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Mars Express investigations of the Martian ionosphere using ASPERA-3 and new MARSIS fixed frequency modes
Umeå University, Faculty of Science and Technology, Department of Physics. Swedish Institute of Space Physics, Kiruna, Sweden.ORCID iD: 0000-0001-5494-5374
Uzhhorod National University, Uzhhorod, Ukraine.
Umeå University, Faculty of Science and Technology, Department of Physics. Swedish Institute of Space Physics, Kiruna, Sweden.
Swedish Institute of Space Physics, Kiruna, Sweden; Royal Institute of Technology, Stockholm, Sweden.
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2025 (English)In: Advances in Space Research, ISSN 0273-1177, E-ISSN 1879-1948, Vol. 75, no 7, p. 5899-5910Article in journal (Refereed) Published
Abstract [en]

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.

Place, publisher, year, edition, pages
Elsevier, 2025. Vol. 75, no 7, p. 5899-5910
Keywords [en]
Active Experiment, Instrumentation, Ionosphere, Mars, Planetary Physics, Plasma Physics
National Category
Fusion, Plasma and Space Physics
Identifiers
URN: urn:nbn:se:umu:diva-235858DOI: 10.1016/j.asr.2025.02.005ISI: 001451552700001Scopus ID: 2-s2.0-85217931044OAI: oai:DiVA.org:umu-235858DiVA, id: diva2:1939818
Funder
Swedish National Space Board, 2022-00104Available from: 2025-02-24 Created: 2025-02-24 Last updated: 2025-04-15Bibliographically approved

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Holmström, MatsBarabash, Stas

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