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

HOP INSTRUCTION PAGE



HOP Proposer:    De Wijn

dwijn [at] ucar.edu


As Primary Proposer:



* As Co-Proposer:

* HOP 41:

No HOP productivity information provided.

* HOP 138:

No HOP productivity information provided.

* HOP 141:

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.