A braided synthetic magnetic field in the low solar atmosphere reproduces the solar disk gamma-ray spectrum above 10 GeV and explains the 30-100 GeV rebrightening through enhanced cosmic-ray trapping.
Title resolution pending
1 Pith paper cite this work, alongside 30 external citations. Polarity classification is still indexing.
1
Pith paper citing it
30
external citations · OpenAlex
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Solar disk gamma-rays emission via synthetic magnetic field from photosphere to low corona
A braided synthetic magnetic field in the low solar atmosphere reproduces the solar disk gamma-ray spectrum above 10 GeV and explains the 30-100 GeV rebrightening through enhanced cosmic-ray trapping.