Solar Images Monday, 16 January 2023

‹ 15.01.2023 2023 18.01.2023 ›

Photosphere sunspot drawing and RDS evaluation

16.01.2023 photosphere drawing

High-resolution scan (3234 px)

Time
10:25 UT
Observer
Hikmet ÇAKMAK
g
12
f
89
R
209
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=16.01.2023
Saat=10:25
Gözlemci=Hikmet ÇAKMAK
KontrolEden=Olcay PLEVNE
Durumaçısı=-5.19
Enlemaçısı=-4.65
Boylamaçısı=161.74
Boylamfark=1
GKalite=3
GDurum=G.T , H.S
Kuzeyaçısı=-0.3
Sırano=19639
AyRasatNo=10
RasatÖnceki=15.01.2023
RasatSonraki=18.01.2023

[Leke Grupları]
Grupsayısı=12:5:7
LekeSayısı=89:43:46
RölatifSayı=209:93:116
01=EKI 14 +24.112 +06.125 167.865 11.409 0000 0 +26.876 +12.820 +21.347 +00.168 +23.830 +10.839 +25.630 +00.974
02=BXO 04 +20.450 -26.764 134.976 +0.000 0000 0 +20.932 -24.996 +19.967 -28.531 +20.450 -25.497 +20.450 -28.310
03=DAC 12 +10.444 -33.755 127.985 09.463 0000 0 +12.491 -29.232 +08.398 -38.278 +11.152 -30.430 +09.992 -37.405
04=AX_ 01 +10.102 -43.786 117.954 -1.000 0000 0 +10.102 -43.786 +10.102 -43.786
05=CAI 12 +18.302 -48.813 112.927 10.441 0000 0 +21.299 -39.282 +15.306 -58.344 +17.202 -42.300 +19.617 -55.528
06=CAO 03 -15.334 +65.480 227.220 23.272 0000 0 -13.428 +69.722 -17.239 +61.237 -14.113 +67.976 -16.729 +61.878
07=AX_ 01 -23.616 +46.899 208.639 -1.000 0000 0 -23.616 +46.899 -23.616 +46.899
08=CAI 05 -21.959 +34.883 196.623 13.901 0000 0 -20.811 +37.390 -23.107 +32.727 -21.546 +36.168 -22.306 +33.950
09=CAI 08 -12.903 +13.354 175.940 07.306 0000 0 -11.620 +21.162 -14.744 +05.547 -13.272 +18.173 -11.846 +06.976
10=BXI 09 -24.174 -17.211 144.529 09.248 0000 0 -22.851 -14.261 -25.497 -20.160 -24.434 -15.680 -23.646 -19.911
11=BXI 06 -22.782 -33.750 128.665 10.695 0000 0 -21.765 -30.230 -23.800 -35.920 -23.278 -30.817 -22.411 -35.414
12=EKI 14 -14.439 -45.247 116.493 06.515 0000 0 -11.907 -37.627 -16.971 -52.868 -14.306 -40.458 -15.624 -52.800
20230116.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 →

2023/20230116_hc · HC · 4 frames · 85.7 MB · 10:25:51–10:42:12 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.