Solar Images Thursday, 4 March 2021
‹ 03.03.2021 2021 05.03.2021 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 08:50 UT
- Observer
- Talar YONTAN
- g
- 2
- f
- 17
- R
- 37
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=4.03.2021 Saat=08:50 Gözlemci=Talar YONTAN KontrolEden=Başar COŞKUNOĞLU Durumaçısı=-22.36 Enlemaçısı=-7.25 Boylamaçısı=178.84 Boylamfark=2 GKalite=3 GDurum=G.T , K.T Kuzeyaçısı=0.0 Sırano=19137 AyRasatNo=4 RasatÖnceki=03.03.2021 RasatSonraki=5.03.2021 [Leke Grupları] Grupsayısı=2:0:2 LekeSayısı=17:0:17 RölatifSayı=37:0:37 01=DRO 07 -31.314 +16.929 195.769 00.208 0000 0 -30.473 +19.982 -32.155 +13.875 -31.333 +19.213 -31.314 +14.750 02=DAO 10 -18.774 -25.887 152.953 04.959 0000 0 -17.614 -22.814 -19.934 -28.960 -19.229 -23.509 -18.774 -28.76020210304.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 →
2021/20210304_ty · TY · 16 frames · 342.8 MB · 09:06:08–09:44:07 UT
09:18:04 UT · 40 ms
09:38:49 UT · 40 ms
09:34:11 UT · 40 ms
09:06:08 UT · 40 ms
09:26:44 UT · 40 ms
09:08:41 UT · 60 ms · over-exposed
09:16:58 UT · 65 ms · over-exposed
09:25:09 UT · 65 ms · over-exposed
09:38:03 UT · 70 ms · over-exposed
09:33:09 UT · 70 ms · over-exposed
09:43:19 UT · 70 ms
09:40:42 UT · 70 ms
09:44:07 UT · 65 ms
09:41:38 UT · 65 ms
09:42:28 UT · 40 ms
09:39:45 UT · 40 ms
Coronado H-α animations from frame sequences
No Coronado observation for this day.