SH024
Space weather events at solar system bodies and beyond
Session ID#: 82766
Session Description:
The characteristics of how different solar system bodies respond to the active solar conditions can be used as an analog for space weather conditions experienced by planets at other stellar systems. The availability of both interplanetary spacecraft observations and advanced modeling techniques allow us to better understand the space weather responses by planets and their satellites within our solar system. In particular, the heliospheric influences on various bodies can be different, depending on the plasma environment of the planet (e.g., airless or tenuous atmosphere, with or without a magnetosphere).
This session will cover a range of interrelated topics, including the propagation and evolution of ICMEs and SEPs in the heliosphere, the space weather responses by planets, moons, and asteroids, and the expected space weather conditions at exoplanets, particularly those within habitable zones of their stellar systems. We welcome both observational and modeling studies on the heliosphere and exoplanetary systems.
Index Terms:
2101 Coronal mass ejections [INTERPLANETARY PHYSICS]
2114 Energetic particles [INTERPLANETARY PHYSICS]
2784 Solar wind/magnetosphere interactions [MAGNETOSPHERIC PHYSICS]
6296 Extra-solar planets [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
Primary Convener: Reka Moldovan Winslow, University of British Columbia, Vancouver, BC, Canada
Conveners: Reka Moldovan Winslow, University of New Hampshire, Durham, NH, United States, Jingnan Guo, University of Science and Technology of China, Hefei, China and Christina O Lee, Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States
Primary Liaison: Reka Moldovan Winslow, University of New Hampshire, Durham, NH, United States
Comparing the Properties of ICME-Induced Forbush Decreases at Earth and Mars (488424)
Johan Lauritz Freiherr von Forstner1, Jingnan Guo1,2, Robert F Wimmer-Schweingruber3, Mateja Dumbovic4, Miho Janvier5, Pascal Demoulin6, Astrid Veronig7, Manuela Temmer7, Don Hassler8 and Cary Zeitlin9, (1)University of Kiel, Institute of Experimental and Applied Physics, Kiel, Germany, (2)University of Science and Technology of China, School of Earth and Space Sciences, Hefei, China, (3)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (4)University of Zagreb, Hvar Observatory, Faculty of Geodesy, Zagreb, Croatia, (5)Institut d'Astrophysique Spatiale, Orsay, France, (6)LESIA, Observatoire de Paris, Meudon, France, (7)University of Graz, Institute of Physics, Graz, Austria, (8)Southwest Research Institute, Boulder, CO, United States, (9)Leidos Innovations Corporation, Houston, TX, United States
Revealing the pivot energy of Solar Energetic Particles Affecting the Martian surface radiation environment (529040)
Jingnan Guo, University of Science and Technology of China, School of Earth and Space Sciences, Hefei, China, Robert F Wimmer-Schweingruber, University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, Yuming Wang, University of Science and Technology of China, Hefei, China, Manuel Grande, Univ Wales Aberystwyth, Ceredigion, United Kingdom, Daniel Matthiae, DLR, Cologne, Germany, Cary Zeitlin, Southwest Research Institute Boulder, Boulder, CO, United States; Leidos Innovations Corporation, Houston, TX, United States, Bent Ehresmann, Southwest Research Institute, Oakland, CA, United States and Don Hassler, Southwest Research Inst, Boulder, CO, United States
Energetic particles measurements on the lunar far side by Lunar Lander Neutron and Dosimetry(LND) experiment (540759)
Zigong Xu1, Robert F Wimmer-Schweingruber2, Jingnan Guo3,4, Jia Yu3, Shenyi Zhang5, Thomas Berger6, Daniel Matthiae7, Soenke Burmeister8, Stephan I Boettcher2 and Bernd Heber3, (1)University of Kiel, Institute of Experimental and Applied Physics, Kiel, Germany, (2)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (3)University of Kiel, Kiel, Germany, (4)USTC University of Science and Technology of China, Hefei, China, (5)NSSC National Space Science Center, CAS, Beijing, China, (6)German Aerospace Center DLR Cologne, Institute for Flight Medicine, Cologne, Germany, (7)DLR, Cologne, Germany, (8)Christian-Albrechts-Universität zu Kiel, Institute for Experimental and Applied Physics, Kiel, Germany
Magnetic Impact of Propagating Interplanetary Coronal Mass Ejections in the Solar and Stellar Habitability Zones (570297)
Manolis K Georgoulis, Academy of Athens, Athens, Greece; Georgia State University, Department of Physics and Astronomy, Atlanta, United States, Spiros Patsourakos, University of Ioannina, Department of Physics, Ioannina, Greece and Evangelia Samara, Observatoire Royal de Belgique, Brussel, Belgium; KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium
