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| 20231228 - Filament data for 12 UTC |
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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 1078 1769 (N48W09 L=282) 1051 143 4 (1031/1723-1141/1828) -41.2 W04-W13 N43-N54
2 1543 1656 (N37W46 L=319) 1612 344 3 (1360/1619-1686/1683) -5.0 W29-W63 N34-N39
3 1301 1527 (N28W21 L=294) 3398 752 2 ( 960/1374-1590/1609) -20.1 E02-W39 N17-N34
4 1001 1396 (N20E00 L=273) 289 83 0 ( 969/1358-1036/1430) -59.0 E02-W01 N17-N22
5 1794 1326 (N14W58 L=331) 1540 204 3 (1731/1252-1859/1407) -48.0 W52-W65 N09-N19
6 1336 1360 (N17W21 L=294) 230 90 0 (1326/1319-1352/1400) 78.7 W20-W22 N14-N19
7 603 1352 (N19E26 L=247) 347 70 2 ( 569/1336- 646/1375) -21.8 E28-E23 N18-N20
8 1718 1294 (N12W49 L=322) 631 120 1 (1659/1254-1757/1329) -29.7 W44-W52 N09-N14
9 1577 1242 (N09W36 L=310) 268 62 2 (1563/1206-1595/1272) 63.4 W35-W38 N06-N11
10 755 1167 (N07E16 L=257) 460 119 0 ( 706/1124- 801/1215) -45.0 E18-E13 N04-N10
11 1765 890 (S12W51 L=324) 2298 329 6 (1691/ 746-1839/1052) 68.7 W45-W58 S20-S02
12 1143 871 (S12W07 L=280) 216 60 1 (1122/ 840-1166/ 897) 56.3 W05-W08 S13-S10
13 1418 769 (S19W25 L=298) 710 245 0 (1386/ 662-1481/ 869) 67.4 W22-W28 S25-S13
14 1878 786 (S18W67 L=341) 660 92 2 (1853/ 755-1903/ 830) -32.0 W63-W72 S20-S15
15 301 690 (S19E55 L=218) 476 102 1 ( 277/ 638- 324/ 730) 71.6 E57-E52 S22-S16
16 1676 542 (S34W52 L=325) 1775 265 2 (1559/ 481-1762/ 627) 30.5 W41-W58 S38-S28
17 1103 589 (S30W04 L=277) 229 67 0 (1077/ 559-1136/ 622) 53.1 W01-W06 S31-S27
18 1310 461 (S39W20 L=293) 423 90 1 (1282/ 435-1355/ 500) -39.8 W17-W24 S41-S36
19 968 421 (S41E07 L=266) 402 55 1 ( 926/ 404-1002/ 441) 0.0 E10-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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