Speaker
Melissa Pesce-Rollins
(INFN-Pisa)
Description
Fermi LAT >30 MeV observations of the active Sun have increased the number of detected solar flares by almost a factor of 10 with respect to previous space observations. These sample both the impulsive and long duration phases of GOES M and X class flares. Of particular interest are the recent detections of two solar flares whose position behind the limb was confirmed by the STEREO-B satellite. While gamma-ray emission up to tens of MeV resulting from proton interactions has been detected before from occulted solar flares, the significance of these particular events lies in the fact that these are the first detections of >100 MeV gamma-ray emission from footpoint-occulted flares. We will present the Fermi-LAT, RHESSI and STEREO observations of these flares and discuss the various emission scenarios for these sources.
| Registration number following "ICRC2015-I/" | 1141 |
|---|---|
| Collaboration | FERMI |
Primary author
Melissa Pesce-Rollins
(INFN-Pisa)
Co-authors
Dr
Fatima Rubio da Costa
(Stanford)
Dr
Liiu Wei
(Stanford)
Dr
Nicola Omodei
(Stanford)
Prof.
Vahe Petrosian
(Stanford)
