SUMER study #1848: Coronal hole scan around 1542 Å
Overview
- date, time: 07.Mar.99, 11:35 - 15:35 UT
- field of view: 54 arcsec E - 54 arcsec W, 1030 - 730 arcsec S
- slit: 1.0 arcsec x 300 arcsec (number 2)
- raster step size: 1.13 arcsec (3 elementary steps)
- exposure time: 150 seconds
- telemetry: 97 images of 512 spectral x 360 spatial pixels (format 38)
- compression: quasilog-min-max (method 5)
- wavelength: 1542.00 Å on reference pixel 510 of Detector A
- rotation compensation: after complete scan, corresponding to
0.75 arcsec after 648.981 seconds
- binning: no spectral, no spatial
- on-board flat field correction: no
Remarks: The scan was performed in west-east direction. Therefore, considering
the Solar rotation, it covers more space (125 arcsec) than the nominal pointing
indicates.
Spectral window
Field of view (EIT image of 19:19 UT)
line = *, continuum = +
Ne VIII 770.4 (630 000 K)
continuum and line intensity, line shift and width
line = *, continuum = +
C IV 1548.2 (100 000 K)
continuum and line intensity, line shift and width
line = *, continuum = +
Si II 1533.4 (14 000 K)
continuum and line intensity, line shift and width
IED, 29.Oct.99