Solar Images Thursday, 21 April 2022
‹ 20.04.2022 2022 23.04.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 07:40 UT
- Observer
- Süleyman FİŞEK
- g
- 4
- f
- 32
- R
- 72
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=21.04.2022 Saat=07:40 Gözlemci=Süleyman FİŞEK KontrolEden=Özgecan ÖNALTAŞ Durumaçısı=-25.5 Enlemaçısı=-5.11 Boylamaçısı=128.8 Boylamfark=2 GKalite=3 GDurum=G.T , B.A Kuzeyaçısı=-0.5 Sırano=19413 AyRasatNo=14 RasatÖnceki=20.04.2022 RasatSonraki=23.04.2022 [Leke Grupları] Grupsayısı=4:3:1 LekeSayısı=32:29:3 RölatifSayı=72:59:13 01=FKC 24 +17.472 -23.817 104.983 31.553 0000 0 +23.171 -14.333 +11.772 -33.302 +20.730 -16.964 +13.185 -29.421 02=HH_ 01 +12.881 -51.455 077.345 +0.000 0000 0 +14.132 -49.782 +11.629 -53.129 +12.881 -50.282 +12.881 -52.629 03=CRO 04 +19.136 -60.669 068.131 63.498 0000 0 +24.538 -56.498 +13.734 -64.840 +15.103 -58.270 +23.829 -62.660 04=CRO 03 -23.177 +10.220 139.200 +0.000 0000 0 -22.297 +11.210 -24.580 +09.230 +00.000 +00.000 +00.000 +00.00020220421.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 →
2022/20220422_sf · SF · 4 frames · 85.7 MB · 08:59:43–09:13:39 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.