SUMER study #2118: Fe II raster scan in coronal hole
- date, time: 23.Oct.99, 00:01 - 04:03 UT
- field of view: 24 - 186 arcsec W, 274 - 394 arcsec N
- slit: 1.0 arcsec x 120 arcsec, centered (number 4)
- raster step size: 1.12 arcsec (3 elementary steps)
- exposure time: 100 seconds
- telemetry: 145 images of 1024 spectral x 120 spatial pixels (format 4)
- compression: quasilog-min-max (method 5)
- wavelength: 1563.00 Å on reference pixel 101 of Detector A
- rotation compensation: after complete scan, corresponding to 0.75 arcsec
after 313.670 seconds
- binning: no spectral, no spatial
- on-board flat field correction: no
Spectral window
Detailed spectral windows
N IV
Fe II
line = *, continuum = +
N IV 1530.31/2 (141 000 K)
continuum and line intensity, line shift and width
Fe II 1563.79 (12 000 K)
continuum and line intensity, line shift and width
IED, 03.May.00