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| 20251003 - Filament data for 11 UTC |
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Available data for 20251003: »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
1 895 1848 (N63W32 L= 72) 748 95 1 ( 861/1809- 922/1888) 13.2 W25-W42 N59-N65
2 855 1785 (N59W20 L= 59) 339 53 1 ( 823/1767- 883/1805) -31.0 W16-W22 N56-N60
3 1242 1729 (N40W42 L= 82) 297 48 0 (1218/1706-1269/1753) -90.0 W40-W44 N37-N41
4 698 1722 (N60W00 L= 39) 456 84 1 ( 664/1692- 738/1746) 6.3 E04-W05 N58-N61
5 1533 1713 (N28W63 L=103) 597 49 0 (1507/1689-1562/1737) -56.3 W59-W66 N26-N29
6 1436 1548 (N23W43 L= 82) 1348 314 3 (1276/1503-1573/1595) -39.1 W34-W51 N17-N30
7 1761 1391 (N05W60 L= 99) 794 161 1 (1742/1320-1781/1477) 45.0 W56-W65 N00-N08
8 1237 1260 (N14W18 L= 58) 225 121 0 (1208/1213-1251/1309) 71.6 W16-W19 N11-N17
9 1068 1237 (N17W08 L= 48) 855 262 4 ( 975/1185-1152/1289) -20.0 W02-W13 N14-N20
10 515 1223 (N30E27 L= 12) 307 91 0 ( 468/1209- 561/1241) -7.1 E31-E23 N29-N31
11 1278 1166 (N08W18 L= 57) 279 82 0 (1237/1149-1302/1196) 0.0 W15-W19 N06-N08
12 921 1157 (N16E02 L= 37) 408 161 0 ( 844/1142-1002/1169) -35.5 E06-W02 N13-N18
13 419 1122 (N27E36 L= 3) 562 127 0 ( 361/1105- 497/1144) -20.0 E41-E30 N23-N28
14 1181 897 (S04W05 L= 45) 437 114 0 (1134/ 877-1231/ 933) 9.5 W02-W08 S05-S03
15 926 717 (S08E13 L= 26) 887 288 0 ( 881/ 604- 971/ 808) 77.0 E15-E09 S15-S02
16 761 472 (S18E31 L= 8) 1150 341 1 ( 656/ 427- 888/ 532) -31.6 E36-E23 S23-S13
17 1542 496 (S41W20 L= 59) 723 85 3 (1499/ 465-1583/ 521) 7.1 W15-W23 S42-S38
18 475 359 (S20E60 L=339) 1805 256 1 ( 452/ 272- 502/ 478) 30.3 E73-E49 S26-S12
19 1146 256 (S45E19 L= 21) 1791 332 1 (1025/ 173-1291/ 345) 8.1 E33-E04 S49-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20251003 ...
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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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