First detection of >100 MeV gamma-rays associated with a behind-the-limb solar flare
Abstract
Here, we report the first detection of >100 MeV gamma-rays associated with a behind-the-limb solar flare, which presents a unique opportunity to probe the underlying physics of high-energy flare emission and particle acceleration. On 2013 October 11 a GOES M1.5 class solar flare occurred ~9°.9 behind the solar limb as observed by STEREO-B. RHESSI observed hard X-ray (HXR) emission above the limb, most likely from the flare loop-top, as the footpoints were occulted. Surprisingly, the Fermi Large Area Telescope (LAT) detected >100 MeV gamma-rays for ~30 minutes with energies up to 3 GeV. The LAT emission centroid is consistent with the RHESSI HXR source, but its uncertainty does not constrain the source to be located there. The gamma-ray spectra can be adequately described by bremsstrahlung radiation from relativistic electrons having a relatively hard power-law (PL) spectrum with a high-energy exponential cutoff, or by the decay of pions produced by accelerated protons and ions with an isotropic pitch-angle distribution and a PL spectrum with a number index of ~3.8. Furthermore, we show that high optical depths rule out the gamma-rays originating from the flare site and a high-corona trap model requires very unusual conditions, so a scenario in which some ofmore »
- Authors:
-
- Istituto Nazionale di Fisica Nucleare, Pisa (Italy); Stanford Univ., Stanford, CA (United States). SLAC National Accelerator Lab.
- Stanford Univ., Stanford, CA (United States). SLAC National Accelerator Lab.
- Publication Date:
- Research Org.:
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1355159
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal. Letters (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal. Letters (Online); Journal Volume: 805; Journal Issue: 2; Journal ID: ISSN 2041-8213
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Sun: flares; Sun: X-rays; gamma rays
Citation Formats
Pesce-Rollins, Melissa, Omodei, Nicola, Petrosian, V., Liu, Wei, Costa, Fatima Rubio da, Allafort, A., and Chen, Qingrong. First detection of >100 MeV gamma-rays associated with a behind-the-limb solar flare. United States: N. p., 2015.
Web. doi:10.1088/2041-8205/805/2/L15.
Pesce-Rollins, Melissa, Omodei, Nicola, Petrosian, V., Liu, Wei, Costa, Fatima Rubio da, Allafort, A., & Chen, Qingrong. First detection of >100 MeV gamma-rays associated with a behind-the-limb solar flare. United States. https://doi.org/10.1088/2041-8205/805/2/L15
Pesce-Rollins, Melissa, Omodei, Nicola, Petrosian, V., Liu, Wei, Costa, Fatima Rubio da, Allafort, A., and Chen, Qingrong. Thu .
"First detection of >100 MeV gamma-rays associated with a behind-the-limb solar flare". United States. https://doi.org/10.1088/2041-8205/805/2/L15. https://www.osti.gov/servlets/purl/1355159.
@article{osti_1355159,
title = {First detection of >100 MeV gamma-rays associated with a behind-the-limb solar flare},
author = {Pesce-Rollins, Melissa and Omodei, Nicola and Petrosian, V. and Liu, Wei and Costa, Fatima Rubio da and Allafort, A. and Chen, Qingrong},
abstractNote = {Here, we report the first detection of >100 MeV gamma-rays associated with a behind-the-limb solar flare, which presents a unique opportunity to probe the underlying physics of high-energy flare emission and particle acceleration. On 2013 October 11 a GOES M1.5 class solar flare occurred ~9°.9 behind the solar limb as observed by STEREO-B. RHESSI observed hard X-ray (HXR) emission above the limb, most likely from the flare loop-top, as the footpoints were occulted. Surprisingly, the Fermi Large Area Telescope (LAT) detected >100 MeV gamma-rays for ~30 minutes with energies up to 3 GeV. The LAT emission centroid is consistent with the RHESSI HXR source, but its uncertainty does not constrain the source to be located there. The gamma-ray spectra can be adequately described by bremsstrahlung radiation from relativistic electrons having a relatively hard power-law (PL) spectrum with a high-energy exponential cutoff, or by the decay of pions produced by accelerated protons and ions with an isotropic pitch-angle distribution and a PL spectrum with a number index of ~3.8. Furthermore, we show that high optical depths rule out the gamma-rays originating from the flare site and a high-corona trap model requires very unusual conditions, so a scenario in which some of the particles accelerated by the CME shock travel to the visible side of the Sun to produce the observed gamma-rays may be at work.},
doi = {10.1088/2041-8205/805/2/L15},
journal = {The Astrophysical Journal. Letters (Online)},
number = 2,
volume = 805,
place = {United States},
year = {Thu May 28 00:00:00 EDT 2015},
month = {Thu May 28 00:00:00 EDT 2015}
}
Web of Science
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