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20130720 - Filament data for 09 UTC
Available data for 20130720: »05 UTC   »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  346 1348 (N28E51 L=150)   523    109        2 ( 296/1325- 404/1371)  -4.4 E57-E44 N26-N29
      2 1715 1306 (N16W53 L=255)   515    166        0 (1648/1248-1761/1361) -53.1 W48-W56 N12-N20
      3  951 1221 (N17E03 L=198)   518    272        3 ( 862/1184-1083/1279) -24.8 E09-W04 N14-N21
      4  207 1085 (N11E62 L=140)   719    156        1 ( 194/1022- 232/1154) -76.0 E64-E58 N07-N15
      5  929  939 (N00E06 L=195)   261     60        1 ( 897/ 913- 959/ 958)  14.0 E08-E04 S01-N01
      6 1435  913 (S05W25 L=227)   763    181        2 (1355/ 885-1526/ 945) -10.3 W20-W31 S06-S02
      7 1720  848 (S12W48 L=249)   436     73        1 (1688/ 825-1764/ 867) -20.6 W44-W52 S13-S10
      8  308  747 (S10E54 L=148)   637    100        2 ( 285/ 693- 339/ 789)  71.6 E56-E50 S13-S07
      9  259  727 (S11E60 L=142)   473     50        1 ( 241/ 697- 277/ 760) -76.0 E62-E58 S13-S09
     10 1338  730 (S16W18 L=220)   230    103        1 (1289/ 703-1382/ 751) -26.6 W15-W21 S17-S14
     11 1351  626 (S23W19 L=221)   398    143        1 (1307/ 580-1379/ 682)  56.3 W16-W21 S25-S19
     12  841  643 (S18E14 L=187)   352    104        1 ( 810/ 610- 891/ 678)  26.6 E16-E10 S20-S15
     13 1474  559 (S29W29 L=231)   359    111        1 (1455/ 509-1489/ 610) -81.9 W27-W31 S32-S25
     14  729  505 (S27E24 L=177)   623    110        2 ( 695/ 464- 777/ 539)  35.5 E28-E21 S30-S24
     15  683  388 (S36E32 L=169)   550     99        1 ( 666/ 332- 712/ 431)  63.4 E35-E28 S40-S32
     16  665  251 (S49E45 L=157)   532     77        0 ( 647/ 229- 699/ 283) -63.4 E49-E41 S51-S45
  
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.