Coronal hole plume observation, 17-Nov-2015
I arranged this joint observation with IRIS when I was EIS CO. XRT was doing a bakeout and SOT did not support.
The plume lay in a narrow, diagonal lane but is quite bright.
The as-run observation was:
The pointing was a little to the left of the plume's core, so
brightest emission is missed by cool_loop_stare. The base is caught
nicelywith the rasters though.
Although cool_loop_stare was scheduled for 3 runs, there are actually four files. However there's a big data drop-out from raster 2 to raster 3 so I the think two files should be put back together into a single file, i.e., there's not actually any data missing.
Hans Courier was the IRIS planner, and the observation was performed in 4 groups of rasters due to the eclipse season:
The 16-step raster given in the HOP 266 description was used.
There was no SOT support for this observation.
Page maintained by Dr Peter Young.