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Galactic Cosmic-Ray Composition and Spectra for Ne through Cu from 0.8 to 10 GeV/nuc with the SuperTIGER Instrument

Labrador, A. W. and Binns, W. R. and Brandt, T. J. 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. (2015) Galactic Cosmic-Ray Composition and Spectra for Ne through Cu from 0.8 to 10 GeV/nuc with the SuperTIGER Instrument. In: 34th International Cosmic Ray Conference (ICRC2015). Proceedings of Science. No.236. SISSA , Trieste, Italy, Art. No. 341. https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925420

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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 elements from Z=10 (Ne) to Z=28 (Ni). We report excellent charge separation throughout this range, with an Fe charge resolution of 0.16 charge units. Using a small sample of our data (~1/40th of our total), we will compare our galactic element secondary to primary ratios (e.g. (Sc+Ti+V)/Fe) with those from other instruments operating at different energy ranges.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.22323/1.236.0341DOIArticle
ORCID:
AuthorORCID
Labrador, A. W.0000-0001-9178-5349
Binns, W. R.0000-0001-6110-3407
Brandt, T. J.0000-0003-4087-1786
Israel, M. H.0000-0002-8104-208X
Mewaldt, R. A.0000-0003-2178-9111
Stone, E. C.0000-0002-2010-5462
Wiedenbeck, M. E.0000-0002-2825-3128
Additional Information:Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-ShareAlike. 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.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANNX09AC17G
NASANNX09AC18G
NASANNX14AB24G
NASANNX14AB25G
NASANNX15AC15G
Peggy and Steve Fossett FoundationUNSPECIFIED
McDonnell Center for the Space SciencesUNSPECIFIED
Series Name:Proceedings of Science
Issue or Number:236
Record Number:CaltechAUTHORS:20180828-122925420
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925420
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:89238
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:30 Aug 2018 21:49
Last Modified:09 Mar 2020 13:19

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