Istanbul University Faculty of Science

SOLAR OBSERVATIONS

Istanbul University Observatory · Sunspot observations since 1950

Observatory

Solar Images Tuesday, 14 March 2023

‹ 13.03.2023 2023 15.03.2023 ›

Photosphere sunspot drawing and RDS evaluation

14.03.2023 photosphere drawing

High-resolution scan (3230 px)

Time
07:30 UT
Observer
Korhan YELKENCİ
g
9
f
26
R
116
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

Group 1 · CSI – 5Group 1 · CSI – 5 Group 2 · HS_ – 1Group 2 · HS_ – 1 Group 3 · HS_ – 2Group 3 · HS_ – 2 Group 4 · HS_ – 1Group 4 · HS_ – 1 Group 5 · CAI – 6Group 5 · CAI – 6 Group 6 · CAI – 8Group 6 · CAI – 8 Group 7 · AX_ – 1Group 7 · AX_ – 1 Group 8 · HS_ – 1Group 8 · HS_ – 1 Group 9 · AX_ – 1Group 9 · AX_ – 1
RDS data file (.gzd) 
[Gözlem]
Tarih=14.03.2023
Saat=07:30
Gözlemci=Korhan YELKENCİ
KontrolEden=Olcay PLEVNE
Durumaçısı=-24.24
Enlemaçısı=-7.19
Boylamaçısı=132.68
Boylamfark=2
GKalite=3
GDurum=K.T
Kuzeyaçısı=-0.5
Sırano=19674
AyRasatNo=8
RasatÖnceki=13.03.2023
RasatSonraki=15.03.2023

[Leke Grupları]
Grupsayısı=9:2:7
LekeSayısı=26:6:20
RölatifSayı=116:26:90
01=CSI 05 +13.397 +09.491 142.171 26.842 0000 0 +14.730 +11.862 +12.630 +07.120 +14.398 +11.586 +12.263 +07.362
02=HS_ 01 +11.641 -16.132 116.548 +0.000 0000 0 +12.117 -15.675 +11.165 -16.589 +11.641 -16.175 +11.641 -16.890
03=HS_ 02 -23.559 +59.156 191.836 +0.000 0000 0 -22.456 +61.650 -24.662 +57.248 -23.559 +60.857 -23.559 +57.455
04=HS_ 01 -24.415 +27.627 160.307 +0.000 0000 0 -23.819 +28.228 -25.100 +27.260 -24.415 +27.611 -24.415 +27.643
05=CAI 06 -25.168 +19.122 151.802 38.760 0000 0 -23.578 +21.570 -26.759 +17.188 -23.778 +20.857 -26.559 +17.388
06=CAI 08 -19.869 +10.448 143.128 36.364 0000 0 -18.470 +12.279 -21.268 +08.617 -18.670 +12.790 -21.680 +08.817
07=AX_ 01 -12.133 +06.286 138.966 -1.000 0000 0 -12.133 +06.286 -12.133 +06.286
08=HS_ 01 -14.800 -15.500 117.675 +0.000 0000 0 -14.300 -14.249 -15.571 -15.760 -14.800 -15.245 -14.800 -15.755
09=AX_ 01 -06.980 -50.793 081.887 -1.000 0000 0 -06.980 -50.793 -06.980 -50.793
20230314.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 →

2023/20230314_ky · KY · 30 frames · 642.7 MB · 07:51:16–08:06:27 UT

07:56:16 UT · 30 ms 07:52:16 UT · 30 ms 08:00:28 UT · 30 ms 08:04:27 UT · 30 ms 07:55:46 UT · 50 ms · over-exposed 07:51:46 UT · 50 ms · over-exposed 08:03:57 UT · 50 ms · over-exposed 07:59:58 UT · 50 ms · over-exposed 07:51:16 UT · 60 ms · over-exposed 07:55:15 UT · 60 ms · over-exposed 08:03:27 UT · 60 ms · over-exposed 07:59:28 UT · 60 ms · over-exposed 07:56:46 UT · 60 ms 07:57:15 UT · 50 ms 07:57:45 UT · 30 ms 07:54:46 UT 07:52:46 UT · 60 ms 07:53:16 UT · 50 ms 07:53:46 UT · 30 ms 07:54:16 UT 08:06:27 UT 08:04:57 UT · 60 ms 08:05:27 UT · 50 ms 08:05:57 UT · 30 ms 08:02:57 UT 08:00:58 UT · 60 ms 08:01:28 UT · 50 ms 08:01:58 UT · 30 ms 08:02:27 UT 07:58:15 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.