Ref: SIDCimport-1199

PROBA2/SWAP EUV images of the large-scale EUV corona up to 3 solar radii: Can we close the gap in coronal magnetic field structure between 1.3 and 2.5 solar radii?

De Groof, A. ; Seaton, D.B. ; Rachmeler, L. A. ; Berghmans, D.

Talk presented at Joint American Astronomical Society/American Geophysical Union Triennial Earth-Sun Summit, meeting #1, #409.01 on 2015-xx-xx

The record appears in these collections:
Conference Contributions & Seminars > Conference Talks > Contributed Talks
Royal Observatory of Belgium > Solar Physics & Space Weather (SIDC)
Solar-Terrestrial Centre of Excellence

 Record created 2016-02-22, last modified 2016-02-22