Friday @ 10:30 a.m.
Magnetic Connections to the Heliosphere
Leader: Kelly Korreck
In order to utilize the SDO data to the fullest, the solar data must be linked through modeling and observation to the heliosphere. Several models already exist and are readily available at the CCMC. The goals of this session:
- To identify complementary data sets that can be used with SDO- EVE, AIA, and HMI data (for example, ACE SWICS data, Stereo or Ground based radio observations)
- Identify the science topics that can reap the most benefit from the collaboration
- Source Regions of the solar wind
- CME initiation, liftoff and propagation
- Composition and Temperature of unprocessed solar wind
- To identify the current and/or future models (MHD, energetic particle transport etc) that will aid in this comparison
- To determine ways in which the CCMC can become involved with the larger effort
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