The 10 September 2017 solar energetic particle (SEP) event was the largest since June 2015 and one of only two ground‐level enhancement (GLE) events of solar cycle 24. GLE events are subset of large SEP events (~15% of events identified by Space Weather Prediction Center) with particularly hard spectra, making them a substantial space weather hazard to space‐based instrumentation and exposed astronauts. We present analysis of the 10 September 2017 event and compare it to the other cycle 24 GLE events, to those of cycle 23, and also to two extreme SEP events observed by Solar Terrestrial Relations Observatory (STEREO). We find the 10 September 2017 event had a broken power law spectrum typical of GLE events but was softer than average at hig...
Solar energetic particles (SEPs) constitute an important component of the radiation environment in i...
Abstract The hourly-averaged of measurements of solar proton fluxes (from Jan' 73 to May 01) ha...
In this work, we apply an updated version of the Neutron Monitor (NM) Based Anisotropic GLE Pure Pow...
The 10 September 2017 solar energetic particle (SEP) event was the largest since June 2015 and one o...
The 10 September 2017 solar energetic particle (SEP) event was the largest since June 2015 and one o...
The Sun is already in the declining phase of cycle 24, but the paucity of high-energy solar energeti...
We discuss our findings from a survey of all large solar energetic particle (SEP) events of Solar Cy...
We report spacecraft measurements of the energy spectra of solar protons and other solar particle pr...
We present a study of the 2014 January 6 solar energetic particle event which produced a small groun...
Large solar eruptive events, including solar flares and coronal mass ejections (CMEs), can lead to s...
Measurements with the ACE, STEREO, and GOES spacecraft during the first 5.8 years of solar cycle 24 ...
In addition to several recent articles devoted to the rare event of ground-level enhancement of the ...
Solar energetic particles (SEPs) constitute a radiation hazard to both humans and hardware in space....
Large solar eruptive events, including solar flares and coronal mass ejections (CMEs), can lead to s...
Aims. The first relativistic solar proton event of solar cycle 25 was detected on 28 October 2021 by...
Solar energetic particles (SEPs) constitute an important component of the radiation environment in i...
Abstract The hourly-averaged of measurements of solar proton fluxes (from Jan' 73 to May 01) ha...
In this work, we apply an updated version of the Neutron Monitor (NM) Based Anisotropic GLE Pure Pow...
The 10 September 2017 solar energetic particle (SEP) event was the largest since June 2015 and one o...
The 10 September 2017 solar energetic particle (SEP) event was the largest since June 2015 and one o...
The Sun is already in the declining phase of cycle 24, but the paucity of high-energy solar energeti...
We discuss our findings from a survey of all large solar energetic particle (SEP) events of Solar Cy...
We report spacecraft measurements of the energy spectra of solar protons and other solar particle pr...
We present a study of the 2014 January 6 solar energetic particle event which produced a small groun...
Large solar eruptive events, including solar flares and coronal mass ejections (CMEs), can lead to s...
Measurements with the ACE, STEREO, and GOES spacecraft during the first 5.8 years of solar cycle 24 ...
In addition to several recent articles devoted to the rare event of ground-level enhancement of the ...
Solar energetic particles (SEPs) constitute a radiation hazard to both humans and hardware in space....
Large solar eruptive events, including solar flares and coronal mass ejections (CMEs), can lead to s...
Aims. The first relativistic solar proton event of solar cycle 25 was detected on 28 October 2021 by...
Solar energetic particles (SEPs) constitute an important component of the radiation environment in i...
Abstract The hourly-averaged of measurements of solar proton fluxes (from Jan' 73 to May 01) ha...
In this work, we apply an updated version of the Neutron Monitor (NM) Based Anisotropic GLE Pure Pow...