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Some characteristics of the GLE on 10 September 2017

In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no. 2
V. Kurt - A. Belov - K. Kudela - B. Yushkov

Details:

Year, pages: 2018, 329 - 338
Keywords:
solar flare, solar proton event, ground level enhancement
About article:
We present a short overview of the event associated with the recent strong solar flare on 10 September 2017 (X8.2) based on the available data both from satellite GOES-13 and from selected neutron monitors. The onset time of SPE/GLE at 1 AU was found between 16:06—16:08 UT. The GLE effect was anisotropic with a maximum increase of 6%. The maximum energy of accelerated protons was ≈ 6 GeV. We estimated the release time of sub-relativistic protons into open field lines as 15:53—15:55 UT.
How to cite:
ISO 690:
Kurt, V., Belov, A., Kudela, K., Yushkov, B. 2018. Some characteristics of the GLE on 10 September 2017. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no.2, pp. 329-338. 1335-1842.

APA:
Kurt, V., Belov, A., Kudela, K., Yushkov, B. (2018). Some characteristics of the GLE on 10 September 2017. Contributions of the Astronomical Observatory Skalnaté Pleso, 48(2), 329-338. 1335-1842.