Applications of Information Theory in Solar and Space Physics.
conditional mutual information
geosynchronous orbit electron flux
information theory
mutual information
radiation belts
solar cycle
solar dynamo
solar wind drivers
sunspot number
transfer entropy
Journal
Entropy (Basel, Switzerland)
ISSN: 1099-4300
Titre abrégé: Entropy (Basel)
Pays: Switzerland
ID NLM: 101243874
Informations de publication
Date de publication:
01 Feb 2019
01 Feb 2019
Historique:
received:
10
12
2018
revised:
18
01
2019
accepted:
20
01
2019
entrez:
3
12
2020
pubmed:
1
2
2019
medline:
1
2
2019
Statut:
epublish
Résumé
Characterizing and modeling processes at the sun and space plasma in our solar system are difficult because the underlying physics is often complex, nonlinear, and not well understood. The drivers of a system are often nonlinearly correlated with one another, which makes it a challenge to understand the relative effects caused by each driver. However, entropy-based information theory can be a valuable tool that can be used to determine the information flow among various parameters, causalities, untangle the drivers, and provide observational constraints that can help guide the development of the theories and physics-based models. We review two examples of the applications of the information theoretic tools at the Sun and near-Earth space environment. In the first example, the solar wind drivers of radiation belt electrons are investigated using mutual information (MI), conditional mutual information (CMI), and transfer entropy (TE). As previously reported, radiation belt electron flux (
Identifiants
pubmed: 33266856
pii: e21020140
doi: 10.3390/e21020140
pmc: PMC7514618
pii:
doi:
Types de publication
Journal Article
Review
Langues
eng
Subventions
Organisme : NASA
ID : NNX15AJ01G
Pays : United States
Organisme : NASA
ID : NNX16AQ87G
Pays : United States
Organisme : NASA
ID : NNX14AM27G
Pays : United States
Organisme : National Science Foundation
ID : AGS-1203299
Références
Phys Rev Lett. 2000 Jul 10;85(2):461-4
pubmed: 10991308
Phys Rev Lett. 2007 Mar 30;98(13):131103
pubmed: 17501179
Science. 2013 Apr 12;340(6129):186-90
pubmed: 23450000
Sci Rep. 2018 Nov 19;8(1):16987
pubmed: 30451956