Solar Images Monday, 31 January 2022

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Photosphere sunspot drawing and RDS evaluation

31.01.2022 photosphere drawing

High-resolution scan (3238 px)

Time
08:00 UT
Observer
Burçin TANIK
g
5
f
29
R
79
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=31.01.2022
Saat=08:00
Gözlemci=Burçin TANIK
KontrolEden=Talar YONTAN
Durumaçısı=-11.86
Enlemaçısı=-5.96
Boylamaçısı=103.13
Boylamfark=2
GKalite=3
GDurum=G.T , K.T
Kuzeyaçısı=-1.0
Sırano=19366
AyRasatNo=16
RasatÖnceki=30.01.2022
RasatSonraki=01.02.2022

[Leke Grupları]
Grupsayısı=5:3:2
LekeSayısı=29:23:6
RölatifSayı=79:53:26
01=DHI 14 +17.178 +10.768 113.898 16.475 0000 0 +19.312 +16.792 +15.430 +04.745 +15.872 +16.195 +18.905 +05.875
02=BXI 03 +16.549 -09.517 093.613 +0.000 0000 0 +17.623 -07.870 +15.475 -11.164 +16.549 -08.700 +16.549 -10.964
03=CRI 06 +16.341 -71.306 031.824 23.742 0000 0 +18.800 -67.316 +14.675 -75.296 +17.808 -67.516 +15.258 -73.328
04=HS_ 01 -24.923 +64.268 167.398 +0.000 0000 0 -23.960 +65.130 -25.886 +63.407 -24.923 +64.630 -24.923 +63.906
05=CRI 05 -16.640 -75.485 027.645 15.709 0000 0 -14.150 -68.783 -18.112 -82.187 -14.358 -69.110 -17.525 -80.454
20220131.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 →

2022/20220131_bto · BTO · 1 frames · 21.4 MB · 08:14:04 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.