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20251228 - Filament data for 11 UTC
Available data for 20251228: »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  655 1672 (N41E27 L=318)   341     40        1 ( 627/1649- 682/1691)  36.9 E29-E25 N39-N42
      2 1085 1575 (N32W06 L=352)   884    184        0 ( 986/1551-1181/1595)   0.0 W00-W12 N29-N33
      3 1301 1535 (N28W21 L=  6)   356     59        1 (1270/1504-1324/1560) -53.1 W18-W22 N26-N30
      4  264 1418 (N25E57 L=288)  1104    106        4 ( 221/1385- 312/1459) -24.4 E64-E51 N22-N27
      5  300 1317 (N18E50 L=296)   309     59        0 ( 267/1292- 322/1342)  36.9 E53-E48 N16-N19
      6 1823 1272 (N11W58 L= 44)   504     57        2 (1799/1242-1844/1303)  71.6 W55-W61 N09-N12
      7  207 1243 (N14E59 L=287)   451     87        2 ( 183/1212- 241/1285) -26.6 E62-E54 N12-N16
      8 1380 1231 (N09W22 L=  8)   711    111        3 (1341/1175-1429/1276)  63.4 W19-W25 N05-N11
      9 1312 1170 (N05W18 L=  3)   196     32        0 (1290/1144-1335/1191) -56.3 W16-W19 N03-N06
     10  242 1072 (N04E53 L=292)   567     93        0 ( 206/1042- 268/1112)  31.0 E57-E50 N01-N05
     11 1746  934 (S09W48 L= 34)   556     82        2 (1713/ 901-1782/ 973)  45.0 W45-W51 S11-S06
     12 1805  861 (S13W55 L= 41)   466    103        0 (1781/ 814-1822/ 908)  71.6 W52-W56 S16-S10
     13  283  740 (S16E54 L=292)  4236    406       12 ( 172/ 602- 377/ 904) -57.1 E62-E44 S24-S05
     14  387  842 (S11E43 L=303)   518     89        2 ( 369/ 793- 415/ 897)  80.5 E44-E40 S13-S07
     15  336  810 (S12E47 L=298)   313     48        0 ( 309/ 792- 359/ 829)   0.0 E49-E45 S13-S11
     16 1685  801 (S17W44 L= 30)   474    106        0 (1634/ 773-1744/ 828)  18.4 W40-W49 S18-S15
  
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.