.46

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article

Mars Express investigations of the Martian ionosphere using ASPERA-3 and new MARSIS fixed frequency modes

A. Cicchetti, Mats Holmström, Simon Joyce, Beatriz Sánchez‐Cano et al.
3 citations
Advances in Space Research
Planetary Science and Exploration
3.46
article

Mars Express investigations of the Martian ionosphere using ASPERA-3 and new MARSIS fixed frequency modes

A. Cicchetti, Mats Holmström, Simon Joyce, Beatriz Sánchez‐Cano, M. Lester, Sebastián Rojas Mata, S. Barabash, Andrii Voshchepynets, Myroslava Hlebena, R. Orosei
article en
3 citations

Abstract

The plasma package Analyzer of Space Plasma and Energetic Atoms (ASPERA-3) onboard Mars Express has observed ions and electrons accelerated by the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) radar when it operates in its active ionospheric sounding mode. To better study the processes involved, new operational modes for MARSIS have been developed. In the first, a fixed frequency mode, the transmitter does not sweep over a range of frequencies, as normal, but instead transmits pulses at a fixed frequency. This frequency has been chosen to be close to the fundamental frequency of the local ionosphere around the spacecraft, which in all cases is < 350 kHz. Also, an alternating mode has been introduced, where observations in the fixed frequency mode are interleaved with observations that sweep over frequencies in order to investigate how ions are accelerated. Here we describe the new operational modes and present the results of several tests performed in the years 2020, 2021, and 2023.

Advances in Space ResearchVol. 75(7)
Swedish Institute of Space Physics (SE), University of Leicester (GB), Institute for Space Astrophysics and Planetology (IT), Istituto di Radioastronomia di Bologna (IT), Uzhhorod National University (UA), KTH Royal Institute of Technology (SE), National Institute for Astrophysics (IT), Umeå University (SE)
Swedish National Space Agency, Science and Technology Facilities Council
Openalex Percentile: Top 9%
Planetary Science and Exploration
3.46
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