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| 20230927 - Filament data for 10 UTC |
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Available data for 20230927: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1055 1695 (N45W28 L= 75) 1030 177 4 ( 980/1657-1139/1718) -31.0 W20-W33 N42-N48
2 1389 1566 (N26W41 L= 89) 299 66 1 (1363/1545-1424/1580) 0.0 W38-W44 N24-N27
3 1598 1459 (N14W50 L= 97) 680 111 1 (1542/1441-1653/1484) -16.7 W45-W55 N12-N15
4 944 1284 (N24W02 L= 50) 292 71 1 ( 915/1254- 976/1314) 14.0 W00-W04 N22-N25
5 1867 1192 (S09W64 L=111) 671 84 1 (1840/1160-1905/1209) 0.0 W59-W70 S11-S07
6 660 1073 (N19E20 L= 27) 697 202 1 ( 589/1004- 731/1145) 18.4 E26-E14 N16-N21
7 1823 1097 (S13W55 L=103) 402 58 0 (1799/1075-1854/1116) -8.1 W52-W59 S14-S11
8 184 997 (N24E64 L=343) 2176 217 3 ( 160/ 907- 234/1109) 76.0 E68-E57 N18-N30
9 997 1025 (N08E01 L= 46) 300 58 2 ( 968/ 994-1025/1057) 45.0 E03-W00 N06-N09
10 347 996 (N21E45 L= 2) 989 256 1 ( 235/ 915- 404/1052) -35.5 E56-E41 N15-N25
11 263 899 (N17E55 L=352) 606 99 1 ( 244/ 861- 284/ 958) 71.6 E58-E53 N14-N20
12 1764 874 (S24W45 L= 92) 725 147 0 (1727/ 818-1804/ 932) 24.0 W40-W49 S25-S21
13 1813 816 (S29W50 L= 97) 394 55 1 (1790/ 793-1834/ 848) 21.8 W46-W52 S30-S27
14 200 768 (N10E67 L=340) 500 73 1 ( 184/ 734- 219/ 807) -78.7 E68-E65 N07-N12
15 1401 763 (S18W15 L= 62) 1059 357 1 (1237/ 746-1560/ 797) -20.9 W05-W26 S22-S13
16 858 600 (S13E21 L= 26) 229 63 1 ( 827/ 581- 893/ 613) -14.0 E22-E18 S14-S11
17 535 441 (S16E50 L=358) 693 168 1 ( 502/ 372- 563/ 516) 42.0 E54-E43 S20-S11
18 871 479 (S21E25 L= 23) 323 62 1 ( 852/ 452- 897/ 516) 63.4 E26-E23 S22-S18
19 470 386 (S18E60 L=348) 629 71 2 ( 440/ 356- 509/ 410) -31.0 E63-E55 S20-S16
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Download FITS filament maps as tar archive
» All Filament Data of 20230927 ...
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The tar archive contains filament maps for all processed Hα images
with at least quality=1.
The maps contain the values 0 and 1, where 1 is the position of a detected filament.
The header in the FITS files is mostly taken from the corresponding Hα file,
so it should be compatible with standard solar software routines.
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