Solar Images Monday, 9 March 2026

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Photosphere sunspot drawing and RDS evaluation

09.03.2026 photosphere drawing

High-resolution scan (3229 px)

Time
07:50 UT
Observer
Burçin TANIK
g
5
f
15
R
65
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=9.03.2026
Saat=07:50
Gözlemci=Burçin TANIK
KontrolEden=İrem ÖZDEMİR
Durumaçısı=-23.37
Enlemaçısı=-7.24
Boylamaçısı=132.52
Boylamfark=2
GKalite=3
GDurum=G.T , K.T
Kuzeyaçısı=0.6
Sırano=20433
AyRasatNo=7
RasatÖnceki=08.03.2026
RasatSonraki=11.03.2026

[Leke Grupları]
Grupsayısı=5:5:0
LekeSayısı=15:15:0
RölatifSayı=65:65:0
01=HH_ 01 +17.345 +79.990 211.619 +0.000 0000 0 +18.842 +82.266 +15.849 +75.933 +17.345 +82.656 +17.345 +77.324
02=CKO 06 +08.681 +46.545 179.650 30.478 0000 0 +10.410 +49.282 +06.951 +43.808 +07.611 +48.230 +09.670 +44.729
03=AX_ 02 +12.419 +33.974 166.494 +0.000 0000 0 +12.745 +34.383 +12.930 +33.565 +12.419 +33.883 +12.419 +34.650
04=CHO 02 +08.889 +18.456 150.976 +0.000 0000 0 +10.150 +23.145 +07.628 +13.768 +08.889 +22.945 +08.889 +13.968
05=BXO 04 +08.843 -61.468 071.520 15.177 0000 0 +10.185 -57.576 +07.501 -65.360 +08.490 -58.651 +09.462 -63.870
20260309.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 →

2026/20260309_bto · BTO · 2 frames · 42.9 MB · 07:57:26–07:59:17 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.