PROBLEM OF MISTAKES IN DATABASES, PROCESSING AND INTERPRETATION OF OBSERVATIONS OF THE SUN. II. SOLAR FLARES

Автор(и)

  • N. I. Lozitska Astronomical Observatory of Taras Shevchenko National University of Kyiv, Ukraine

DOI:

https://doi.org/10.18524/1810-4215.2016.29.85231

Ключові слова:

Sun, Solar Activity, Observations, Solar Flares, Solar Proton Events, correction the datasets

Анотація

The contribution of space-based observations of solar flares in the database for the past 50 years has increased significantly, almost completely replacing the ground observations. The statistical parameters of the temporal distribution of solar flares, obtained using ground-based and space-based observations, differ significantly. We investigated the reasons for these differences to be taken into account in the study of flare activity of the Sun in the solar activity cycles 21-24.

Посилання

Database SPDF NASA (Space Physics Data Facility, Goddard Space Flight Center, OMNIWeb), http://omniweb.gsfc.nasa.gov/ow.html/

Database NGDC NOAA (National Geophysical Data Center), ftp://ftp.ngdc.noaa.gov/STP/space-weather/solar-data/

Electronic library WDС (World Data Centers) http://www.wdcb.ru/stp/online_data.ru.html

ref113_r/ (Catalog of Solar Proton Events 1970-1979, 1982, 184 с;

Solar Proton Events. Catalogue 1980-1986, 1989, 159с.;

Catalogue of Solar Proton Events 1987-1996, 1998, 246с.; Catalogue of Solar Proton Events in the 23rd Cycle of Solar Activity (1996 – 2008), 2016, 740 с.)

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Опубліковано

2016-12-02

Номер

Том 29 (2016)

Розділ

Сонце та Сонячна система

Ліцензія

Авторське право (c) 2016 Odessa Astronomical Publications

Creative Commons License

Ця робота ліцензується відповідно до Creative Commons Attribution-NonCommercial 4.0 International License.

Відповідно Закону України про авторське право і суміжні права N 3792-XII від 23 грудня 1993 року