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The Coronal-Sounding Experiment.

Bird, M.K. 1), Asmar, S.W. 2), Brenkle, J.P. 2), Edenhofer, P. 3), Paetzold, M., Volland, H. 1), (1992) The Coronal-Sounding Experiment. Astron. Astrophys. Suppl. Ser., 92, pp. 425-430.

Full text not available from this repository.

Abstract

The main science objective of the Ulysses Solar Corona Experiment is to derive the plasma parameters of the solar atmosphere using established coronal-sounding techniques. Applying appropriate model assumptions, the 3-D electron density distribution will be determined from dual-frequency ranging and Doppler measurements recorded at the NASA Deep Space Network during the solar conjunctions. Multi-station observations will be used to derive the plasma bulk velocity at solar distances where the solar wind is expected to undergo its greatest acceleration. As a secondary objective profiting from the favorable geometry during Jupiter encounter, radio-sounding measurements will yield a unique cross-scan of the electron density in the Io Plasma Torus.

Document Type:Article
Additional Information: LIDO-Berichtsjahr=1992,
Title:The Coronal-Sounding Experiment.
Authors:
AuthorsInstitution or Email of Authors
Bird, M.K. 1), Asmar, S.W. 2), Brenkle, J.P. 2), Edenhofer, P. 3), Paetzold, M., Volland, H. 1), UNSPECIFIED
Date:1992
Journal or Publication Title:Astron. Astrophys. Suppl. Ser.
Refereed publication:Yes
In ISI Web of Science:Yes
Volume:92
Page Range:pp. 425-430
Status:Published
Keywords:Interplanetary Medium, Solar Corona
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: Oberpfaffenhofen
Institutes and Institutions:Institut für Hochfrequenztechnik
Deposited By: elib DLR-Beauftragter
Deposited On:02 Apr 2006
Last Modified:27 Apr 2009 08:47

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