Computer Science – Performance
Scientific paper
Feb 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jgr....90.1205b&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 90, Feb. 1, 1985, p. 1205-1216. Research sponsored by the U.S. Department
Computer Science
Performance
52
Energy Storage, Energy Transfer, Geomagnetic Tail, Magnetic Storms, Magnetospheric Instability, Energy Dissipation, Solar Terrestrial Interactions, Solar Wind, Time Response
Scientific paper
The concept of the Coordinated Data Analysis Workshop (CDAW) grew out of the International Magnetospheric Study (IMS) program. According to this concept, data are to be pooled from a wide variety of spacecraft and ground-based sources for limited time intervals. These data are to provide the basis for the performance of very detailed correlative analyses, usually with fairly limited physical problems in mind. However, in the case of the CDAW 6 truly global goals are involved. The primary goal is to trace the flow of energy from the solar wind through the magnetosphere to its ultimate dissipation by substorm processes. The present investigation has the specific goal to examine the evidence for the storage of solar wind energy in the magnetotail prior to substorm expansion phase onsets. Of particular interest is the determination, in individual substorm cases, of the time delays between the loading of energy into the magnetospheric system and the subsequent unloading of this energy.
Baker Daniel N.
Baumjohann Wolfgang
Fairfield Donald H.
Fritz Teresa A.
Kamide Yohsuke
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