|
|
|
|
| 20251112 - Filament data for 07 UTC |
|
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 1494 1697 (N30W55 L=289) 937 185 3 (1439/1618-1548/1757) 9.0 W45-W64 N26-N33
2 1271 1687 (N36W37 L=271) 640 151 0 (1229/1629-1310/1748) 71.6 W34-W39 N31-N40
3 637 1598 (N47E14 L=220) 327 40 0 ( 617/1571- 663/1619) 14.0 E15-E11 N45-N49
4 496 1569 (N49E28 L=206) 645 106 1 ( 465/1525- 534/1613) -74.1 E31-E23 N45-N52
5 1445 1574 (N24W42 L=276) 570 104 3 (1414/1534-1474/1613) 68.2 W39-W45 N21-N26
6 1570 1501 (N17W48 L=281) 533 203 0 (1490/1453-1610/1561) 8.7 W39-W52 N15-N20
7 1058 1533 (N32W15 L=249) 1580 362 2 ( 872/1495-1212/1558) -16.9 W02-W25 N28-N35
8 1451 1266 (N07W30 L=264) 562 258 0 (1339/1235-1532/1321) -28.6 W24-W36 N04-N12
9 1833 1270 (S02W61 L=295) 422 42 1 (1808/1247-1852/1290) -11.3 W58-W63 S03-N00
10 407 1101 (N20E37 L=196) 1124 322 1 ( 272/1040- 524/1179) -34.4 E49-E29 N14-N27
11 181 903 (N13E62 L=172) 1632 217 5 ( 150/ 799- 211/1008) 81.3 E65-E58 N06-N19
12 805 939 (N03E14 L=220) 236 81 1 ( 776/ 908- 837/ 974) 45.0 E15-E11 N01-N04
13 1218 835 (S12W07 L=241) 1142 403 7 (1126/ 740-1297/ 932) 85.2 W01-W11 S17-S05
14 1766 698 (S34W46 L=280) 805 136 0 (1706/ 663-1813/ 745) 9.5 W39-W51 S35-S32
15 735 657 (S12E25 L=209) 621 274 1 ( 650/ 600- 842/ 697) -4.4 E30-E17 S14-S09
16 430 500 (S15E53 L=181) 367 82 1 ( 393/ 486- 473/ 516) -18.4 E55-E49 S15-S13
17 692 386 (S27E39 L=195) 1912 381 2 ( 547/ 318- 868/ 479) 5.4 E55-E23 S29-S24
18 1099 288 (S45E17 L=217) 1530 266 1 ( 993/ 235-1210/ 374) 10.3 E26-E04 S47-S41
|
Download FITS filament maps as tar archive
» All Filament Data of 20251112 ...
|
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.
|
|
|
|