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image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Journal of Geophysic...arrow_drop_down
image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao
Journal of Geophysical Research Atmospheres
Article . 1961 . Peer-reviewed
License: Wiley TDM
Data sources: Crossref
https://doi.org/10.1029/sp037p...
Part of book or chapter of book . 1993 . Peer-reviewed
Data sources: Crossref
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Intensity variations in outer Van Allen radiation belt

Authors: D. Venkatesan; Scott E. Forbush; Carl E. McIlwain;

Intensity variations in outer Van Allen radiation belt

Abstract

Using data from Explorer VII, the changes in the intensity of the outer Van Allen radiation belt were investigated in detail over the period October 26, 1959, to December 9, 1959. To relate the intensities to location in the belt, the parameter L was used. L is defined as a function of the integral invariant I and scalar magnetic field B, such that everywhere on the shell described by the motion of a trapped particle in the earth's magnetic field, L closely approximates the equatorial radius of the shell. For the period under study, the intensity variations at selected values of L were negatively correlated with geomagnetic activity. However, an analysis of data over a much longer period is required to determine whether this correlation is statistically significant. For the period studied, the decrease in measured intensity during periods of magnetic storms (large a/sub p/) is consistent with the idea that some of the particles are 'dumped' into the auroral and subauroral zones where they may partly contribute to the auroral zone currents that account for a /sub p/. In addition, the reduction in intensity generally occurred in the outer part of the zone. The low values of intensity, formore » L = 3.5, 4.1, and 4.7, oc curred in the interval November 22 to December 9, at times when the equatorial ring current field, U (southward on the earth at the equator), was large. Thus, U cannot be due to the westward current due to the longitudinal drift of measured trapped particles in the region for which L is greater than 3.5, since a decrease in particle density therein would diminish the westward drift current with a consequent decrease in U, which is opposite to what is observed. This result indicates that the site of the ring current is either elsewhere, or that the principal contribution to it comes from drifting particles having energies below the detection thresholds of Explorer VII equipment. The phenomena were investigated over a longer period, using daily averages of the maximum counting rates. This procedure had serious limitations. (auth)« less

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
22
Average
Top 10%
Top 10%
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