Physics
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsh51c1221s&link_type=abstract
American Geophysical Union, Fall Meeting 2005, abstract #SH51C-1221
Physics
7513 Coronal Mass Ejections (2101), 7514 Energetic Particles (2114), 7526 Magnetic Reconnection (2723, 7835), 7594 Instruments And Techniques, 7924 Forecasting (2722)
Scientific paper
The S3C Great Observatory concept is guided by a systems approach to understanding the heliosphere. A Solar Energetic Particle Mission (SEPM) can make valuable contributions to this Great Observatory in conjunction with upcoming Living with a Star (LWS) missions e.g. Solar Dynamics Observatory and Sentinels. SEPM can provide the remote sensing component to a program for better understanding how, when, and where solar energetic particles (SEPs) are produced. Such a coordinated approach will include coronagraphic UV spectroscopy and visible light polarimetery with SEPM, along with in situ particles and fields, X-ray and gamma-ray measurements from spacecraft close to the Sun (Inner Heliospheric Sentinels). While SEPM will use plasma diagnostics that are derived from the UVCS and LASCO coronagaraphs on SOHO, it will have an order of magnitude improvement in its capabilities.
Cranmer Steven R.
Esser Ruth
Gardner Larry D.
Kohl John L.
Lin Juhn-Jong
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