Solar Images Monday, 9 September 2024

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Photosphere sunspot drawing and RDS evaluation

09.09.2024 photosphere drawing

High-resolution scan (3224 px)

Time
06:50 UT
Observer
Burçin TANIK
g
11
f
68
R
178
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=9.09.2024
Saat=06:50
Gözlemci=Burçin TANIK
KontrolEden=Süleyman FİŞEK
Durumaçısı=23.03
Enlemaçısı=7.25
Boylamaçısı=136.14
Boylamfark=3
GKalite=3
GDurum=B.A
Kuzeyaçısı=0.4
Sırano=20087
AyRasatNo=8
RasatÖnceki=08.09.2024
RasatSonraki=10.09.2024

[Leke Grupları]
Grupsayısı=11:4:7
LekeSayısı=68:17:51
RölatifSayı=178:57:121
01=CRO 05 +13.927 +39.982 176.122 28.863 0000 0 +15.287 +42.485 +12.567 +37.479 +13.101 +41.434 +14.763 +38.416
02=CHI 08 +15.205 -22.780 113.360 30.121 0000 0 +17.206 -19.968 +13.204 -25.592 +14.780 -21.306 +15.917 -24.479
03=AX_ 02 +15.900 -27.229 108.911 +0.000 0000 0 +15.640 -26.929 +14.540 -27.529 +15.900 -27.429 +15.900 -27.290
04=BXO 02 +12.964 -33.550 103.850 +0.000 0000 0 +13.188 -31.436 +12.740 -34.675 +12.964 -32.431 +12.964 -34.669
05=AX_ 05 -13.720 +39.826 175.966 +0.000 0000 0 -12.913 +40.963 -14.527 +38.689 +00.000 +00.000 +00.000 +00.000
06=CKO 07 -10.770 +36.324 172.464 28.862 0000 0 -08.900 +39.718 -12.146 +32.930 -08.736 +38.872 -11.294 +34.223
07=AX_ 04 -17.312 +22.508 158.648 +0.000 0000 0 -16.764 +23.203 -17.861 +21.814 -17.312 +22.702 -17.312 +22.313
08=?__ 10 -22.134 +15.336 151.476 +0.000 0000 0 -18.685 +19.940 -25.582 +10.732 -22.134 +19.440 -22.134 +11.232
09=CSI 04 -10.280 +13.353 149.493 +0.000 0000 0 -08.726 +16.219 -11.331 +10.487 -10.280 +16.190 -10.280 +10.687
10=AX_ 06 -09.699 +08.267 144.407 +0.000 0000 0 -08.707 +09.619 -10.691 +06.916 +00.000 +00.000 +00.000 +00.000
11=CHO 15 -24.253 +00.370 136.177 19.950 0000 0 -20.791 +08.833 -27.716 -08.760 -21.976 +08.201 -27.132 -06.907
20240909.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 →

2024/20240909_bto · BTO · 4 frames · 85.7 MB · 07:00:46–07:23:39 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.