Solar Images Friday, 14 July 2023

‹ 13.07.2023 2023 15.07.2023 ›

Photosphere sunspot drawing and RDS evaluation

14.07.2023 photosphere drawing

High-resolution scan (3230 px)

Time
08:15 UT
Observer
Korhan YELKENCİ
g
11
f
82
R
192
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=14.07.2023
Saat=08:15
Gözlemci=Korhan YELKENCİ
KontrolEden=Hikmet ÇAKMAK
Durumaçısı=3.19
Enlemaçısı=4.21
Boylamaçısı=319.67
Boylamfark=2
GKalite=3
GDurum=K.T
Kuzeyaçısı=-0.6
Sırano=19762
AyRasatNo=13
RasatÖnceki=13.07.2023
RasatSonraki=15.07.2023

[Leke Grupları]
Grupsayısı=11:5:6
LekeSayısı=82:38:44
RölatifSayı=192:88:104
01=HS_ 01 +26.100 +79.328 038.998 +0.000 0000 0 +27.258 +80.888 +24.762 +77.769 +26.100 +80.388 +26.100 +78.269
02=EAI 17 +11.118 +57.590 016.729 15.900 0000 0 +13.245 +64.150 +08.992 +49.968 +12.970 +63.572 +09.192 +50.168
03=FAC 16 +23.669 -51.697 267.973 21.832 0000 0 +27.312 -42.319 +20.270 -61.760 +27.112 -42.519 +20.227 -60.590
04=HS_ 02 +06.971 -74.555 245.115 +0.000 0000 0 +08.335 -72.448 +05.607 -76.663 +06.971 -72.948 +06.971 -76.162
05=HS_ 02 +10.778 -84.165 235.505 +0.000 0000 0 +12.360 -80.182 +09.519 -88.149 +10.778 -80.682 +10.778 -87.648
06=AX_ 02 -07.284 +47.791 007.461 +0.000 0000 0 -07.730 +48.820 -07.495 +47.500 -07.284 +47.951 -07.284 +47.631
07=HK_ 33 -21.870 +22.720 341.742 +0.000 0000 0 -16.932 +26.487 -25.241 +17.656 -21.870 +26.635 -21.870 +18.804
08=AX_ 02 -14.144 -13.930 305.740 +0.000 0000 0 -13.798 -13.597 -14.491 -14.263 -14.144 -14.970 -14.144 -13.763
09=AX_ 03 -14.772 -30.389 289.281 +0.000 0000 0 -13.694 -29.297 -15.850 -31.481 +00.000 +00.000 +00.000 +00.000
10=AX_ 02 -20.606 -39.308 280.362 +0.000 0000 0 -20.118 -38.890 -21.940 -39.726 -20.606 -39.390 -20.606 -39.226
11=AX_ 02 -06.986 -79.967 239.703 +0.000 0000 0 -05.946 -79.121 -08.260 -80.812 +00.000 +00.000 +00.000 +00.000
20230714.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 →

2023/20230714_ky · KY · 14 frames · 299.9 MB · 08:54:17–09:00:47 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.