ground level enhancements
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Space Weather ◽  
2021 ◽  
Author(s):  
A. D. P. Hands ◽  
F. Baird ◽  
K. A. Ryden ◽  
C. S. Dyer ◽  
F. Lei ◽  
...  

Solar Physics ◽  
2020 ◽  
Vol 295 (7) ◽  
Author(s):  
Leonty I. Miroshnichenko ◽  
Chuan Li ◽  
Victor G. Yanke

2020 ◽  
Vol 67 (6) ◽  
pp. 1139-1143
Author(s):  
Alexander Dyer ◽  
Alex Hands ◽  
Keith Ryden ◽  
Clive Dyer ◽  
Ian Flintoft ◽  
...  

2020 ◽  
Vol 10 ◽  
pp. 17
Author(s):  
Alexander Mishev ◽  
Ilya Usoskin

The global neutron monitor network has been successfully used over several decades to study cosmic ray variations and fluxes of energetic solar particles. Nowadays, it is used also for space weather purposes, e.g. alerts and assessment of the exposure to radiation. Here, we present the current status of the global neutron monitor network. We discuss the ability of the global neutron monitor network to study solar energetic particles, specifically during large ground level enhancements. We demonstrate as an example, the derived solar proton characteristics during ground level enhancements GLE #5 and the resulting effective dose over the globe at a typical commercial jet flight altitude of 40 kft (≈12,200 m) above sea level. We present a plan for improvement of space weather services and applications of the global neutron monitor network, specifically for studies related to solar energetic particles, namely an extension of the existing network with several new monitors. We discuss the ability of the optimized global neutron monitor network to study various populations of solar energetic particles and to provide reliable space weather services.


2019 ◽  
Vol 9 ◽  
pp. E1 ◽  
Author(s):  
Alexander Mishev ◽  
Piers Jiggens

The Sun emits energetic particles following eruptive events such as solar flares and Coronal Mass Ejections (CMEs). Solar Energetic Particles (SEPs) arrive in bursts known as Solar Particle Events (SPEs), which penetrate into the Earth’s magnetosphere. SEPs with large enough energy induce a complicated atmospheric cascade, which secondary particles lead to an enhancement of count rate of ground-based detectors e.g. Neutron Monitors (NMs). This class of SEPs is therefore referred as Ground Level Enhancements (GLEs). The characterisation of the high-energy SEPs environment with corresponding space weather effects is important for space flights, aviation, and satellite industry. In this topical issue recent developments, addressing important user needs in the space radiation environment domain are published. Some articles are relevant to the specification of the SEP environment whilst others focus on space weather prediction of SEP fluxes. Catalogues based on measurement and processing of SEPs including ground-based data, and modelling of aircrew radiation exposure during major events are also presented.


Solar Physics ◽  
2018 ◽  
Vol 293 (7) ◽  
Author(s):  
Sergey A. Koldobskiy ◽  
Gennady A. Kovaltsov ◽  
Ilya G. Usoskin

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