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Radio Absorption in the Nightside Ionosphere of Mars During Solar Energetic Particle Events
DOI: 10.1029/2023SW003755 Bibcode: 2023SpWea..2103755H

Lester, M.; Leblanc, F.; Sánchez-Cano, B. +3 more

Characterization, understanding, and prediction of the Martian radio environment are of increasing importance to the forthcoming human exploration of Mars. Here we investigate 3-5 MHz radio absorption in the nightside ionosphere of Mars caused by enhanced ionization at <100 km altitudes during solar energetic particle (SEP) events. We conduct a…

2023 Space Weather
MEx 5
Solar Energetic Particle Events Detected in the Housekeeping Data of the European Space Agency's Spacecraft Flotilla in the Solar System
DOI: 10.1029/2023SW003540 Bibcode: 2023SpWea..2103540S

Wimmer-Schweingruber, Robert F.; Wood, Simon; Wilson, Colin +37 more

Despite the growing importance of planetary Space Weather forecasting and radiation protection for science and robotic exploration and the need for accurate Space Weather monitoring and predictions, only a limited number of spacecraft have dedicated instrumentation for this purpose. However, every spacecraft (planetary or astronomical) has hundred…

2023 Space Weather
BepiColombo ExoMars-16 MEx SolarOrbiter VenusExpress 2
CMEs and SEPs During November-December 2020: A Challenge for Real-Time Space Weather Forecasting
DOI: 10.1029/2021SW002993 Bibcode: 2022SpWea..2002993P

Maksimovic, Milan; Möstl, Christian; Galvin, Antoinette B. +20 more

Predictions of coronal mass ejections (CMEs) and solar energetic particles (SEPs) are a central issue in space weather forecasting. In recent years, interest in space weather predictions has expanded to include impacts at other planets beyond Earth as well as spacecraft scattered throughout the heliosphere. In this sense, the scope of space weathe…

2022 Space Weather
MEx SOHO SolarOrbiter 29
CME Evolution in the Structured Heliosphere and Effects at Earth and Mars During Solar Minimum
DOI: 10.1029/2022SW003215 Bibcode: 2022SpWea..2003215P

Nitta, Nariaki V.; Holmström, Mats; Futaana, Yoshifumi +13 more

The activity of the Sun alternates between a solar minimum and a solar maximum, the former corresponding to a period of "quieter" status of the heliosphere. During solar minimum, it is in principle more straightforward to follow eruptive events and solar wind structures from their birth at the Sun throughout their interplanetary journey. In this p…

2022 Space Weather
MEx SOHO 25
CME Magnetic Structure and IMF Preconditioning Affecting SEP Transport
DOI: 10.1029/2020SW002654 Bibcode: 2021SpWea..1902654P

Lowrance, Patrick J.; Möstl, Christian; Guo, Jingnan +15 more

Coronal mass ejections (CMEs) and solar energetic particles (SEPs) are two phenomena that can cause severe space weather effects throughout the heliosphere. The evolution of CMEs, especially in terms of their magnetic structure, and the configuration of the interplanetary magnetic field (IMF) that influences the transport of SEPs are currently are…

2021 Space Weather
MEx SOHO 33
Modeling the Evolution and Propagation of 10 September 2017 CMEs and SEPs Arriving at Mars Constrained by Remote Sensing and In Situ Measurement
DOI: 10.1029/2018SW001973 Bibcode: 2018SpWea..16.1156G

Dumbović, Mateja; Temmer, Manuela; Veronig, Astrid +13 more

On 10 September 2017, solar energetic particles originating from the active region 12673 produced a ground level enhancement at Earth. The ground level enhancement on the surface of Mars, 160 longitudinally east of Earth, observed by the Radiation Assessment Detector (RAD) was the largest since the landing of the Curiosity rover in August 2012. Ba…

2018 Space Weather
MEx SOHO 70