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| 20231229 - Filament data for 11 UTC |
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Available data for 20231229: »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 1212 1780 (N48W21 L=281) 1318 209 6 (1143/1731-1297/1841) -36.0 W15-W27 N43-N54
2 1610 1660 (N38W54 L=315) 1246 183 2 (1515/1639-1691/1681) 0.0 W43-W70 N36-N39
3 1542 1493 (N25W38 L=299) 6329 971 9 (1144/1240-1878/1623) -21.4 W10-W66 N09-N35
4 1524 1369 (N17W34 L=295) 458 112 0 (1508/1313-1549/1411) -90.0 W32-W36 N13-N20
5 816 1345 (N17E12 L=249) 561 123 3 ( 765/1302- 866/1382) -45.0 E15-E08 N14-N20
6 1743 1249 (N10W50 L=311) 432 82 1 (1728/1200-1769/1291) 71.6 W48-W53 N06-N12
7 1653 1258 (N10W42 L=303) 287 49 0 (1629/1236-1677/1287) 53.1 W40-W44 N08-N12
8 1833 1217 (N08W59 L=320) 718 60 1 (1807/1186-1860/1247) -36.9 W56-W62 N06-N09
9 403 1204 (N11E40 L=220) 348 130 0 ( 354/1183- 469/1234) 12.5 E44-E35 N09-N12
10 967 1193 (N08E03 L=258) 276 92 0 ( 928/1157-1003/1229) -45.0 E05-W00 N05-N09
11 1886 875 (S13W66 L=326) 2832 283 1 (1826/ 759-1945/1012) 53.7 W59-W74 S19-S04
12 1600 797 (S18W38 L=299) 844 276 0 (1558/ 685-1663/ 925) 71.6 W35-W42 S24-S09
13 404 766 (S16E43 L=218) 831 211 4 ( 306/ 739- 498/ 791) -3.6 E51-E35 S17-S13
14 389 601 (S26E49 L=211) 581 114 0 ( 342/ 568- 436/ 643) 18.4 E55-E43 S27-S23
15 1266 590 (S30W15 L=276) 226 74 0 (1240/ 557-1301/ 621) 53.1 W13-W17 S32-S28
16 1734 506 (S36W62 L=323) 1716 195 1 (1649/ 472-1806/ 560) 16.4 W50-W72 S38-S32
17 1467 464 (S39W34 L=295) 683 109 3 (1417/ 422-1510/ 505) -12.5 W29-W38 S42-S36
18 1149 449 (S40W08 L=268) 769 179 2 (1066/ 419-1233/ 486) 14.0 W01-W13 S41-S37
19 374 384 (S40E69 L=192) 647 72 0 ( 342/ 359- 397/ 416) 7.8 E82-E60 S41-S38
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Download FITS filament maps as tar archive
» All Filament Data of 20231229 ...
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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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