Solar Images Tuesday, 13 August 2024

‹ 12.08.2024 2024 14.08.2024 ›

Photosphere sunspot drawing and RDS evaluation

13.08.2024 photosphere drawing

High-resolution scan (3230 px)

Time
08:10 UT
Observer
Korhan YELKENCİ
g
11
f
101
R
211
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=13.08.2024
Saat=08:10
Gözlemci=Korhan YELKENCİ
KontrolEden=Süleyman FİŞEK
Durumaçısı=15.56
Enlemaçısı=6.57
Boylamaçısı=132.14
Boylamfark=2
GKalite=3
GDurum=K.T
Kuzeyaçısı=-0.2
Sırano=20061
AyRasatNo=13
RasatÖnceki=12.08.2024
RasatSonraki=14.08.2024

[Leke Grupları]
Grupsayısı=11:5:6
LekeSayısı=101:36:65
RölatifSayı=211:86:125
01=AX_ 01 +11.612 +43.408 175.548 +0.000 0000 0 +11.993 +43.967 +11.230 +42.849 +11.612 +43.467 +11.612 +43.349
02=BXI 02 +15.366 +33.150 165.155 21.386 0000 0 +16.486 +35.588 +14.246 +30.442 +16.286 +35.388 +14.446 +30.681
03=BXI 02 +18.280 +18.630 150.203 31.232 0000 0 +19.564 +20.469 +16.493 +15.656 +19.364 +20.269 +16.693 +15.856
04=CAI 05 +03.619 +05.160 137.300 26.932 0000 0 +04.906 +07.440 +02.333 +02.881 +04.643 +07.240 +02.533 +03.810
05=DKC 26 +14.369 -17.337 114.803 40.976 0000 0 +17.889 -13.353 +10.849 -21.320 +17.716 -13.390 +11.133 -21.257
06=DAI 03 -09.675 +73.530 205.193 15.677 0000 0 -08.204 +78.117 -11.145 +67.990 -08.404 +77.773 -10.945 +68.677
07=FKC 28 -08.801 +37.841 169.981 17.634 0000 0 -04.979 +50.740 -12.624 +25.608 -05.138 +49.535 -12.839 +25.497
08=DAI 09 -21.755 +16.214 148.354 13.427 0000 0 -20.504 +20.850 -23.600 +11.578 -20.704 +20.623 -22.806 +11.778
09=AX_ 02 -09.880 +01.600 133.146 +0.000 0000 0 -08.183 +02.224 -09.994 -00.211 +00.000 +00.000 +00.000 +00.000
10=BXI 07 -08.676 -29.241 102.899 52.850 0000 0 -06.353 -27.414 -11.000 -31.680 -06.633 -27.614 -10.800 -30.868
11=DAI 16 -06.690 -44.926 087.214 16.258 0000 0 -05.393 -40.895 -07.987 -48.957 -05.593 -41.209 -07.787 -48.757
20240813.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 →

2024/20240813_ky · KY · 14 frames · 299.9 MB · 08:37:15–08:43:48 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.