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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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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.

Item URL in elib:https://elib.dlr.de/35382/
Document Type:Article
Additional Information: LIDO-Berichtsjahr=1996,
Title:Radial dependence of solar wind parameters in the ecliptic (1.1 Ro - 61 AU)
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Journal or Publication Title:Solar Physics
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In ISI Web of Science:Yes
Page Range:pp. 209-213
Publisher:Kluwer Academic Publishers
Series Name:169
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: DLR-Beauftragter, elib
Deposited On:02 Apr 2006
Last Modified:27 Apr 2009 09:52

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