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20260221 - Filament data for 11 UTC
Available data for 20260221: »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1397 1553 (N33W12 L=353)   321     69        1 (1377/1517-1420/1586)  80.5 W10-W13 N30-N36
      2  645 1497 (N13E34 L=308)   942    167        4 ( 603/1428- 693/1571)  90.0 E35-E31 N08-N18
      3 1247 1516 (N27W02 L=344)   317     59        0 (1216/1493-1279/1538)   0.0 W00-W04 N25-N28
      4 1654 1489 (N37W34 L= 15)   393    100        0 (1613/1444-1692/1520)  -7.1 W29-W37 N34-N38
      5  297 1270 (S06E53 L=288)   832    165        1 ( 263/1196- 351/1312)  58.0 E55-E48 S10-S02
      6 1711 1139 (N16W40 L= 22)   950    297        0 (1601/1028-1768/1246) -29.4 W30-W46 N10-N19
      7  580 1172 (S07E29 L=312)   210     72        0 ( 560/1135- 604/1205)  78.7 E30-E28 S09-S04
      8 1847 1076 (N16W54 L= 36)   344    106        0 (1814/1051-1864/1122)  59.0 W50-W56 N14-N19
      9  345  964 (S23E44 L=298)  1342    398        3 ( 234/ 853- 466/1097)  43.4 E55-E35 S30-S13
     10  715  931 (S18E16 L=325)   191     93        0 ( 674/ 915- 766/ 944)  21.8 E18-E13 S20-S17
     11 1356  911 (S06W21 L=  3)   285     87        1 (1310/ 887-1388/ 937) -11.3 W18-W23 S07-S04
     12 1626  780 (S06W43 L= 24)   331     99        1 (1598/ 735-1649/ 827)  90.0 W41-W43 S09-S03
     13 1376  673 (S19W29 L= 11)  1062    368        0 (1203/ 608-1512/ 755)  45.0 W20-W35 S26-S10
     14  971  711 (S26W04 L=345)   207     33        0 ( 954/ 684- 990/ 731) -33.7 W02-W05 S27-S24
     15 1760  664 (S09W59 L= 40)   709    148        0 (1718/ 606-1805/ 725)  71.6 W56-W60 S12-S03
     16 1803  556 (S12W71 L= 53)  1225     87        2 (1763/ 530-1839/ 577)   7.1 W64-W80 S14-S10
     17 1574  487 (S23W52 L= 34)   489    118        1 (1534/ 437-1621/ 536)  90.0 W50-W54 S26-S19
     18 1632  454 (S23W60 L= 41)   894    177        1 (1557/ 408-1698/ 509)  56.3 W56-W63 S27-S18
  
Data will be available after one hour of observations. 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.