|
|
|
|
| 20240930 - Filament data for 11 UTC |
|
Available data for 20240930: »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 1230 1747 (N41W44 L=260) 747 121 1 (1179/1698-1268/1788) 12.1 W36-W50 N39-N42
2 1669 1677 (N21W76 L=292) 805 63 0 (1637/1654-1691/1704) -3.0 W68-W87 N19-N21
3 1692 1530 (N13W62 L=278) 1770 179 4 (1640/1455-1739/1615) 59.0 W57-W66 N08-N19
4 1590 1301 (N05W41 L=258) 779 173 0 (1506/1240-1653/1342) -56.3 W37-W44 N00-N09
5 1461 1212 (N05W30 L=246) 296 84 0 (1439/1167-1482/1254) 38.7 W27-W32 N02-N06
6 1819 1030 (S17W52 L=268) 682 142 0 (1772/ 965-1848/1059) -58.0 W47-W55 S21-S13
7 1022 853 (S03E05 L=212) 1183 393 0 ( 960/ 692-1114/ 975) 80.0 E06-W00 S13-N04
8 1797 905 (S23W47 L=263) 306 69 0 (1763/ 884-1823/ 932) 0.0 W43-W50 S24-S22
9 650 880 (N08E25 L=191) 219 64 0 ( 613/ 862- 679/ 902) 0.0 E27-E22 N07-N08
10 456 774 (N06E41 L=175) 376 119 0 ( 398/ 763- 513/ 786) -18.4 E45-E36 N04-N07
11 693 648 (S06E29 L=187) 232 110 0 ( 643/ 632- 743/ 673) 0.0 E32-E25 S06-S05
12 633 552 (S10E36 L=180) 1509 276 4 ( 568/ 455- 695/ 647) 81.3 E41-E32 S17-S04
13 560 462 (S14E46 L=171) 1446 368 4 ( 500/ 362- 677/ 598) -90.0 E50-E41 S22-S04
14 768 515 (S16E29 L=187) 430 89 0 ( 713/ 495- 808/ 542) 0.0 E33-E26 S16-S14
15 743 435 (S20E35 L=182) 582 140 2 ( 690/ 377- 788/ 486) 22.6 E41-E29 S22-S17
16 914 388 (S27E26 L=190) 1301 206 3 ( 860/ 303- 969/ 480) 28.1 E34-E19 S32-S21
17 497 341 (S21E60 L=156) 1411 160 1 ( 448/ 274- 534/ 410) 24.2 E71-E51 S25-S16
18 1077 345 (S35E18 L=198) 1239 203 3 ( 974/ 302-1166/ 396) -3.6 E26-E10 S36-S33
19 724 228 (S34E51 L=165) 760 98 1 ( 693/ 193- 754/ 283) 28.3 E57-E44 S36-S29
|
Download FITS filament maps as tar archive
» All Filament Data of 20240930 ...
|
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.
|
|
|
|