|
|
|
|
| 20250124 - Filament data for 12 UTC |
|
Available data for 20250124: »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
1 684 1676 (N33E33 L= 94) 389 51 1 ( 655/1655- 712/1704) 14.0 E34-E30 N31-N35
2 1169 1540 (N28W04 L=131) 1158 393 2 (1070/1486-1351/1639) -20.2 E03-W16 N24-N33
3 1625 1262 (N16W36 L=163) 408 83 3 (1599/1221-1650/1297) 51.3 W34-W38 N12-N17
4 1733 1225 (N15W45 L=172) 395 92 0 (1711/1181-1764/1272) -59.0 W43-W48 N12-N17
5 1559 1124 (N06W32 L=159) 1386 379 1 (1419/ 978-1630/1262) -40.9 W21-W38 S01-N12
6 362 1065 (S08E43 L= 84) 261 98 0 ( 353/1011- 373/1119) -81.9 E44-E42 S11-S04
7 1034 1066 (S03W00 L=127) 440 162 0 ( 955/1016-1093/1092) -20.6 E04-W04 S05-S01
8 169 888 (S19E63 L= 63) 4629 382 6 ( 95/ 761- 215/1069) 52.1 E83-E57 S26-S08
9 105 1006 (S12E72 L= 55) 752 69 2 ( 75/ 979- 135/1033) -16.7 E79-E67 S13-S09
10 1435 959 (S05W25 L=152) 204 47 1 (1410/ 944-1467/ 975) 33.7 W23-W27 S05-S03
11 368 888 (S18E43 L= 84) 1063 285 1 ( 303/ 825- 430/ 956) -45.0 E48-E37 S22-S14
12 1807 864 (S05W56 L=182) 864 103 4 (1763/ 823-1859/ 905) 0.0 W50-W61 S07-S03
13 1295 736 (S19W20 L=147) 888 333 2 (1221/ 631-1382/ 876) -42.7 W13-W28 S24-S11
14 1748 717 (S14W54 L=181) 1935 232 5 (1660/ 656-1825/ 773) 28.3 W47-W63 S18-S11
15 1524 722 (S17W36 L=163) 876 271 2 (1402/ 659-1627/ 767) 32.7 W28-W43 S22-S13
16 1657 726 (S15W46 L=173) 276 44 0 (1637/ 700-1675/ 755) 90.0 W44-W46 S16-S13
17 324 549 (S40E56 L= 71) 1787 159 5 ( 245/ 499- 402/ 584) 5.9 E74-E45 S43-S37
18 1640 393 (S35W64 L=190) 1109 103 2 (1600/ 368-1686/ 426) 0.0 W56-W71 S37-S33
19 1580 300 (S42W68 L=195) 523 60 1 (1561/ 264-1598/ 331) -26.6 W62-W74 S44-S40
|
Download FITS filament maps as tar archive
» All Filament Data of 20250124 ...
|
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.
|
|
|
|