REVIEW 2 cited by
Cosmic ray ensembles as signatures of ultra-high energy photons interacting with the solar magnetic field
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
read the original abstract
Propagation of ultra-high energy photons in the solar magnetosphere gives rise to cascades comprising thousands of photons. We study the cascade development using Monte Carlo simulations and find that the photons in the cascades are spatially extended over millions of kilometers on the plane distant from the Sun by 1 AU. We compare results from simulations which use two models of the solar magnetic field, and show that although signatures of such cascades are different for the models used, for practical detection purpose in the ground-based detectors, they are similar.
Forward citations
Cited by 2 Pith papers
-
Cosmic Ray Extremely Distributed Observatory: Status and perspectives of a global cosmic ray detection framework
CREDO proposes a global network of smartphones and established detectors to search for cosmic-ray ensembles, and reports a first null-result test of its time-correlation tool.
-
Public engagement as a scientific tool to implement multi-messenger strategies with the Cosmic-Ray Extremely Distributed Observatory
CREDO reports early operations and argues that large-scale public participation is necessary to search for cosmic-ray ensembles, a hypothesized new multi-messenger signal.
Discussion (0). Continue with ORCID to comment.