This catalog lists the radio signatures of in situ observed electron events from the ACE/EPAM instrument since 1996. The catalog is organized as a table that presents the remote radio signatures of electrons observed during solar cycle 23 (1996-2008) and 24 (2009-2018).
Explanatory notes:
The catalog provides the following information:
date of the electron event;
onset time (in UT) of the electron event;
solar origin:
flare SXR class, onset time and location
time of CME first appearance (in UT), linear speed (in km/s) and AW (in degrees);
radio burst types: appearance of types II, III, IV in different wavelength ranges;
RSTN identification: peak flux [sfu], peak frequency [MHz] and spectral index;
Comment.
The reported here peak radio flux is based on 1-sec data.
Abbreviations:
AW: angular width
nd: next day
pd: previous day
SXR: soft X-ray
u: uncertain
v: visual
wavelength ranges:
dm: decimetric (3-1 GHz)
dm-m: decimetric to metric (1 GHz-300 MHz)
m: metric (300-100 MHz)
m-Dm: metric to decametric (100-30 MHz)
Dm-Hm-km (DH-km): decametric-hectometric-kilometric (30 MHz-10 kHz)
If you want to use the results in a paper, book, or any other kind of electronic publication, please give credit to Radio emission signatures catalog http://newserver.stil.bas.bg/SEPcatalog/.
Preliminary results can be found in the publication:
R. Miteva, S. W. Samwel and V. Krupar, Solar energetic particles and radio burst emission, JSWSC (2017), DOI: 10.1051/swsc/2017035.
Acknowledgements:
For the identifications we use radio data and dynamic spectra provided by:
RSTN,
Wind/WAVES;
Radio monitoring;
as well as various ground-based observatories.
Flare information is adopted from: GOES flare listings and www.Solarmonitor.org;
and CME information from: CDAW LASCO CME catalog.
Contact: R. Miteva
Links:
Space Climate Group Homepage
Space Research and Technology Institute Homepage
