Calibration of the GOES 13/15 high-energy proton detectors based on the PAMELA solar energetic particle observations
Author:
Affiliation:
1. Istituto Nazionale di Fisica Nucleare; Bari Italy
Funder
PAMELA collaboration
Publisher
American Geophysical Union (AGU)
Subject
Atmospheric Science
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1002/2017SW001672/fullpdf
Reference27 articles.
1. Observations of the 2006 December 13 and 14 solar particle events in the 80 MeV n−1-3 GeV n−1 range from space with the PAMELA detector;Adriani;Astrophys. J.,2011
2. Time dependence of the proton flux measured by PAMELA during the 2006 July-2009 December solar minimum;Adriani;Astrophys. J.,2013
3. The PAMELA Mission: Heralding a new era in precision cosmic ray physics;Adriani;Phys. Rep.,2014
4. Trapped proton fluxes at low Earth orbits measured by the PAMELA experiment;Adriani;Astrophys. J.,2015a
5. Re-entrant albedo proton fluxes measured by the PAMELA experiment;Adriani;J. Geophys. Res. Space Physics,2015b
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