Solar Images Monday, 6 June 2022
‹ 05.06.2022 2022 08.06.2022 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 07:40 UT
- Observer
- Ergün EGE
- g
- 3
- f
- 4
- R
- 34
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=6.06.2022 Saat=07:40 Gözlemci=Ergün EGE KontrolEden=Özgecan ÖNALTAŞ Durumaçısı=-13.4 Enlemaçısı=-0.06 Boylamaçısı=240.51 Boylamfark=2 GKalite=3 GDurum=B.A , Y.B Kuzeyaçısı=-0.6 Sırano=19454 AyRasatNo=6 RasatÖnceki=05.06.2022 RasatSonraki=08.06.2022 [Leke Grupları] Grupsayısı=3:0:3 LekeSayısı=4:0:4 RölatifSayı=34:0:34 01=AX_ 01 -34.868 +71.270 311.780 +0.000 0000 0 -34.610 +72.130 -35.126 +70.409 -34.868 +71.630 -34.868 +70.910 02=BXO 02 -16.764 +53.999 294.509 +0.000 0000 0 -15.792 +55.952 -17.736 +52.460 -16.764 +55.752 -16.764 +52.246 03=AX_ 01 -17.601 -42.842 197.668 +0.000 0000 0 -17.277 -42.343 -17.926 -43.341 -17.601 -42.843 -17.601 -42.84120220606.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 →
2022/20220606_ee · EE · 6 frames · 128.6 MB · 07:43:10–07:48:18 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.