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| 20251112 - Filament data for 08 UTC |
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Available data for 20251112: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1517 1735 (N32W61 L=294) 593 60 1 (1489/1708-1551/1760) -7.1 W56-W64 N30-N33
2 1275 1696 (N36W38 L=271) 516 129 1 (1231/1645-1307/1746) 76.0 W36-W39 N32-N40
3 1463 1644 (N28W48 L=281) 328 63 1 (1440/1620-1497/1666) 9.5 W45-W51 N26-N29
4 641 1602 (N48E13 L=220) 333 44 0 ( 621/1574- 667/1621) 45.0 E15-E10 N45-N49
5 1525 1597 (N24W49 L=283) 326 43 2 (1500/1569-1548/1619) 0.0 W46-W52 N22-N25
6 498 1568 (N49E28 L=206) 580 103 3 ( 469/1526- 534/1611) -74.1 E31-E23 N45-N52
7 1465 1552 (N23W42 L=276) 457 118 1 (1419/1506-1505/1596) -81.9 W41-W43 N19-N26
8 1587 1512 (N17W49 L=283) 428 146 0 (1538/1478-1615/1561) 26.6 W44-W52 N15-N20
9 1059 1536 (N32W15 L=249) 1383 355 3 ( 878/1497-1211/1560) -17.7 W03-W25 N28-N36
10 1406 1278 (N09W28 L=261) 903 345 2 (1287/1239-1537/1324) -17.4 W20-W36 N04-N12
11 417 1100 (N20E37 L=197) 1103 312 2 ( 279/1039- 530/1183) -33.0 E48-E28 N14-N27
12 187 907 (N13E61 L=172) 1078 244 2 ( 161/ 810- 214/1032) 81.3 E64-E58 N07-N20
13 815 945 (N03E13 L=220) 241 73 2 ( 782/ 912- 851/ 982) 45.0 E15-E10 N01-N04
14 1181 874 (S09W06 L=239) 366 162 2 (1155/ 837-1228/ 933) 68.2 W03-W07 S10-S05
15 1250 812 (S14W08 L=242) 710 256 5 (1185/ 732-1301/ 895) 60.9 W03-W11 S17-S08
16 1769 698 (S34W46 L=280) 807 124 0 (1709/ 664-1814/ 744) 9.5 W39-W51 S35-S32
17 750 664 (S11E24 L=209) 555 248 1 ( 657/ 619- 850/ 703) 0.0 E30-E17 S13-S09
18 696 385 (S27E39 L=195) 1961 380 6 ( 545/ 318- 870/ 479) 5.2 E55-E22 S29-S24
19 1101 288 (S45E16 L=217) 1589 274 2 ( 996/ 231-1221/ 377) 9.9 E26-E03 S47-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20251112 ...
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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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