A comparative analysis of the helios and istp era sun-earth connection during solar minimum

Details A comparative analysis of the helios and istp era sun-earth connection during solar minimum A comparative analysis of the helios and istp era sun-earth connection during solar minimum

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....13892b&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #13892

Physics

Scientific paper

We discuss the similarities and differences of two intervals of extreme interplanetary solar wind conditions, separated almost precisely by two solar cycles, in Feb-Apr 1976 and Jan-Apr 2001. The similarities extend to various data-sets: Energetic particles, solar wind plasma and interplanetary magnetic field. In Jan-April 1979 observations were made by spacecraft at three locations covering a wide longitudinal range (from ~30 to 70°) in the heliosphere. Data are presented from Helios 2, Helios 1, and from near the Earth. Observations of the 1997 interval are from Wind, and solar conditions from SOHO. We examine the geomagnetic activity during each interval. This Study is partially supported by the following Grants: ATM-0208414 (NSF), and NASA NASW-02025 and NAG 5-10883

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