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20151024 - Filament data for 12 UTC
Available data for 20151024: »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1161 1729 (N42W35 L=132)   590    171        2 (1093/1689-1229/1765) -16.7 W29-W41 N40-N43
      2 1166 1488 (N27W22 L=119)   507    193        1 (1080/1452-1253/1540)   0.0 W15-W29 N25-N27
      3 1515 1482 (N16W44 L=141)   986    301        2 (1399/1451-1658/1536) -38.7 W38-W53 N10-N22
      4 1853 1395 (N01W72 L=169)   704    184        0 (1828/1375-1884/1411)   0.0 W67-W81 N00-N01
      5 1390 1376 (N14W31 L=128)   297     67        1 (1364/1350-1426/1400) -11.3 W28-W33 N12-N15
      6 1872 1133 (S14W60 L=157)  1585    275        1 (1852/1003-1894/1252)  49.8 W55-W68 S21-S07
      7 1229 1058 (N02W12 L=109)   246     84        1 (1181/1042-1268/1080) -31.0 W09-W14 N00-N04
      8  350  966 (N18E44 L= 53)   793    178        3 ( 292/ 923- 438/1016) -35.0 E48-E37 N14-N21
      9 1680  948 (S17W38 L=135)   621    134        1 (1631/ 900-1718/ 998) -54.5 W35-W40 S20-S13
     10 1713  829 (S26W38 L=135)   335     64        1 (1692/ 800-1733/ 865)  36.9 W36-W40 S26-S23
     11 1253  702 (S19W04 L=101)   863    363        2 (1159/ 626-1409/ 797)   9.5 E02-W16 S22-S16
     12 1577  645 (S33W25 L=122)   326     53        1 (1550/ 617-1602/ 670)  14.0 W22-W26 S34-S30
     13 1341  520 (S33W05 L=102)  1094    194        2 (1301/ 440-1371/ 619)  54.0 W00-W08 S37-S26
     14  781  415 (S24E33 L= 64)   929    245        4 ( 746/ 321- 837/ 492)  69.0 E36-E27 S31-S18
     15 1499  397 (S49W15 L=112)  2743    444        3 (1398/ 326-1604/ 479)  18.4 W05-W25 S54-S42
     16  518  331 (S23E57 L= 40)  1767    348        2 ( 492/ 259- 561/ 421)  47.5 E64-E51 S28-S16
  
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.