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IPS activity observed as a precursor of solar induced terrestrial activityA radio telescope designed to exploit the interplanetary scintillation (IPS) technique and locate, map, and track solar wind disturbances which result in geomagnetic disturbances, thereby providing a forecast capability, is described. Preliminary results from operation of the telescope include: (1) evidence for a precursor signal in the IPS activity with a 1-2 day lead time with respect to density enhancements which frequently give rise to geomagnetic activity; (2) detection of a spectral broadening signature which also serves as a precursor of geomagnetic activity; (3) out-of-the-ecliptic plasma density enhancements which were not detected by near-Earth, ecliptic plane spacecraft; (4) detection of 12 corotating density enhancements;(5) detection of over 80 sources which give detectable scintillation of which 45 have been used for detailed synoptic analysis and 9 for spectral analysis; and (6) measurement of 0-lag coefficient of 0.56 between density and IPS activity enhancements.
Document ID
19790009953
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Cronyn, W. M.
(Iowa Univ. Iowa City, IA, United States)
Shawhan, S. D.
(Iowa Univ. Iowa City, IA, United States)
Rickard, J. J.
(Iowa Univ. Iowa City, IA, United States)
Mitchell, D. G.
(Iowa Univ. Iowa City, IA, United States)
Roelof, E. C.
(APL Laurel, Md., United States)
Gotwols, B. L.
(APL Laurel, Md., United States)
Date Acquired
August 10, 2013
Publication Date
November 1, 1978
Publication Information
Publication: AGARD Operational Modelling of the Aerospace Propagation Environ., Vol. 1 and 2
Subject Category
Solar Physics
Accession Number
79N18124
Funding Number(s)
CONTRACT_GRANT: AFOSR-NPP-75-157
CONTRACT_GRANT: NOAA-04-3-022-289
CONTRACT_GRANT: N00017-72-C-4401
CONTRACT_GRANT: NSF ATM-73-06559
CONTRACT_GRANT: NGL-16-001-002
Distribution Limits
Public
Copyright
Other
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