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NuSTAR Hard X-Ray Observation of a Sub-A Class Solar Flare

Glesener, Lindsay and Krucker, Säm and Hannah, Iain G. and Hudson, Hugh and Grefenstette, Brian W. and White, Stephen M. and Smith, David M. and Marsh, Andrew J. (2017) NuSTAR Hard X-Ray Observation of a Sub-A Class Solar Flare. Astrophysical Journal, 845 (2). Art. No. 122. ISSN 1538-4357. https://resolver.caltech.edu/CaltechAUTHORS:20170911-142325771

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Abstract

We report a Nuclear Spectroscopic Telescope Array (NuSTAR) observation of a solar microflare, SOL2015-09-01T04. Although it was too faint to be observed by the GOES X-ray Sensor, we estimate the event to be an A0.1 class flare in brightness. This microflare, with only ~5 counts s^(−1) detector−1 observed by the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI), is fainter than any hard X-ray (HXR) flare in the existing literature. The microflare occurred during a solar pointing by the highly sensitive NuSTAR astrophysical observatory, which used its direct focusing optics to produce detailed HXR microflare spectra and images. The microflare exhibits HXR properties commonly observed in larger flares, including a fast rise and more gradual decay, earlier peak time with higher energy, spatial dimensions similar to the RHESSI microflares, and a high-energy excess beyond an isothermal spectral component during the impulsive phase. The microflare is small in emission measure, temperature, and energy, though not in physical size; observations are consistent with an origin via the interaction of at least two magnetic loops. We estimate the increase in thermal energy at the time of the microflare to be 2.4 × 10^(27) erg. The observation suggests that flares do indeed scale down to extremely small energies and retain what we customarily think of as "flare-like" properties.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-4357/aa80e9DOIArticle
http://iopscience.iop.org/article/10.3847/1538-4357/aa80e9/metaPublisherArticle
https://arxiv.org/abs/1707.04770arXivDiscussion Paper
ORCID:
AuthorORCID
Glesener, Lindsay0000-0001-7092-2703
Hannah, Iain G.0000-0003-1193-8603
Hudson, Hugh0000-0001-5685-1283
Grefenstette, Brian W.0000-0002-1984-2932
White, Stephen M.0000-0002-8574-8629
Smith, David M.0000-0002-0542-5759
Marsh, Andrew J.0000-0003-1086-6900
Additional Information:© 2017 American Astronomical Society. Received 2017 April 12 Accepted 2017 July 17 Published 2017 August 18 Support for this work was provided by NASA HSR grant NNX14AG07G, as well as an NSF Faculty Development Grant (AGS-1429512) to the University of Minnesota. S.K. acknowledges funding from the Swiss National Science Foundation (200021-140308 and 200020-169046). I.G.H. is supported by a Royal Society University Fellowship. The authors are grateful to the NuSTAR Science and Operation teams for promoting and supporting solar observations, to Matej Kuhar and Kathy Reeves for insightful comments on paper drafts, and to the anonymous reviewer for excellent comments and questions that undoubtedly improved the paper.
Funders:
Funding AgencyGrant Number
NASANNX14AG07G
NSFAGS-1429512
Swiss National Science Foundation (SNSF)200021-140308
Swiss National Science Foundation (SNSF)200020-169046
Royal Society University FellowshipUNSPECIFIED
Issue or Number:2
Record Number:CaltechAUTHORS:20170911-142325771
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170911-142325771
Official Citation:Lindsay Glesener et al 2017 ApJ 845 122
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:81308
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:11 Sep 2017 21:44
Last Modified:03 Oct 2019 18:41

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