Comparison of outflow velocity determinations with UVCS and LASCO for the coronal mass ejection of 13-14 August 1997

Details Comparison of outflow velocity determinations with UVCS and LASCO for the coronal mass ejection of 13-14 August 1997 Comparison of outflow velocity determinations with UVCS and LASCO for the coronal mass ejection of 13-14 August 1997

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..637s&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 637-640 (1999).

Astronomy and Astrophysics

Astronomy

1

Solar Wind Plasma, Sources Of Solar Wind, Astronomical Observations

Scientific paper

The Ultraviolet Coronagraph Spectrometer (UVCS) on SOHO observed a Coronal Mass Ejection (CME) on 13-14 August 1997. The event was observed simultaneously with the LASCO white light coronagraphs. This paper describes the results from a comparison of outflow velocities determined from UVCS Doppler dimming studies with the velocities determined by examining the proper motions of the CME as measured by LASCO. In addition, estimates for line of sight velocities, densities and kinetic temperatures are discussed.

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