Solar Images Saturday, 7 March 2026

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Photosphere sunspot drawing and RDS evaluation

07.03.2026 photosphere drawing

High-resolution scan (3230 px)

Time
07:00 UT
Observer
Süleyman FİŞEK
g
5
f
17
R
67
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=7.03.2026
Saat=07:00
Gözlemci=Süleyman FİŞEK
KontrolEden=Süleyman FİŞEK
Durumaçısı=-22.95
Enlemaçısı=-7.25
Boylamaçısı=159.33
Boylamfark=3
GKalite=3
GDurum=K.T
Kuzeyaçısı=-0.5
Sırano=20431
AyRasatNo=5
RasatÖnceki=06.03.2026
RasatSonraki=08.03.2026

[Leke Grupları]
Grupsayısı=5:4:1
LekeSayısı=17:16:1
RölatifSayı=67:56:11
01=HH_ 01 +18.896 +78.870 238.200 +0.000 0000 0 +19.924 +81.810 +17.867 +76.658 +18.896 +80.946 +18.896 +76.794
02=DHO 03 +15.728 +49.570 208.387 +0.000 0000 0 +17.730 +51.612 +13.725 +46.502 +15.728 +51.412 +15.728 +46.702
03=EHI 08 +08.910 +15.230 174.560 +0.000 0000 0 +09.915 +21.302 +06.268 +09.158 +08.910 +21.102 +08.910 +09.358
04=EHO 04 +09.740 -09.750 150.255 +0.000 0000 0 +10.536 -03.871 +07.611 -14.280 +09.740 -04.710 +09.740 -14.800
05=AX_ 01 -08.798 +01.482 160.812 +0.000 0000 0 -08.490 +01.827 -09.106 +01.137 -08.798 +01.327 -08.798 +01.637
20260307.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 →

2026/20260307_sf · SF · 6 frames · 128.6 MB · 07:16:00–07:18:59 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.