DOE PAGES title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: 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 » 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.« less

Authors:
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [2]; ORCiD logo [2]; ORCiD logo [2];  [2];  [2]
  1. Istituto Nazionale di Fisica Nucleare, Pisa (Italy); Stanford Univ., Stanford, CA (United States). SLAC National Accelerator Lab.
  2. 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}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record

Citation Metrics:
Cited by: 41 works
Citation information provided by
Web of Science

Save / Share:

Works referenced in this record:

FERMI DETECTION OF γ-RAY EMISSION FROM THE M2 SOFT X-RAY FLARE ON 2010 JUNE 12
journal, January 2012


THE FERMI LARGE AREA TELESCOPE ON ORBIT: EVENT CLASSIFICATION, INSTRUMENT RESPONSE FUNCTIONS, AND CALIBRATION
journal, October 2012

  • Ackermann, M.; Ajello, M.; Albert, A.
  • The Astrophysical Journal Supplement Series, Vol. 203, Issue 1
  • DOI: 10.1088/0067-0049/203/1/4

HIGH-ENERGY GAMMA-RAY EMISSION FROM SOLAR FLARES: SUMMARY OF FERMI LARGE AREA TELESCOPE DETECTIONS AND ANALYSIS OF TWO M-CLASS FLARES
journal, April 2014


Impulsive and long Duration High-Energy Gamma-Ray Emission from the very Bright 2012 March 7 Solar Flares
journal, June 2014


Electron Trapping Times and Trap Densities in Solar Flare Loops Measured with COMPTON and YOHKOH
journal, October 1997

  • Aschwanden, Markus J.; Bynum, Robert M.; Kosugi, Takeo
  • The Astrophysical Journal, Vol. 487, Issue 2
  • DOI: 10.1086/304633

THE LARGE AREA TELESCOPE ON THE FERMI GAMMA-RAY SPACE TELESCOPE MISSION
journal, May 2009


Evidence for intense coronal prompt gamma-ray line emission from a solar flare
journal, April 1994

  • Barat, C.; Trottet, G.; Vilmer, N.
  • The Astrophysical Journal, Vol. 425
  • DOI: 10.1086/187322

Background estimation in a wide-field background-limited instrument such as Fermi GBM
conference, September 2012

  • Fitzpatrick, Gerard; McBreen, Sheila; Connaughton, Valerie
  • SPIE Astronomical Telescopes + Instrumentation, SPIE Proceedings
  • DOI: 10.1117/12.928036

Impulsive Phase Flare Energy Transport by Large‐Scale Alfvén Waves and the Electron Acceleration Problem
journal, March 2008

  • Fletcher, L.; Hudson, H. S.
  • The Astrophysical Journal, Vol. 675, Issue 2
  • DOI: 10.1086/527044

Solar Auroras
journal, April 2012


Implications of X-ray Observations for Electron Acceleration and Propagation in Solar Flares
journal, August 2011


Origin and Location of the Hard X-Ray Emission in a Two-Ribbon Flare
journal, May 1981

  • Hoyng, P.; Duijveman, A.; Machado, M. E.
  • The Astrophysical Journal, Vol. 246
  • DOI: 10.1086/183574

Hard X‐Ray Emissions from Partially Occulted Solar Flares
journal, February 2008

  • Krucker, Sam; Lin, R. P.
  • The Astrophysical Journal, Vol. 673, Issue 2
  • DOI: 10.1086/524010

Solar Flare Hard X-Ray Emission from the High Corona
journal, October 2007

  • Krucker, Säm; White, S. M.; Lin, R. P.
  • The Astrophysical Journal, Vol. 669, Issue 1
  • DOI: 10.1086/523759

Gamma-Ray and High-Energy-Neutron Measurements on CORONAS-F during the Solar Flare of 28 October 2003
journal, November 2010


The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)
journal, June 2011


RHESSI Observations of a Simple Large X-Ray Flare on 2003 November 3
journal, July 2004

  • Liu, Wei; Jiang, Yan Wei; Liu, Siming
  • The Astrophysical Journal, Vol. 611, Issue 1
  • DOI: 10.1086/423371

Double Coronal Hard and Soft X‐Ray Source Observed by RHESSI : Evidence for Magnetic Reconnection and Particle Acceleration in Solar Flares
journal, March 2008

  • Liu, Wei; Petrosian, Vahé; Dennis, Brian R.
  • The Astrophysical Journal, Vol. 676, Issue 1
  • DOI: 10.1086/527538

The Height of a White-Light Flare and its hard X-Ray Sources
journal, June 2012

  • Martínez Oliveros, Juan-Carlos; Hudson, Hugh S.; Hurford, Gordon J.
  • The Astrophysical Journal, Vol. 753, Issue 2
  • DOI: 10.1088/2041-8205/753/2/L26

A loop-top hard X-ray source in a compact solar flare as evidence for magnetic reconnection
journal, October 1994

  • Masuda, S.; Kosugi, T.; Hara, H.
  • Nature, Vol. 371, Issue 6497
  • DOI: 10.1038/371495a0

The Likelihood Analysis of EGRET Data
journal, April 1996

  • Mattox, J. R.; Bertsch, D. L.; Chiang, J.
  • The Astrophysical Journal, Vol. 461
  • DOI: 10.1086/177068

The hard X-rays and gamma rays from solar flares
journal, August 1990

  • McTiernan, James M.; Petrosian, Vahe
  • The Astrophysical Journal, Vol. 359
  • DOI: 10.1086/169085

