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20140514 - Filament data for 12 UTC
Available data for 20140514: »04 UTC   »05 UTC   »06 UTC   »07 UTC   »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  526 1682 (N26E54 L=175)   748    174        1 ( 479/1641- 557/1709)  -5.7 E59-E49 N23-N27
      2  558 1553 (N18E44 L=185)   284     89        1 ( 546/1504- 569/1594) -45.0 E46-E41 N15-N20
      3  839 1434 (N17E21 L=208)   209     72        1 ( 828/1394- 856/1467) -68.2 E22-E19 N14-N19
      4 1187 1380 (N22W01 L=230)   345    117        1 (1176/1321-1201/1433) -74.1 W00-W02 N18-N25
      5 1469 1321 (N25W21 L=250)   425     75        0 (1432/1285-1505/1354) -15.9 W17-W24 N23-N27
      6 1070 1189 (N08E01 L=228)   302     66        1 (1040/1149-1094/1218) -26.6 E03-W01 N05-N09
      7 1121 1136 (N06W03 L=232)   247     83        2 (1109/1081-1136/1177) -71.6 W01-W04 N02-N08
      8 1401 1091 (N10W21 L=250)   206     49        1 (1375/1077-1425/1116)  33.7 W19-W22 N08-N11
      9 1610 1015 (N11W36 L=265)   543    146        2 (1559/ 971-1656/1074) -18.4 W31-W40 N08-N13
     10  450  842 (S26E33 L=196)   619    305       -1 ( 385/ 798- 485/ 931)  66.0 E38-E30 S29-S20
     11  423  875 (S25E36 L=193)   299     57       -1 ( 389/ 835- 457/ 898)  51.3 E38-E33 S27-S22
     12 1566  592 (S14W46 L=275)   793    130        2 (1519/ 561-1616/ 634)  50.2 W42-W49 S16-S10
     13  932  569 (S32W06 L=235)   318     64        1 ( 905/ 547- 972/ 599)  26.6 W04-W08 S33-S30
     14 1429  405 (S29W46 L=275)   611    100        2 (1402/ 376-1467/ 435)   0.0 W42-W49 S31-S27
     15 1157  301 (S44W34 L=263)   450     54        0 (1139/ 273-1176/ 331) -38.7 W31-W37 S46-S42
     16 1210  255 (S46W42 L=271)   737    107        2 (1169/ 224-1243/ 291)  90.0 W39-W45 S48-S42
  
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.