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The flare origin of Forbush decreases not associated with solar flares on the visible hemisphere of the SunInvestigations have shown that Forbush decreases (Fds) are produced by the propagation into the interplanetary space of a strong perturbation originating from a solar flare (Sf) accompanied by Type IV radioemission. As the front of the perturbation propagates into the interplanetary space, the region in which the galactic cosmic rays are modulated (Fd-modulated region) rotates westward with the Sun and is generally included between two boundary streams; therefore the Fds not associated with observed type IV Sfs (N.Ass.Fds) are likely to be produced by type IV Sfs occurred on the Sun's backside: these vents can be observed when the Earth crosses the corotating Western boundary of the modulated region.
Document ID
19850026745
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Iucci, N.
(Consiglio Nazionale delle Ricerche Rome, Italy)
Parisi, M.
(Consiglio Nazionale delle Ricerche Rome, Italy)
Signorini, C.
(Consiglio Nazionale delle Ricerche Rome, Italy)
Storini, M.
(Consiglio Nazionale delle Ricerche Rome, Italy)
Villoresi, G.
(Consiglio Nazionale delle Ricerche Rome, Italy)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 5
Subject Category
Solar Physics
Report/Patent Number
SH-5.1-4
Accession Number
85N35058
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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