Solar Images Monday, 30 May 2022

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Photosphere sunspot drawing and RDS evaluation

30.05.2022 photosphere drawing

High-resolution scan (3231 px)

Time
07:25 UT
Observer
Hikmet ÇAKMAK
g
5
f
12
R
62
Seeing
4 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=30.05.2022
Saat=07:25
Gözlemci=Hikmet ÇAKMAK
KontrolEden=Talar YONTAN
Durumaçısı=-16.07
Enlemaçısı=-0.9
Boylamaçısı=333.28
Boylamfark=3
GKalite=4
GDurum=G.T , H.S
Kuzeyaçısı=-0.5
Sırano=19447
AyRasatNo=27
RasatÖnceki=29.05.2022
RasatSonraki=31.05.2022

[Leke Grupları]
Grupsayısı=5:2:3
LekeSayısı=12:8:4
RölatifSayı=62:28:34
01=BXO 02 +21.884 +69.700 042.350 +0.000 0000 0 +22.260 +70.635 +21.507 +67.505 +21.884 +70.765 +21.884 +68.635
02=CAI 06 +28.940 +53.832 027.112 10.501 0000 0 +29.375 +57.820 +26.814 +49.844 +27.523 +56.881 +28.647 +50.805
03=AX_ 01 -06.181 +15.144 348.424 -1.000 0000 0 -06.181 +15.144 -06.181 +15.144
04=HA_ 02 -13.240 -09.284 323.996 +0.000 0000 0 -11.957 -08.220 -14.920 -10.546 -13.240 -08.621 -13.240 -09.947
05=HS_ 01 -32.566 -15.780 317.500 +0.000 0000 0 -31.859 -14.858 -33.273 -16.702 -32.566 -15.358 -32.566 -16.202
20220530.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 →

2022/20220530_hc · HC · 9 frames · 192.8 MB · 07:29:54–07:42:34 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.