Solar Images Monday, 10 October 2022

‹ 09.10.2022 2022 11.10.2022 ›

Photosphere sunspot drawing and RDS evaluation

10.10.2022 photosphere drawing

High-resolution scan (3229 px)

Time
10:41 UT
Observer
Ergün EGE
g
4
f
34
R
74
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=10.10.2022
Saat=10:41
Gözlemci=Ergün EGE
KontrolEden=Talar YONTAN
Durumaçısı=26.26
Enlemaçısı=6.21
Boylamaçısı=13.19
Boylamfark=1
GKalite=3
GDurum=
Kuzeyaçısı=-0.4
Sırano=19571
AyRasatNo=6
RasatÖnceki=09.10.2022
RasatSonraki=11.10.2022

[Leke Grupları]
Grupsayısı=4:4:0
LekeSayısı=34:34:0
RölatifSayı=74:74:0
01=FSC 14 +22.352 +31.795 044.985 +0.000 0000 0 +25.738 +43.510 +18.966 +20.540 +22.352 +42.851 +22.352 +20.740
02=CSI 05 +30.604 +28.310 041.221 +0.000 0000 0 +33.660 +34.130 +28.141 +22.490 +30.604 +33.813 +30.604 +22.249
03=ESI 12 +28.726 -05.424 007.766 +0.000 0000 0 +31.171 +00.867 +26.282 -11.715 +28.726 +00.667 +28.726 -11.515
04=AX_ 03 +09.508 -17.639 355.551 +0.000 0000 0 +11.160 -16.549 +08.000 -18.729 +00.000 +00.000 +00.000 +00.000
20221010.gzd

Chromosphere (H-α) FITS frames

H-α

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 →

2022/20221010_ee · EE · 7 frames · 150.0 MB · 08:27:28–08:35:07 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.