Solar Physics

, Volume 107, Issue 1, pp 63–72

Shifts of the Caii K line in Hei 10830 dark points

Authors

  • Rush D. Holt
    • Physics DepartmentSwarthmore College
  • D. J. Mullan
    • Bartol Research Foundation of the Franklin Institute, University of Delaware
Article

DOI: 10.1007/BF00155342

Cite this article as:
Holt, R.D. & Mullan, D.J. Sol Phys (1986) 107: 63. doi:10.1007/BF00155342

Abstract

We investigate the velocity field of the solar chromosphere at the location of 65 He i 10830 dark points (DP's). We have obtained spectra of such points in the vicinity of the Ca II K line. As a measure of differential chromospheric velocity, we use the shift of the K line center relative to a nearby photospheric Fe i line. We find that in He i DP's, the distribution of K line shifts is skewed towards the blue: the blueward skewing is more pronounced in He i DP's located in coronal holes. To the extent that He i DP's are proxies of coronal bright points, our study is relevant to previous reports of outflows from such bright points.

Copyright information

© D. Reidel Publishing Company 1986