THE FERMI GAMMA-RAY BURST MONITOR
journal, August 2009


High-energy processes in solar flares
journal, February 1987

  • Murphy, R. J.; Dermer, C. D.; Ramaty, R.
  • The Astrophysical Journal Supplement Series, Vol. 63
  • DOI: 10.1086/191180

Soft X-ray Fluxes of Major Flares Far Behind the Limb as Estimated Using STEREO EUV Images
journal, May 2013


On the Nonthermal Emission and Acceleration of Electrons in Coma and Other Clusters of Galaxies
journal, August 2001

  • Petrosian, Vahe
  • The Astrophysical Journal, Vol. 557, Issue 2
  • DOI: 10.1086/321557

Loop Top Hard X‐Ray Emission in Solar Flares: Images and Statistics
journal, April 2002

  • Petrosian, Vahé; Donaghy, Timothy Q.; McTiernan, James M.
  • The Astrophysical Journal, Vol. 569, Issue 1
  • DOI: 10.1086/339240

Gamma-ray emission and electron acceleration in solar flares
journal, October 1994

  • Petrosian, Vahe; McTiernan, James M.; Marschhauser, Holger
  • The Astrophysical Journal, Vol. 434
  • DOI: 10.1086/174777

Evidence for the Formation of a Large-Scale Current Sheet in a Solar Flare
journal, September 2003

  • Sui, Linhui; Holman, Gordon D.
  • The Astrophysical Journal, Vol. 596, Issue 2
  • DOI: 10.1086/379343

Calibration of the Energetic Gamma-Ray Experiment Telescope (EGRET) for the Compton Gamma-Ray Observatory
journal, May 1993

  • Thompson, D. J.; Bertsch, D. L.; Fichtel, C. E.
  • The Astrophysical Journal Supplement Series, Vol. 86
  • DOI: 10.1086/191793

Use of the FITS World Coordinate System by STEREO/SECCHI
journal, December 2009


Evidence for a spatially extended component of gamma rays from solar flares
journal, May 1993

  • Vestrand, W. T.; Forrest, David J.
  • The Astrophysical Journal, Vol. 409
  • DOI: 10.1086/186862

The Large-Sample Distribution of the Likelihood Ratio for Testing Composite Hypotheses
journal, March 1938


EUVI: the STEREO-SECCHI extreme ultraviolet imager
conference, February 2004

  • Wuelser, Jean-Pierre; Lemen, James R.; Tarbell, Theodore D.
  • Optical Science and Technology, SPIE's 48th Annual Meeting, SPIE Proceedings
  • DOI: 10.1117/12.506877

Perpendicular Transport of Solar Energetic Particles in Heliospheric Magnetic Fields
journal, September 2003

  • Zhang, Ming; Jokipii, J. R.; McKibben, R. B.
  • The Astrophysical Journal, Vol. 595, Issue 1
  • DOI: 10.1086/377301

Works referencing / citing this record:

Source of Energetic Protons in the 2014 September 1 Sustained Gamma-ray Emission Event
journal, February 2020


Electron Power-Law Spectra in Solar and Space Plasmas
journal, June 2018


The Relationship between Long-Duration Gamma-Ray Flares and Solar Cosmic Rays
journal, July 2017


On the Shock Source of Sustained Gamma-Ray Emission from the Sun
journal, November 2019


On the expected γ-ray emission from nearby flaring stars
journal, October 2017

  • Ohm, S.; Hoischen, C.
  • Monthly Notices of the Royal Astronomical Society, Vol. 474, Issue 1
  • DOI: 10.1093/mnras/stx2806

EVIDENCE FOR ENHANCED 3 HE IN FLARE-ACCELERATED PARTICLES BASED ON NEW CALCULATIONS OF THE GAMMA-RAY LINE SPECTRUM
journal, December 2016


A Statistical Study to Determine the Origin of Long-duration Gamma-Ray Flares
journal, August 2018


Magnetic Flux Reconnection in Flaring Active Regions with Sustained Gamma-Ray Emission
journal, November 2018

  • Kahler, S. W.; Cliver, E. W.; Kazachenko, M.
  • The Astrophysical Journal, Vol. 868, Issue 2
  • DOI: 10.3847/1538-4357/aae9d8

Characteristics of Late-phase >100 MeV Gamma-Ray Emission in Solar Eruptive Events
journal, December 2018


Infrequent Occurrence of Significant Linear Polarization in H α Solar Flares
journal, February 2019


The Disappearing Solar Filament of 2013 September 29 and Its Large Associated Proton Event: Implications for Particle Acceleration at the Sun
journal, May 2019

  • Cliver, E. W.; Kahler, S. W.; Kazachenko, M.
  • The Astrophysical Journal, Vol. 877, Issue 1
  • DOI: 10.3847/1538-4357/ab0e03

Fermi -LAT Observations of the 2017 September 10 Solar Flare
journal, September 2018

  • Omodei, Nicola; Pesce-Rollins, Melissa; Longo, Francesco
  • The Astrophysical Journal, Vol. 865, Issue 1
  • DOI: 10.3847/2041-8213/aae077

The Relation between Escape and Scattering Times of Energetic Particles in a Turbulent Magnetized Plasma: Application to Solar Flares
journal, November 2018


On the expected $\gamma$-ray emission from nearby flaring stars
text, January 2017


Unexpected Dip in the Solar Gamma-Ray Spectrum
text, January 2018


Electron Power-Law Spectra in Solar and Space Plasmas
text, January 2018


A Statistical Study to Determine the Origin of Long-Duration Gamma-ray Flares
text, January 2018


On the Shock Source of Sustained Gamma-Ray Emission from the Sun
text, January 2019