Solar Images Monday, 3 June 2024
‹ 02.06.2024 2024 04.06.2024 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 09:50 UT
- Observer
- Korhan YELKENCİ
- g
- 12
- f
- 136
- R
- 256
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=3.06.2024 Saat=09:50 Gözlemci=Korhan YELKENCİ KontrolEden=Olcay PLEVNE Durumaçısı=-14.34 Enlemaçısı=-0.35 Boylamaçısı=350.65 Boylamfark=1 GKalite=3 GDurum=H.S Kuzeyaçısı=-0.6 Sırano=19994 AyRasatNo=2 RasatÖnceki=02.06.2024 RasatSonraki=04.06.2024 [Leke Grupları] Grupsayısı=12:7:5 LekeSayısı=136:57:79 RölatifSayı=256:127:129 01=DAI 07 +24.822 +47.772 038.422 13.858 0000 0 +26.205 +52.563 +23.439 +42.981 +25.893 +52.363 +23.639 +43.181 02=CAI 10 +03.957 +36.347 026.997 21.725 0000 0 +05.580 +40.129 +02.335 +32.564 +05.380 +39.929 +02.535 +32.764 03=BXI 03 +18.183 +35.530 026.180 38.480 0000 0 +19.352 +37.213 +17.150 +33.847 +19.152 +36.906 +17.215 +34.468 04=CAI 08 +22.313 +33.322 023.972 22.229 0000 0 +23.524 +35.992 +21.101 +30.651 +23.206 +35.517 +21.301 +30.851 05=BXI 07 +28.179 +30.436 021.860 43.333 0000 0 +30.197 +32.446 +26.160 +28.427 +29.642 +32.112 +26.360 +28.627 06=DAC 21 +22.500 +04.985 355.635 15.804 0000 0 +23.679 +10.726 +20.331 -00.756 +23.745 +10.857 +20.248 -00.925 07=HS_ 01 +16.500 -65.199 285.451 +0.000 0000 0 +17.651 -64.320 +15.349 -66.365 +16.500 -64.676 +16.500 -65.721 08=DSO 11 -04.197 +53.619 044.269 18.985 0000 0 -02.400 +58.488 -05.995 +48.749 -02.600 +58.288 -05.795 +48.949 09=FKC 40 -18.414 -03.416 347.234 21.133 0000 0 -14.927 +05.422 -21.900 -12.253 -15.127 +05.222 -21.675 -12.530 10=DAI 13 -05.430 -13.349 337.301 25.222 0000 0 -03.341 -10.225 -06.745 -16.472 -03.866 -10.572 -06.545 -16.272 11=BXI 14 -07.548 -28.352 322.298 30.532 0000 0 -06.205 -26.252 -08.891 -30.453 -06.461 -26.452 -08.691 -30.239 12=AX_ 01 -17.650 -71.900 279.641 -1.000 0000 0 -17.650 -71.900 -17.650 -71.90020240603.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 →
2024/20240603_ky · KY · 14 frames · 299.9 MB · 10:08:44–10:15:14 UT
10:13:14 UT · 30 ms
10:09:44 UT · 30 ms
10:12:44 UT · 76 ms · over-exposed
10:09:14 UT · 76 ms · over-exposed
10:12:14 UT · 70 ms · over-exposed
10:08:44 UT · 70 ms · over-exposed
10:15:14 UT
10:14:44 UT · 70 ms
10:13:44 UT · 60 ms
10:14:14 UT · 30 ms
10:11:44 UT
10:11:14 UT · 70 ms
10:10:14 UT · 60 ms
10:10:44 UT · 30 ms
Coronado H-α animations from frame sequences
No Coronado observation for this day.


