Solar Images Wednesday, 18 June 2025

‹ 17.06.2025 2025 19.06.2025 ›

Photosphere sunspot drawing and RDS evaluation

18.06.2025 photosphere drawing

High-resolution scan (3229 px)

Time
07:50 UT
Observer
Burçin TANIK
g
6
f
72
R
132
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=18.06.2025
Saat=07:50
Gözlemci=Burçin TANIK
KontrolEden=Korhan YELKENCİ
Durumaçısı=-8.27
Enlemaçısı=1.41
Boylamaçısı=15.7
Boylamfark=2
GKalite=3
GDurum=G.T
Kuzeyaçısı=-0.8
Sırano=20274
AyRasatNo=17
RasatÖnceki=17.06.2025
RasatSonraki=19.06.2025

[Leke Grupları]
Grupsayısı=6:3:3
LekeSayısı=72:59:13
RölatifSayı=132:89:43
01=?__ 07 +14.574 +40.302 056.200 -1.000 0000 0 +17.162 +43.113 +11.986 +37.492
02=EKC 43 +18.192 +15.835 031.535 21.950 0000 0 +21.711 +22.611 +14.673 +09.580 +15.604 +19.541 +18.892 +11.346
03=EKO 09 +20.337 +01.972 017.672 11.400 0000 0 +22.672 +08.552 +18.300 -04.608 +19.105 +06.286 +21.520 -03.423
04=CAO 07 -12.147 +17.435 033.135 +0.000 0000 0 -10.852 +21.454 -13.441 +13.417 -12.147 +21.254 -12.147 +13.617
05=DRO 05 -15.265 -76.820 298.880 +0.000 0000 0 -14.770 -71.285 -16.453 -82.355 -15.265 -71.485 -15.265 -82.155
06=AX_ 01 -11.170 -80.557 295.143 -1.000 0000 0 -11.170 -80.557 -11.170 -80.557
20250618.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 →

2025/20250618_bto · BTO · 4 frames · 85.7 MB · 07:54:32–08:00:14 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.