Solar Images Thursday, 2 June 2022

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Photosphere sunspot drawing and RDS evaluation

02.06.2022 photosphere drawing

High-resolution scan (3230 px)

Time
06:45 UT
Observer
Süleyman FİŞEK
g
4
f
26
R
66
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=2.06.2022
Saat=06:45
Gözlemci=Süleyman FİŞEK
KontrolEden=Başar COŞKUNOĞLU
Durumaçısı=-14.97
Enlemaçısı=-0.55
Boylamaçısı=293.95
Boylamfark=3
GKalite=3
GDurum=G.T , H.S
Kuzeyaçısı=-1.0
Sırano=19450
AyRasatNo=2
RasatÖnceki=01.06.2022
RasatSonraki=03.06.2022

[Leke Grupları]
Grupsayısı=4:1:3
LekeSayısı=26:17:9
RölatifSayı=66:27:39
01=DSI 17 +16.429 +38.105 332.550 06.770 0000 0 +18.352 +42.753 +14.507 +33.457 +15.891 +41.561 +16.730 +34.474
02=DSO 02 -13.564 +29.480 323.430 +0.000 0000 0 -12.675 +30.992 -14.453 +27.967 -13.564 +30.792 -13.564 +28.167
03=HS_ 01 -33.407 +20.850 314.350 +0.000 0000 0 -32.638 +21.140 -34.175 +19.156 -33.407 +21.342 -33.407 +20.358
04=DSO 06 -16.128 -01.600 292.944 24.217 0000 0 -14.619 +01.433 -17.636 -03.445 -16.927 +00.600 -15.469 -02.645
20220602.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 →

2022/20220602_sf · SF · 8 frames · 171.4 MB · 07:05:21–07:16:45 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.