Year: 2025
Type: conference-paper
Abstract: Neutron monitors are essential instruments for studying interplanetary conditions and space weather. Complementary to space-borne detectors, they extend the observable energy range beyond 50 GeV. While ground-level enhancements and Forbush decreases are well documented, shorter temporal increases in neutron count rates remain under-explored. This work investigates potential causes of such short intensity increases—single peaks—ranging from terrestrial effects (gamma-ray flashes, muon bursts) to solar energetic events and high-energy cosmic rays. Additionally, we aim to distinguish genuine physical phenomena from instrumental noise to avoid spurious data interpretation.
DOI: 10.22323/1.501.1364
Author: Danislav Sapundjiev
Institution: Royal Meteorological Institute of Belgium
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
OpenAlex ID: W4415363274
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