Solar Images Saturday, 18 June 2022

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Photosphere sunspot drawing and RDS evaluation

18.06.2022 photosphere drawing

High-resolution scan (3226 px)

Time
11:35 UT
Observer
Özgecan ÖNALTAŞ
g
12
f
77
R
197
Seeing
4 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=18.06.2022
Saat=11:35
Gözlemci=Özgecan ÖNALTAŞ
KontrolEden=Ergün EGE
Durumaçısı=-8.31
Enlemaçısı=1.4
Boylamaçısı=79.51
Boylamfark=0
GKalite=4
GDurum=
Kuzeyaçısı=0.0
Sırano=19465
AyRasatNo=17
RasatÖnceki=17.06.2022
RasatSonraki=19.06.2022

[Leke Grupları]
Grupsayısı=12:8:4
LekeSayısı=77:51:26
RölatifSayı=197:131:66
01=AX_ 02 +13.791 +57.746 137.256 +0.000 0000 0 +14.629 +58.169 +12.954 +57.323 +13.791 +57.669 +13.791 +57.823
02=AX_ 01 +14.400 +53.392 132.902 -1.000 0000 0 +14.400 +53.392 +14.400 +53.392
03=CAI 20 +18.563 +37.670 116.577 22.470 0000 0 +20.749 +39.233 +16.376 +34.900 +17.757 +38.636 +19.800 +35.546
04=HH_ 15 +19.551 +32.375 111.885 +0.000 0000 0 +21.159 +34.188 +17.942 +30.562 +19.551 +33.688 +19.551 +31.620
05=HS_ 01 +20.930 +24.217 103.727 +0.000 0000 0 +21.934 +25.226 +19.925 +23.208 +20.930 +24.726 +20.930 +23.708
06=AX_ 01 +16.858 +05.100 084.610 -1.000 0000 0 +16.858 +05.100 +16.858 +05.100
07=HS_ 01 +02.260 -08.709 070.801 +0.000 0000 0 +03.150 -07.789 +01.380 -09.628 +02.260 -08.289 +02.260 -09.128
08=CAI 10 +15.922 -29.540 049.970 +0.000 0000 0 +17.245 -24.554 +14.599 -34.527 +15.922 -24.754 +15.922 -34.327
09=BXI 07 -20.165 +58.412 137.922 +0.000 0000 0 -18.842 +62.433 -21.488 +54.390 -20.165 +62.233 -20.165 +54.590
10=CSO 03 -25.304 +48.684 128.194 +0.000 0000 0 -23.282 +50.984 -27.326 +46.384 -25.304 +50.784 -25.304 +46.584
11=AX_ 03 -28.465 +39.480 118.558 +0.000 0000 0 -27.513 +39.997 -29.418 +38.980 +00.000 +00.000 +00.000 +00.000
12=BXI 13 -16.602 -11.210 068.489 +0.000 0000 0 -15.770 -06.497 -18.128 -15.545 -16.602 -06.697 -16.602 -15.345
20220618.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 →

2022/20220618_ööt · ÖÖT · 6 frames · 128.6 MB · 12:21:55–12:37:24 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.