Solar Images Tuesday, 10 May 2022

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Photosphere sunspot drawing and RDS evaluation

10.05.2022 photosphere drawing

High-resolution scan (3231 px)

Time
07:35 UT
Observer
Süleyman FİŞEK
g
3
f
45
R
75
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=10.05.2022
Saat=07:35
Gözlemci=Süleyman FİŞEK
KontrolEden=Burçin TANIK
Durumaçısı=-22.18
Enlemaçısı=-3.22
Boylamaçısı=237.75
Boylamfark=2
GKalite=3
GDurum=G.T
Kuzeyaçısı=-0.6
Sırano=19428
AyRasatNo=8
RasatÖnceki=09.05.2022
RasatSonraki=11.05.2022

[Leke Grupları]
Grupsayısı=3:0:3
LekeSayısı=45:0:45
RölatifSayı=75:0:75
01=CAI 29 -30.539 -02.108 235.642 28.153 0000 0 -26.210 +04.691 -34.867 -08.906 -28.510 +03.599 -34.114 -07.851
02=HS_ 01 -23.541 -47.749 190.100 +0.000 0000 0 -22.627 -46.553 -24.456 -48.946 -23.541 -47.530 -23.541 -48.445
03=CRI 15 -23.237 -57.845 179.905 24.531 0000 0 -20.121 -53.300 -26.353 -62.661 -22.336 -54.510 -25.581 -61.646
20220510.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 →

2022/20220510_sf · SF · 16 frames · 342.8 MB · 08:01:30–08:17:22 UT

2022/20220512_sf · SF · 9 frames · 192.8 MB · 08:11:59–08:16:27 UT

2022/20220520_sf · SF · 9 frames · 192.8 MB · 08:11:59–08:16:27 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.