Solar Images Friday, 17 May 2024

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Photosphere sunspot drawing and RDS evaluation

17.05.2024 photosphere drawing

High-resolution scan (3229 px)

Time
08:00 UT
Observer
Ergün EGE
g
12
f
41
R
161
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=17.05.2024
Saat=08:00
Gözlemci=Ergün EGE
KontrolEden=Burçin TANIK
Durumaçısı=-20.17
Enlemaçısı=-2.38
Boylamaçısı=216.62
Boylamfark=2
GKalite=3
GDurum=B.A
Kuzeyaçısı=-0.4
Sırano=19980
AyRasatNo=10
RasatÖnceki=16.05.2024
RasatSonraki=18.05.2024

[Leke Grupları]
Grupsayısı=12:3:9
LekeSayısı=41:7:34
RölatifSayı=161:37:124
01=BXO 03 +21.419 +64.492 281.112 +0.000 0000 0 +23.100 +68.746 +19.837 +60.239 +21.419 +68.546 +21.419 +60.439
02=CSO 02 +19.529 +34.155 250.775 +0.000 0000 0 +20.365 +35.830 +18.692 +32.480 +19.529 +35.630 +19.529 +32.680
03=BXO 02 +15.900 -22.710 193.910 +0.000 0000 0 +17.429 -19.679 +12.751 -25.741 +15.900 -19.879 +15.900 -25.541
04=HS_ 02 -19.548 +48.261 264.881 +0.000 0000 0 -18.389 +50.141 -20.708 +46.380 -19.548 +49.642 -19.548 +46.881
05=BXI 09 -23.680 +22.763 239.383 +0.000 0000 0 -21.110 +27.680 -25.125 +18.457 -23.680 +26.868 -23.680 +18.657
06=HS_ 01 -08.655 +14.358 230.978 +0.000 0000 0 -08.104 +14.642 -09.205 +14.740 -08.655 +13.907 -08.655 +14.809
07=CSI 05 -12.496 +03.346 219.966 +0.000 0000 0 -10.580 +06.422 -14.411 +00.270 -12.496 +06.222 -12.496 +00.470
08=CSI 08 -08.485 -17.832 198.788 +0.000 0000 0 -06.375 -11.924 -10.595 -23.740 -08.485 -12.124 -08.485 -23.540
09=HK_ 02 -14.881 -61.509 155.111 +0.000 0000 0 -13.527 -60.596 -16.235 -62.422 -14.881 -61.960 -14.881 -61.922
10=CSO 03 -12.130 -64.374 152.246 +0.000 0000 0 -10.808 -60.606 -13.218 -68.141 -12.130 -60.806 -12.130 -67.941
11=CSO 02 -15.200 -70.919 145.701 +0.000 0000 0 -13.641 -67.647 -16.363 -74.192 -15.200 -67.847 -15.200 -73.992
12=HK_ 02 -08.490 -75.219 141.401 +0.000 0000 0 -06.884 -73.465 -09.214 -76.974 -08.490 -73.965 -08.490 -76.474
20240517.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 →

2024/20240517_ee · EE · 9 frames · 192.8 MB · 08:08:42–08:21:56 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.