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Radial dependence of solar wind parameters in the ecliptic (1.1 Ro - 61 AU)

Koehnlein, W. (1996) Radial dependence of solar wind parameters in the ecliptic (1.1 Ro - 61 AU). Solar Physics, 1, pp. 209-213. Kluwer Academic Publishers.

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Abstract

The radial denpendence of four solar wind parameters (plasma density N, velocity V, temperature T, and magnitude of the interplanetary magnetic field B) are derived from remote sensing data of the solar corona and from in situ measurements in the heliosphere (Helios-1, 2,Pioneer-10, 11, and Voyager-1, 2). Using doubly logarithmic scaling ('solar wind parameter vs radial distance from the Sun') one finds two distinct intervals in the ecliptic, i.e., an exponential section within, approximately, the inner heliosphere and a linear section - up to at least 61 AU - in the outer heliosphere.

Document Type:Article
Additional Information: LIDO-Berichtsjahr=1996,
Title:Radial dependence of solar wind parameters in the ecliptic (1.1 Ro - 61 AU)
Authors:
AuthorsInstitution or Email of Authors
Koehnlein, W.UNSPECIFIED
Date:1996
Journal or Publication Title:Solar Physics
Refereed publication:Yes
In ISI Web of Science:Yes
Volume:1
Page Range:pp. 209-213
Publisher:Kluwer Academic Publishers
Series Name:169
Status:Published
HGF - Research field:UNSPECIFIED
HGF - Program:Space (old)
HGF - Program Themes:W EO - Erdbeobachtung
DLR - Research area:UNSPECIFIED
DLR - Program:W EO - Erdbeobachtung
DLR - Research theme (Project):UNSPECIFIED
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Institut für Planetenerkundung
Deposited By: elib DLR-Beauftragter
Deposited On:02 Apr 2006
Last Modified:27 Apr 2009 09:52

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