Solar Images Monday, 30 May 2022
‹ 29.05.2022 2022 31.05.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 07:25 UT
- Observer
- Hikmet ÇAKMAK
- g
- 5
- f
- 12
- R
- 62
- Seeing
- 4 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=30.05.2022 Saat=07:25 Gözlemci=Hikmet ÇAKMAK KontrolEden=Talar YONTAN Durumaçısı=-16.07 Enlemaçısı=-0.9 Boylamaçısı=333.28 Boylamfark=3 GKalite=4 GDurum=G.T , H.S Kuzeyaçısı=-0.5 Sırano=19447 AyRasatNo=27 RasatÖnceki=29.05.2022 RasatSonraki=31.05.2022 [Leke Grupları] Grupsayısı=5:2:3 LekeSayısı=12:8:4 RölatifSayı=62:28:34 01=BXO 02 +21.884 +69.700 042.350 +0.000 0000 0 +22.260 +70.635 +21.507 +67.505 +21.884 +70.765 +21.884 +68.635 02=CAI 06 +28.940 +53.832 027.112 10.501 0000 0 +29.375 +57.820 +26.814 +49.844 +27.523 +56.881 +28.647 +50.805 03=AX_ 01 -06.181 +15.144 348.424 -1.000 0000 0 -06.181 +15.144 -06.181 +15.144 04=HA_ 02 -13.240 -09.284 323.996 +0.000 0000 0 -11.957 -08.220 -14.920 -10.546 -13.240 -08.621 -13.240 -09.947 05=HS_ 01 -32.566 -15.780 317.500 +0.000 0000 0 -31.859 -14.858 -33.273 -16.702 -32.566 -15.358 -32.566 -16.20220220530.gzd
Chromosphere (H-α) FITS frames
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 →
2022/20220530_hc · HC · 9 frames · 192.8 MB · 07:29:54–07:42:34 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.











