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Evolution of Coronal Mass Ejections and the Corresponding Forbush Decreases: Modeling vs. Multi-Spac...

Evolution of Coronal Mass Ejections and the Corresponding Forbush Decreases: Modeling vs. Multi-Spac...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2574937553

Evolution of Coronal Mass Ejections and the Corresponding Forbush Decreases: Modeling vs. Multi-Spacecraft Observations

About this item

Full title

Evolution of Coronal Mass Ejections and the Corresponding Forbush Decreases: Modeling vs. Multi-Spacecraft Observations

Publisher

Dordrecht: Springer Netherlands

Journal title

Solar physics, 2020-07, Vol.295 (7), Article 104

Language

English

Formats

Publication information

Publisher

Dordrecht: Springer Netherlands

More information

Scope and Contents

Contents

One of the very common in situ signatures of interplanetary coronal mass ejections (ICMEs), as well as other interplanetary transients, are Forbush decreases (FDs), i.e. short-term reductions in the galactic cosmic ray (GCR) flux. A two-step FD is often regarded as a textbook example, which presumably owes its specific morphology to the fact that t...

Alternative Titles

Full title

Evolution of Coronal Mass Ejections and the Corresponding Forbush Decreases: Modeling vs. Multi-Spacecraft Observations

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2574937553

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2574937553

Other Identifiers

ISSN

0038-0938

E-ISSN

1573-093X

DOI

10.1007/s11207-020-01671-7

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