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20251228 - Filament data for 10 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  804 1666 (N40E15 L=332)   240     41        0 ( 782/1647- 830/1683)  26.6 E16-E12 N38-N40
      2 1077 1574 (N32W06 L=352)   822    202        1 ( 976/1547-1176/1594)   0.0 E01-W12 N29-N33
      3 1292 1536 (N28W20 L=  6)   306     48        1 (1267/1506-1313/1559) -63.4 W18-W21 N26-N30
      4  253 1425 (N25E59 L=287)  1846    198        5 ( 209/1369- 305/1485)  35.5 E65-E51 N21-N29
      5 1821 1272 (N11W58 L= 44)   361     45        1 (1803/1246-1841/1298)  36.9 W55-W60 N09-N12
      6  215 1244 (N14E58 L=288)   715    134        4 ( 179/1214- 270/1296) -18.4 E63-E51 N12-N17
      7 1372 1232 (N09W22 L=  8)   657    108        2 (1332/1176-1421/1274)  63.4 W19-W24 N05-N11
      8 1304 1168 (N05W17 L=  3)   209     40        0 (1281/1140-1326/1191) -56.3 W15-W18 N03-N06
      9  237 1072 (N04E54 L=292)   600    105        0 ( 202/1040- 274/1112)  26.6 E57-E50 N01-N05
     10 1742  934 (S09W48 L= 34)   570     76        1 (1709/ 902-1778/ 974)  38.7 W45-W51 S11-S06
     11 1797  854 (S14W54 L= 40)   606    115        0 (1772/ 797-1819/ 906)  81.9 W51-W56 S17-S10
     12  209  879 (S08E59 L=288)   465     51        2 ( 180/ 860- 240/ 900)  -9.5 E62-E55 S08-S06
     13  384  820 (S12E43 L=303)   294     53        1 ( 366/ 791- 403/ 850)  56.3 E44-E41 S13-S10
     14  288  716 (S18E54 L=292)  3503    323       11 ( 207/ 603- 349/ 844) -68.2 E61-E47 S24-S09
     15  331  808 (S13E48 L=298)   345     54        0 ( 304/ 782- 355/ 828) -33.7 E50-E45 S14-S11
     16 1676  800 (S17W43 L= 30)   471    128        0 (1611/ 773-1735/ 827)  16.7 W38-W48 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.