Solar Images Thursday, 1 August 2024

‹ 31.07.2024 2024 02.08.2024 ›

Photosphere sunspot drawing and RDS evaluation

01.08.2024 photosphere drawing

High-resolution scan (3230 px)

Time
11:10 UT
Observer
Süleyman FİŞEK
g
11
f
116
R
226
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=1.08.2024
Saat=11:10
Gözlemci=Süleyman FİŞEK
KontrolEden=Süleyman FİŞEK
Durumaçısı=11.16
Enlemaçısı=5.83
Boylamaçısı=289.15
Boylamfark=0
GKalite=3
GDurum=G.T , K.T
Kuzeyaçısı=-0.6
Sırano=20049
AyRasatNo=1
RasatÖnceki=31.07.2024
RasatSonraki=02.08.2024

[Leke Grupları]
Grupsayısı=11:5:6
LekeSayısı=116:22:94
RölatifSayı=226:72:154
01=HH_ 01 +05.202 +54.677 343.827 +0.000 0000 0 +06.304 +55.979 +04.100 +53.375 +05.202 +55.479 +05.202 +53.875
02=DHC 11 +08.531 +33.997 323.147 12.530 0000 0 +10.519 +38.534 +06.543 +29.460 +07.653 +36.642 +08.984 +30.397
03=HH_ 01 +22.309 -05.601 283.549 +0.000 0000 0 +23.622 -04.310 +20.996 -06.893 +22.309 -04.809 +22.309 -06.392
04=BXI 04 +09.980 -42.686 246.464 12.683 0000 0 +11.660 -39.293 +08.893 -46.790 +10.470 -39.883 +09.256 -45.285
05=CRI 05 +17.504 -53.357 235.793 10.132 0000 0 +18.410 -50.223 +16.598 -56.491 +17.167 -51.410 +17.927 -55.662
06=EHO 05 -15.940 +72.513 001.663 14.198 0000 0 -12.966 +79.366 -17.222 +65.660 -14.539 +74.497 -16.171 +68.290
07=BXO 02 -06.952 +65.300 354.153 +0.000 0000 0 -06.355 +66.875 -07.549 +63.131 -06.952 +66.672 -06.952 +63.928
08=FHC 58 -07.649 +37.353 326.503 08.440 0000 0 -01.707 +51.693 -13.590 +23.140 -06.570 +49.709 -08.623 +32.129
09=BXO 03 -18.287 +25.514 314.664 +0.000 0000 0 -17.659 +26.689 -18.915 +24.339 -18.287 +26.189 -18.287 +24.839
10=EHC 16 -23.103 -40.882 248.268 05.410 0000 0 -21.230 -34.359 -25.183 -47.405 -23.258 -35.623 -22.478 -43.891
11=DKC 10 -06.400 -63.569 225.581 10.499 0000 0 -03.371 -57.705 -08.709 -69.432 -06.474 -58.900 -04.885 -67.507
20240801.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 →

2024/20240801_sf · SF · 6 frames · 128.6 MB · 11:22:44–11:31:05 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.