Solar Images Thursday, 23 June 2022
‹ 22.06.2022 2022 24.06.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 07:40 UT
- Observer
- Ö.ÖNALTAŞ=B.T.
- g
- 4
- f
- 39
- R
- 79
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=23.06.2022 Saat=07:40 Gözlemci=Ö.ÖNALTAŞ=B.T. KontrolEden=Olcay PLEVNE Durumaçısı=-6.18 Enlemaçısı=1.97 Boylamaçısı=15.49 Boylamfark=2 GKalite=3 GDurum=G.T , H.S Kuzeyaçısı=0.0 Sırano=19470 AyRasatNo=22 RasatÖnceki=22.06.2022 RasatSonraki=24.06.2022 [Leke Grupları] Grupsayısı=4:2:2 LekeSayısı=39:31:8 RölatifSayı=79:51:28 01=HS_ 01 +01.101 +55.141 070.631 +0.000 0000 0 +01.860 +56.360 +00.341 +54.245 +01.101 +55.698 +01.101 +54.583 02=EKC 30 +15.136 +36.718 052.208 10.409 0000 0 +17.395 +43.323 +12.877 +30.113 +15.981 +41.337 +14.240 +31.816 03=CSI 03 -17.549 +55.650 071.140 +0.000 0000 0 -16.557 +56.789 -18.540 +54.511 +00.000 +00.000 +00.000 +00.000 04=DSC 05 -11.991 -52.709 322.781 16.580 0000 0 -10.250 -49.160 -13.732 -56.259 -11.304 -50.331 -12.669 -54.92120220623.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 →
2022/20220623_oot · OOT · 13 frames · 278.6 MB · 07:56:45–09:08:52 UT
08:43:58 UT · 30 ms
08:59:33 UT · 30 ms
07:59:08 UT · 30 ms
09:07:41 UT · 30 ms
08:32:32 UT · 30 ms
09:08:52 UT · 60 ms · over-exposed
08:14:06 UT · 30 ms
07:56:45 UT · 40 ms
08:35:28 UT · 60 ms · over-exposed
08:01:13 UT · 60 ms · over-exposed
08:11:44 UT · 60 ms · over-exposed
08:45:45 UT · 60 ms · over-exposed
08:58:43 UT · 60 ms · over-exposed
Coronado H-α animations from frame sequences
No Coronado observation for this day.


