Solar Images Friday, 5 April 2024

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Photosphere sunspot drawing and RDS evaluation

05.04.2024 photosphere drawing

High-resolution scan (3229 px)

Time
07:20 UT
Observer
Ergün EGE
g
5
f
13
R
63
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=5.04.2024
Saat=07:20
Gözlemci=Ergün EGE
KontrolEden=Süleyman FİŞEK
Durumaçısı=-26.25
Enlemaçısı=-6.28
Boylamaçısı=51.9
Boylamfark=3
GKalite=3
GDurum=
Kuzeyaçısı=-0.6
Sırano=19951
AyRasatNo=4
RasatÖnceki=04.04.2024
RasatSonraki=06.04.2024

[Leke Grupları]
Grupsayısı=5:4:1
LekeSayısı=13:10:3
RölatifSayı=63:50:13
01=BXO 05 +05.287 +15.682 067.582 +0.000 0000 0 +06.258 +17.682 +04.316 +13.682 +05.287 +17.482 +05.287 +13.882
02=AX_ 02 +08.913 -02.285 049.615 +0.000 0000 0 +09.344 -01.447 +08.482 -03.123 +08.913 -01.947 +08.913 -02.623
03=AX_ 01 +07.460 -30.140 021.886 +0.000 0000 0 +07.949 -29.660 +06.970 -30.367 +07.460 -30.286 +07.460 -29.993
04=HS_ 02 +06.536 -51.487 000.413 +0.000 0000 0 +07.815 -49.959 +05.257 -53.150 +06.536 -50.391 +06.536 -52.583
05=AX_ 03 -11.404 +11.693 063.593 +0.000 0000 0 -10.817 +12.180 -11.992 +11.206 -11.404 +11.680 -11.404 +11.706
20240405.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 →

2024/20240405_ee · EE · 10 frames · 214.3 MB · 07:26:03–07:41:41 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.