Solar Images Saturday, 29 October 2022

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Photosphere sunspot drawing and RDS evaluation

29.10.2022 photosphere drawing

High-resolution scan (3231 px)

Time
10:00 UT
Observer
Ergün EGE
g
4
f
20
R
60
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=29.10.2022
Saat=10:00
Gözlemci=Ergün EGE
KontrolEden=Ergün EGE
Durumaçısı=24.89
Enlemaçısı=4.66
Boylamaçısı=122.8
Boylamfark=1
GKalite=3
GDurum=B.A
Kuzeyaçısı=-0.5
Sırano=19587
AyRasatNo=22
RasatÖnceki=28.10.2022
RasatSonraki=30.10.2022

[Leke Grupları]
Grupsayısı=4:3:1
LekeSayısı=20:17:3
RölatifSayı=60:47:13
01=CSI 03 +23.701 -13.429 109.371 +0.000 0000 0 +26.750 -08.914 +21.327 -17.944 +23.701 -09.114 +23.701 -17.744
02=BXI 10 +26.118 -29.153 093.647 +0.000 0000 0 +27.815 -24.804 +24.420 -33.503 +26.118 -25.400 +26.118 -33.303
03=DRI 04 +27.263 -60.900 062.710 +0.000 0000 0 +28.478 -55.311 +26.470 -64.869 +27.263 -55.511 +27.263 -64.669
04=CRI 03 -23.352 +60.930 183.730 +0.000 0000 0 -22.565 +64.266 -24.138 +57.594 -23.352 +63.766 -23.352 +58.940
20221029.gzd

Chromosphere (H-α) FITS frames

H-α

The images are made automatically with a fixed, gentle rule: uneven illumination and most of the limb darkening are removed, and the brightness is shown on a linear scale (no sharpening); prominences get their own scale outside the limb. Frames are ordered by sharpness (seeing); frames without the Sun (darks, bias) come last. Method →

2022/20221029_ee · EE · 8 frames · 171.4 MB · 10:11:41–10:28:29 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.