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| 20231228 - Latest Filament data |
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Available data for 20231228: »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 1082 1767 (N48W09 L=282) 922 138 3 (1036/1723-1142/1818) -41.2 W05-W13 N43-N53
2 1548 1656 (N37W47 L=320) 1594 353 1 (1364/1627-1691/1682) -5.0 W30-W65 N34-N39
3 1302 1529 (N28W21 L=294) 3275 751 4 ( 964/1377-1593/1612) -19.7 E02-W40 N17-N34
4 1005 1399 (N20W00 L=273) 232 86 0 ( 980/1364-1039/1435) -53.1 E01-W02 N18-N22
5 1799 1322 (N14W58 L=331) 1406 185 4 (1747/1256-1856/1402) -55.0 W54-W63 N09-N19
6 610 1351 (N19E26 L=247) 310 75 2 ( 576/1333- 649/1372) -21.8 E28-E23 N17-N20
7 1720 1295 (N12W49 L=322) 622 128 0 (1662/1254-1760/1330) -26.6 W44-W52 N09-N14
8 1582 1245 (N09W37 L=310) 226 69 0 (1569/1206-1601/1271) 53.1 W35-W38 N06-N10
9 763 1168 (N07E15 L=258) 400 130 1 ( 710/1122- 806/1220) -45.0 E18-E12 N04-N10
10 1769 892 (S12W52 L=325) 2196 342 5 (1696/ 746-1841/1055) 68.7 W45-W58 S20-S02
11 1149 871 (S12W07 L=280) 193 56 1 (1129/ 841-1173/ 896) 56.3 W05-W08 S13-S10
12 1425 774 (S19W25 L=298) 647 244 0 (1395/ 659-1486/ 876) 69.0 W23-W28 S25-S12
13 1878 789 (S18W67 L=340) 730 94 3 (1850/ 755-1904/ 834) -32.0 W63-W72 S20-S15
14 205 763 (S14E64 L=209) 568 92 1 ( 173/ 741- 254/ 795) -26.6 E67-E57 S15-S11
15 305 686 (S20E55 L=218) 476 112 2 ( 278/ 635- 325/ 729) 71.6 E57-E52 S22-S16
16 1677 540 (S34W52 L=325) 1702 245 1 (1571/ 480-1765/ 627) 33.7 W42-W59 S38-S28
17 1108 591 (S30W04 L=277) 203 79 0 (1082/ 557-1138/ 624) 45.0 W02-W06 S31-S27
18 1314 463 (S39W20 L=293) 392 92 1 (1288/ 437-1357/ 502) -39.8 W18-W24 S41-S36
19 970 420 (S41E07 L=266) 385 64 1 ( 933/ 404-1005/ 441) 11.3 E09-E04 S42-S39
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Download FITS filament maps as tar archive
» All Filament Data of 20231228 ...
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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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