Solar Images Thursday, 29 August 2024

‹ 28.08.2024 2024 30.08.2024 ›

Photosphere sunspot drawing and RDS evaluation

29.08.2024 photosphere drawing

High-resolution scan (3228 px)

Time
06:30 UT
Observer
Burçin TANIK
g
11
f
48
R
158
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=29.08.2024
Saat=06:30
Gözlemci=Burçin TANIK
KontrolEden=Süleyman FİŞEK
Durumaçısı=20.44
Enlemaçısı=7.15
Boylamaçısı=281.61
Boylamfark=3
GKalite=3
GDurum=
Kuzeyaçısı=-0.8
Sırano=20077
AyRasatNo=29
RasatÖnceki=28.08.2024
RasatSonraki=30.08.2024

[Leke Grupları]
Grupsayısı=11:6:5
LekeSayısı=48:22:26
RölatifSayı=158:82:76
01=HR_ 01 +06.567 +48.909 330.519 +0.000 0000 0 +07.115 +49.747 +06.190 +48.710 +06.567 +48.928 +06.567 +48.890
02=DSI 04 +07.628 +18.280 299.890 22.996 0000 0 +08.890 +20.319 +06.367 +16.240 +06.865 +19.697 +08.830 +16.826
03=AX_ 02 +07.499 +09.255 290.865 +0.000 0000 0 +07.759 +09.896 +07.240 +08.614 +07.499 +09.396 +07.499 +09.114
04=AX_ 01 +20.591 -40.262 241.348 -1.000 0000 0 +20.591 -40.262 +20.591 -40.262
05=CAI 12 +13.329 -40.424 241.186 32.610 0000 0 +15.217 -37.716 +11.440 -43.133 +14.325 -38.957 +12.284 -42.150
06=BXO 02 +23.253 -55.320 226.578 +0.000 0000 0 +24.100 -53.362 +22.496 -56.701 +23.253 -54.151 +23.253 -56.489
07=BXO 03 -03.160 +72.681 354.291 +0.000 0000 0 -01.671 +77.956 -04.650 +67.406 -03.160 +77.756 -03.160 +67.606
08=FHI 14 -27.346 +49.626 331.236 08.600 0000 0 -25.310 +57.879 -29.661 +41.374 -26.480 +55.951 -28.378 +43.296
09=HK_ 03 -10.710 +36.553 318.163 +0.000 0000 0 -08.865 +38.769 -12.555 +34.336 -10.710 +38.270 -10.710 +34.837
10=HS_ 01 -24.602 -33.690 247.920 +0.000 0000 0 -23.551 -32.569 -25.654 -34.812 -24.602 -33.680 -24.602 -34.312
11=?__ 05 -10.395 -66.783 214.827 +0.000 0000 0 -08.367 -62.843 -12.424 -70.723 -10.395 -63.343 -10.395 -70.223
20240829.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 →

2024/20240829_bto · BTO · 5 frames · 107.1 MB · 06:36:22–06:40:17 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.