SM019
NASA’s Heliophysics Research Program supported by the Heliophysics System Observatory

Session ID#: 157157

Session Description:
NASA’s Heliophysics Research Program encompasses studies of solar dynamics, the interplanetary space, the solar wind, and its interaction with the Earth’s magnetosphere-ionosphere-thermosphere (MIT) system. Given the large volume of the system, it is difficult to draw general conclusions by looking at localized regions in the heliosphere. Moreover, the use of multi-point observations from different parts of the system, such as observations performed by NASA’s Heliophysics System Observatory (HSO) missions, can be an effective way to alleviate these difficulties. We then invite papers covering data analyses from several different regions from the Sun’s interior to the MIT system, such as solar dynamics and atmosphere, solar wind perturbations and turbulence, radiation belts, magnetic field variability at geosynchronous orbit, satellite surface charging, ionosphere variability, thermosphere dynamics and drag effects in low-Earth orbit, ground magnetometer response, geomagnetically induced currents, and others. We encourage papers that use multiple observations from non-HSO missions/datasets as well.
Co-Organized:
  • SA - SPA-Aeronomy
  • SH - SPA-Solar and Heliospheric Physics
Index Terms:

7904 Geomagnetically induced currents [SPACE WEATHER]
7949 Ionospheric storms [SPACE WEATHER]
7954 Magnetic storms [SPACE WEATHER]
7969 Satellite drag [SPACE WEATHER]

Primary Convener:  Denny M. Oliveira, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Conveners:  Amy M Keesee, University of New Hampshire, Physics and Space Science Center, Durham, NH, United States, Sergio Vidal-Luengo, University of Michigan, Ann Arbor, MI, United States and James M Weygand, IGPP/UCLA---ESS, Los Angeles, CA, United States
Student/Early Career Convener:  Sergio Vidal-Luengo, University of Michigan, Ann Arbor, MI, United States
 
Field-Aligned Currents of Dipolarizing Flux Bundles and the Associated Plasma Disturbance: Understanding the Asymmetry of Wedgelets (Invited) (1050635)
Jiang Liu, University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, United States
 
Heliophysics With HERMES From Gateway in Lunar Orbit (1073429)
William R Paterson1, Daniel J Gershman2, Shrikanth G Kanekal3, Roberto Livi4, Mark B. Moldwin5, Eftyhia Zesta6, Brent Randol6 and Marilia Samara2, (1)NASA Goddard Space Flight Center, Geospace Physics Laboratory, Greenbelt, MD, United States, (2)NASA Goddard Space Flight Center, Greenbelt, United States, (3)NASA GSFC, Greenbelt, MD, United States, (4)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (5)University of Michigan Ann Arbor, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Investigating Energy Release during Solar Eruptive Events (Invited) (1087897)
Juliana Therese Vievering, Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Chunming Zhu, Montana State University, Physics, Bozeman, MT, United States, Jiong Qiu, Montana State University, Department of Physics, Bozeman, MT, United States, Laura Balmaceda, George Mason University, Fairfax, United States and Lindsay Glesener, University of Minnesota Twin Cities, Minneapolis, United States
 
The Machine learning Enabled Thermosphere Advanced by HASDM (META-HASDM) system (1193075)
W Kent Tobiska, Marcin Pilinski2, Shaylah Mutschler2, Kaiya Wahl2, Dave Bouwer2, Piyush Mehta2, Richard Licata3, Vishal Ray4 and Siamak Hesar5, (1)Space Environment Technologies, Pacific Palisades, United States, (2)West Virginia University, Morgantown, WV, United States, (3)Boulder, CO, United States, (4)Kayhan Space, Boulder, United States
See more of: SPA-Magnetospheric Physics
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