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Galactic Cosmic Ray Energy Spectrum for Fe from ~0.8 to ~10 GeV/nuc with the SuperTIGER Instrument

Labrador, A. W. and Binns, W. R. and Bose, R. G. and Brandt, T. J. and Dowkontt, P. F. and Hams, T. and Israel, M. H. and Link, J. T. and Mewaldt, R. A. and Mitchell, J. W. and Murphy, R. P. and Rauch, B. F. and Sakai, K. and Sasaki, M. and Stone, E. C. and Waddington, C. J. and Ward, J. E. and Wiedenbeck, M. E. (2017) Galactic Cosmic Ray Energy Spectrum for Fe from ~0.8 to ~10 GeV/nuc with the SuperTIGER Instrument. In: 35th International Cosmic Ray Conference (ICRC2017). Proceedings of Science. No.301. SISSA , Trieste, Italy, Art. No. 167. http://resolver.caltech.edu/CaltechAUTHORS:20180828-122926511

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Abstract

SuperTIGER (Trans-Iron Galactic Element Recorder) is a large-area balloon-borne instrument built to measure the galactic cosmic-ray abundances of elements from Z=10 (Ne) through Z=56 (Ba) at energies from 0.8 to ~10 GeV/nuc. SuperTIGER successfully flew around Antarctica for a record-breaking 55 days, from December 8, 2012 to February 1, 2013. In this paper, we present results of an analysis of the data taken during the flight for Fe (Z=26). We report on energy calibrations and instrumental and atmospheric corrections to obtain cosmic ray intensities vs. energy, and we will compare selected SuperTIGER galactic cosmic ray Fe spectrum with those from ACE/SIS during the time of the SuperTIGER flight.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.22323/1.301.0167DOIArticle
ORCID:
AuthorORCID
Brandt, T. J.0000-0003-4087-1786
Mewaldt, R. A.0000-0003-2178-9111
Stone, E. C.0000-0002-2010-5462
Additional Information:Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License. This work was supported by NASA under grants NNX09AC17G NNX09AC18G, NNX14AB24G, NNX14AB25G, and NNX15AC15G, by the Peggy and Steve Fossett Foundation, and by the McDonnell Center for the Space Sciences at Washington University in St. Louis. We thank the ACE/CRIS instrument team and the ACE Science Center for providing ACE data.
Funders:
Funding AgencyGrant Number
NASANNX09AC17G
NASANNX09AC18G
NASANNX14AB24G
NASANNX14AB25G
NASANNX15AC15G
Peggy and Steve Fossett FoundationUNSPECIFIED
McDonnell Center for the Space SciencesUNSPECIFIED
Record Number:CaltechAUTHORS:20180828-122926511
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20180828-122926511
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:89248
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:30 Aug 2018 20:44
Last Modified:30 Aug 2018 20:44

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