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This catalog lists the proton enhancements from the High Energy Detector (HED) aboard SOHO/ERNE instrument identified during solar cycle (SC) 23 (1996÷2008) and SC24 (2009÷2018). The catalog lists the peak intensity for the solar proton events in the different HED energy channels (in the range 14÷131 MeV) and additional information organized in table-form separately for SC23 and SC24.
Explanatory notes:
Proton peak: identified at the maximum of the particle profile (local enhancements are not considered).
Onset time: identified as the time of 3-sigma intensity value above pre-event level.
Peak time: the time at the peak proton intensity.
Jp: peak proton intensity after subtraction of the pre-event level in protons/(cm2 s sr MeV).
class: GOES soft X-ray flare class
speed: linear speed of the CME in km s-1
time: all time markers are in UT
Abbreviations:
AW: angular width of the CME (in degrees)
CME: coronal mass ejection
N/A: onset not found and/or it was fully masked by previous ongoing event
nd: next day
pd: previous day
p: peak is poorly defined
u: uncertain
v: visual
Acknowledgements:
We use proton data provided by SOHO/ERNE PI Prof. Eino Valtonen
(ERNE data is also available via: SEPServer data server);
flare information from: GOES flare listings and www.Solarmonitor.org;
and CME information from: CDAW LASCO CME catalog.
We acknowledge the use of SOHO/ERNE data in our study. SOHO is a project of international collaboration between ESA and NASA.
Disclaimer: The data used is a subject to instrumental saturation effects.
Contact: R. Miteva
Links:
Space Climate Group Homepage
Space Research and Technology Institute Homepage