Revised GLE database: Fluences of solar energetic particles as measured by the neutron-monitor network since 1956

I. Usoskin; S. Koldobskiy; G. A. Kovaltsov; A. Gil; I. Usoskina; T. Willamo; A. Ibragimov

doi:10.1051/0004-6361/202038272

Home

All issues

Volume 640 (August 2020)

A&A, 640 (2020) A17

Full HTML

Free Access

Fig. 4.

Open with DEXTER Download original image

Dependence of the χ² value on the MER spectral parameters (Eq. (5)) for GLE 38 shown in Fig. 3. The best-fit values () are shown with the red stars. The horizontal dashed blue line corresponds to , and the vertical blue arrows denote the 68% bounds for the parameter values.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.