Solar Images Sunday, 30 January 2022

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Photosphere sunspot drawing and RDS evaluation

30.01.2022 photosphere drawing

High-resolution scan (3235 px)

Time
08:30 UT
Observer
Burçin TANIK
g
5
f
40
R
90
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=30.01.2022
Saat=08:30
Gözlemci=Burçin TANIK
KontrolEden=Burçin TANIK
Durumaçısı=-11.46
Enlemaçısı=-5.89
Boylamaçısı=116.03
Boylamfark=2
GKalite=3
GDurum=G.T , K.T
Kuzeyaçısı=-0.7
Sırano=19365
AyRasatNo=15
RasatÖnceki=29.01.2022
RasatSonraki=31.01.2022

[Leke Grupları]
Grupsayısı=5:3:2
LekeSayısı=40:38:2
RölatifSayı=90:68:22
01=BXO 03 +32.309 +44.740 160.770 +0.000 0000 0 +33.592 +47.712 +31.250 +41.769 +32.309 +47.512 +32.309 +41.969
02=FHC 30 +16.339 -02.269 113.761 15.463 0000 0 +19.500 +03.885 +13.674 -08.423 +17.364 +03.225 +14.230 -08.191
03=AX_ 05 +17.129 -24.691 091.339 +0.000 0000 0 +18.230 -23.261 +16.234 -26.122 +00.000 +00.000 +00.000 +00.000
04=HS_ 01 -25.179 +51.733 167.763 -1.000 0000 0 -24.151 +52.904 -26.207 +50.563
05=?__ 01 -14.741 -85.779 030.251 -1.000 0000 0 -13.458 -82.207 -16.240 -89.352
20220130.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 →

2022/20220130_bto · BTO · 6 frames · 128.6 MB · 08:40:59–08:55:21 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.