Characteristics of Long Duration Gamma-Ray Flares

23 Oct 2015, 09:30
45m
Queen Kapiolani Hotel

Queen Kapiolani Hotel

150 Kapahulu Avenue, Honolulu, HI 96815

Speaker

Dr Gerald Share (University of Maryland)

Description

Fermi LAT has observed >100 MeV emission from at least twenty-five events following impulsive flares with GOES X-ray classes from M1.5 to X5.4. The emission is consistent with pion-decay radiation produced by > 300 MeV protons. Almost all the events are associated with fast (>800 km/s) CMEs, SEPs, and impulsive hard X-ray emission >100 keV. We discuss the time profiles of the LAT events on minute- and hour-long scales and information derived from a four-year systematic study of 95 energetic solar events and their association with sustained >100 MeV emission. We also discuss spectroscopic studies of the impulsive flares and sustained-emission phases that provide information on the numbers of >500 MeV protons and their spectra at the Sun and compare these properties with those observed in SEPs. This work was supported by the NSF-SHINE and NASA-Fermi-GI programs.

Author

Dr Gerald Share (University of Maryland)

Co-authors

Dr Allan Tylka (none) Ms Anne K. Tolbert (Catholic University) Dr Brian Dennis (NASA-GSFC) Dr Richard Schwartz (Catholic University) Dr Ronald Murphy (Naval Research Lab) Dr Stephen White (Kirtland AFB)

Presentation materials