SUMER study #664: Sunspot localization
- date, time: 30.Aug.96, 08:12 - 08:49 UT
- field of view: 29 - 149 arcsec W, 360 - 240 arcsec S
- slit: 1.0 arcsec x 120 arcsec, bottom (number 5)
- raster step size: 1.13 arcsec (3 elementary steps, "Schmierschritt")
- exposure time: 10.0 seconds
- telemetry: 2(scans)*2(lines)*106 images of 50 spectral x 120 spatial pixels
(format 10)
- compression: quasilog-min-max (method 5)
- wavelengths: 944.520 Å on reference pixel 334 of Detector A
937.803 Å on reference pixel 484 of Detector A
- rotation compensation: 0.75 arcsec after 298.650 seconds
- binning: no spectral, no spatial
- on-board flat field correction: no
Remark: The field of view was scanned twice, in alternating direction.
Image taken before EUV scans by the Rear Slit Camera; time: 08:08 UT, field
of view: 88" - 427" W, 360" - 240" S
Spectral windows
H I Ly e
Average detector image, average profile.
S VI
Average detector image, average profile.
Si VIII
Average detector image, average profile.
H I Ly e 937.80 (~10 000 K)
Line intensity, line shift, line width.
S VI 944.55 (200 000 K)
Line intensity, line shift, line width.
Si VIII 944.34 (850 000 K)
Line intensity.
RSC and EUV images (overlapping parts) on same scale
IED, 09.Jan.03