SH014
Interior Dynamics to Surface Magnetism: Probing the Full Sun with Observations from the Sun-Earth Line Augmented with New Data from the Poles, the Far Side, and Other Vantage Points
Interior Dynamics to Surface Magnetism: Probing the Full Sun with Observations from the Sun-Earth Line Augmented with New Data from the Poles, the Far Side, and Other Vantage Points
Session ID#: 249007
Session Description:
Understanding the solar cycle and its variability requires full views of the Sun. Solar magnetic activity arises from interactions of flows and fields within the convection zone and across the surface. Full Sun observations allow us to more effectively probe both interior dynamics and surface magnetic phenomena. With long-term datasets from SDO/HMI, SOHO/MDI, and GONG, and new high latitude and far-side vantages provided by Solar Orbiter and STEREO, we are able to better investigate the global magnetic activity via advances in helioseismology, modeling, and data assimilation. These capabilities will be further expanded by the Vigil mission and the Solar Polar mission recommended by the Decadal Survey. This session welcomes studies that address the physical processes governing the solar activity cycle across all vantage points, from tachocline to the convection zone and through the surface. Contributions from the solar community, including the COFFIES DRIVE Science Center, are welcome.
Index Terms:
7522 Helioseismology [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7536 Solar activity cycle [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7544 Stellar interiors and dynamo theory [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
Primary Convener: Ruizhu Chen, Stanford University, Stanford, CA, United States
Convener: Lisa Upton, Southwest Research Institute Boulder, Boulder, CO, United States
See more of: SPA-Solar and Heliospheric Physics