Solar Images Saturday, 18 June 2022
‹ 17.06.2022 2022 19.06.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 11:35 UT
- Observer
- Özgecan ÖNALTAŞ
- g
- 12
- f
- 77
- R
- 197
- Seeing
- 4 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=18.06.2022 Saat=11:35 Gözlemci=Özgecan ÖNALTAŞ KontrolEden=Ergün EGE Durumaçısı=-8.31 Enlemaçısı=1.4 Boylamaçısı=79.51 Boylamfark=0 GKalite=4 GDurum= Kuzeyaçısı=0.0 Sırano=19465 AyRasatNo=17 RasatÖnceki=17.06.2022 RasatSonraki=19.06.2022 [Leke Grupları] Grupsayısı=12:8:4 LekeSayısı=77:51:26 RölatifSayı=197:131:66 01=AX_ 02 +13.791 +57.746 137.256 +0.000 0000 0 +14.629 +58.169 +12.954 +57.323 +13.791 +57.669 +13.791 +57.823 02=AX_ 01 +14.400 +53.392 132.902 -1.000 0000 0 +14.400 +53.392 +14.400 +53.392 03=CAI 20 +18.563 +37.670 116.577 22.470 0000 0 +20.749 +39.233 +16.376 +34.900 +17.757 +38.636 +19.800 +35.546 04=HH_ 15 +19.551 +32.375 111.885 +0.000 0000 0 +21.159 +34.188 +17.942 +30.562 +19.551 +33.688 +19.551 +31.620 05=HS_ 01 +20.930 +24.217 103.727 +0.000 0000 0 +21.934 +25.226 +19.925 +23.208 +20.930 +24.726 +20.930 +23.708 06=AX_ 01 +16.858 +05.100 084.610 -1.000 0000 0 +16.858 +05.100 +16.858 +05.100 07=HS_ 01 +02.260 -08.709 070.801 +0.000 0000 0 +03.150 -07.789 +01.380 -09.628 +02.260 -08.289 +02.260 -09.128 08=CAI 10 +15.922 -29.540 049.970 +0.000 0000 0 +17.245 -24.554 +14.599 -34.527 +15.922 -24.754 +15.922 -34.327 09=BXI 07 -20.165 +58.412 137.922 +0.000 0000 0 -18.842 +62.433 -21.488 +54.390 -20.165 +62.233 -20.165 +54.590 10=CSO 03 -25.304 +48.684 128.194 +0.000 0000 0 -23.282 +50.984 -27.326 +46.384 -25.304 +50.784 -25.304 +46.584 11=AX_ 03 -28.465 +39.480 118.558 +0.000 0000 0 -27.513 +39.997 -29.418 +38.980 +00.000 +00.000 +00.000 +00.000 12=BXI 13 -16.602 -11.210 068.489 +0.000 0000 0 -15.770 -06.497 -18.128 -15.545 -16.602 -06.697 -16.602 -15.34520220618.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 →
2022/20220618_ööt · ÖÖT · 6 frames · 128.6 MB · 12:21:55–12:37:24 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.








