Questions / Comments: sabrina.savage [at] nasa.gov

HOP INSTRUCTION PAGE



HOP 269, TOO

Prominence-Coronal Cavity Systems: Cyclic Mass Transport and Magnetic Flux Emergence

Number of runs (8/24/15):    2

Dates:    Oct-14; Feb-15

Primary Proposer(s):

W. Liu -- weiliu [at] lmsal.com

Co-proposer(s):

Okamoto -- take [at] joten.info
De Pontieu -- bdp [at] lmsal.com
Tarbell -- tarbell [at] lmsal.com
Berger -- tberger [at] nso.edu


HOP Productivity:

No productivity information provided.


REASON FOR LACK OF PRODUCTIVITY:

During the first run in 2014-Oct, the IRIS slit missed the prominence bubble, although SOT/BFI captured the bubble within its field of view. Data analysis is currently underway. During the second run in 2015-Feb, the target prominence was missed.