Physical properties of coronal streamers as observed by Spartan 201

Details Physical properties of coronal streamers as observed by Spartan 201 Physical properties of coronal streamers as observed by Spartan 201

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..239m&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 239-242 (1999).

Computer Science

Ultraviolet

Scientific paper

The three Spartan 201 flights from 1993 to 1995 provided us with observations in HI Lyman-α of several streamers in the declining phase of the current solar cycle. Analysis of the heliocentric height dependence of the HI Ly-α LOS velocity distribution width clearly show that there is a maximum in the proton 1/e velocities at heights ranging from 2.1 to 2.5 Rsolar for all of the observed streamers. We compare UVCS/Spartan results with proton velocity distributions from UVCS/SOHO during solar minimum. We also discuss differences in the proton velocity distributions for different types of streamers over the three year period of Spartan 201 observations.

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