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AbstractAbstract
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Journal Article
Journal
Journal of Geophysical Research; v. 77(31); p. 6226-6229
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AbstractAbstract
No abstract available
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Schindler, Karl (ed.); p. 113-122; 1972; Plenum Publishing Corp; New York; Conference on cosmic plasma physics; Frascati, Italy; 20 Sep 1971
Record Type
Book
Literature Type
Conference
Country of publication
Reference NumberReference Number
INIS VolumeINIS Volume
INIS IssueINIS Issue
Chao, J.K.; Sheu, J.H.
STIP symposium on physical interpretation of solar/interplanetary and cometary intervals1987
STIP symposium on physical interpretation of solar/interplanetary and cometary intervals1987
AbstractAbstract
[en] Three interplanetary shock wave events are selected from the plasma and magnetic field data of Helios 1 and 2, IMP-8, and Voyagers 1 and 2 for study of the interactions of a weak interplantary shock with a nonuniform ambient solar wind. These events occurred during the periods 22-26 November 1977, 1-7 January 1978, and 2-5 April 1979, respectively. It is found that the shock surfaces of these events are highly distorted. In addition, a portion of the shock surface may be degenerated into a disturbance which does not satisfy the Rankine-Hugoniot jump conditions
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National Aeronautics and Space Administration, Greenbelt, MD (USA). Goddard Space Flight Center; vp; Sep 1987; vp; STIP symposium on physical interpretation of solar/interplanetary and cometary intervals; Huntsville, AL (USA); 12-15 May 1987; Available from NTIS, PC A04/MF A01
Record Type
Report
Literature Type
Conference; Numerical Data
Report Number
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Reference NumberReference Number
INIS VolumeINIS Volume
INIS IssueINIS Issue
AbstractAbstract
No abstract available
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Journal Article
Journal
Journal of Geophysical Research; v. 77(28); p. 5455-5466
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Reference NumberReference Number
INIS VolumeINIS Volume
INIS IssueINIS Issue
AbstractAbstract
No abstract available
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Source
Schindler, Karl (ed.); p. 103-104; 1972; Plenum Publishing Corp; New York; Conference on cosmic plasma physics; Frascati, Italy; 20 Sep 1971
Record Type
Book
Literature Type
Conference
Country of publication
Reference NumberReference Number
INIS VolumeINIS Volume
INIS IssueINIS Issue
Chao, J.K.; Sakurai, K.
National Aeronautics and Space Administration, Greenbelt, Md. (USA). Goddard Space Flight Center1974
National Aeronautics and Space Administration, Greenbelt, Md. (USA). Goddard Space Flight Center1974
AbstractAbstract
[en] The interaction of the earth's magnetic field with the solar wind is discussed with emphasis on the influence of solar flares. The geomagnetic storms are considered to be the result of the arrival of shock wave generated by solar flares in interplanetary space. Basic processes in the solar atmosphere and interplanetary space, and hydromagnetic disturbances associated with the solar flares are discussed along with observational and theoretical problems of interplanetary shock waves. The origin of interplanetary shock waves is also discussed. (U.S.)
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Source
Jun 1974; 48 p; NASA-TM-X--70683; X--693-74-168
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Report
Report Number
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Reference NumberReference Number
INIS VolumeINIS Volume
INIS IssueINIS Issue
AbstractAbstract
No abstract available
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Record Type
Journal Article
Journal
Journal of Geophysical Research; v. 77(31); p. 6060-6070
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Reference NumberReference Number
INIS VolumeINIS Volume
INIS IssueINIS Issue
AbstractAbstract
No abstract available
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Source
Russell, C.T. (ed.); p. 169-174; 1974; Univ. of California; Los Angeles; 3. conference on solar wind three; Pacific Grove, CA, USA; 25 Mar 1974
Record Type
Book
Literature Type
Conference
Country of publication
Reference NumberReference Number
INIS VolumeINIS Volume
INIS IssueINIS Issue
AbstractAbstract
[en] The propagation and dissipation of interplanetary shock waves (IPS) generated by coronal mass ejection (CME) or corotating streams of solar flare ejecta are considered. CME shocks interact with the solar wind, resulting in shock fronts which propagate at uneven velocities in different regions. The solar wind may also dampen out the fronts at various locations so that the propagating fronts deviate from the spherical and have holes. The dissipation in the solar wind can degrade the shocks into fast MHD waves. An expression is developed for predicting the probability that a shock wave will disappear at a given distance from the sun. 21 references
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Source
25. plenary session of COSPAR; Graz (Austria); 25 Jun - 7 Jul 1984; CONF-8406167--
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Journal Article
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Conference
Journal
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INIS IssueINIS Issue
AbstractAbstract
[en] Equations are derived which allow the ratio of specific heats behind the earth's bow shock to be evaluated if several pre-shock parameters (the specific-heat ratio, the Alfvenic Mach number, the sonic Mach number, and the angle between the shock normal at the stagnation point and the magnetic field) and the density jump across the shock are known. Numerical examples show that the dependence of the post-shock ratio on the pre-shock ratio is weak
Primary Subject
Secondary Subject
Source
Russell, C.T. (ed.); p. 455-459; 1974; Univ. of California; Los Angeles; 3. conference on solar wind three; Pacific Grove, CA, USA; 25 Mar 1974
Record Type
Book
Literature Type
Conference
Country of publication
Reference NumberReference Number
INIS VolumeINIS Volume
INIS IssueINIS Issue
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