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

HOP INSTRUCTION PAGE



HOP 141, TOO

Velocity flows in quiet sun magnetic loop footpoints

Number of runs (8/24/15):    2

Dates:    ToO: Oct-09; Nov-09

Primary Proposer(s):

Fisher -- cfischer [at] kis.uni-freiburg.de

Co-proposer(s):

Keller -- current email address needed
De Wijn -- dwijn [at] ucar.edu


HOP Productivity:

No productivity information provided.


REASON FOR LACK OF PRODUCTIVITY:

Unfortunately we were not able to observe the events we were looking for. This was perhaps due to the fact that the SP FOV and the two runs did not produce enough scans to capture this type of events. In addition we are looking for connected structures where one leg of the loop might be observed in the small FOV of the SP scan but we might be missing the other leg of the magnetic loop. We decided to obtain data from spectropolarimetric 2D-imagers to improve our statistics.