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Characteristics of a stable arc based on FAST and MIRACLE observations
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2000 (English)In: ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, ISSN 0992-7689, Vol. 18, no 2, 152-160 p.Article in journal (Refereed) Published
Abstract [en]

A stable evening sector are is studied using observations from the FAST satellite at 1250 km altitude and the MIRACLE ground-based network, which contains all-sky cameras, coherent radars (STARE), and magnetometers. Both FAST and STARE observe a northward

Place, publisher, year, edition, pages
SPRINGER VERLAG , 2000. Vol. 18, no 2, 152-160 p.
Keyword [en]
ionosphere (auroral ionosphere; ionosphere-magnetosphere interactions); magnetospheric physics (auroral phenomena); HALL CONDUCTANCE DISTRIBUTION; MAGNETIC-FIELD DATA; AURORAL ARC; ELECTRIC-FIELD; RADAR
Identifiers
URN: urn:nbn:se:uu:diva-36995OAI: oai:DiVA.org:uu-36995DiVA: diva2:64894
Note
Addresses: Janhunen P, Finnish Meteorol Inst, FIN-00101 Helsinki, Finland. Finnish Meteorol Inst, FIN-00101 Helsinki, Finland. Swedish Inst Space Phys, Uppsala Div, Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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