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20260302 - Filament data for 10 UTC
Available data for 20260302: »10 UTC   »11 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  476 1564 (N13E49 L=174)  1856    388        6 ( 361/1443- 617/1677)  62.1 E56-E43 N03-N22
      2  643 1597 (N18E39 L=185)   467    109        1 ( 622/1550- 660/1649) -50.2 E42-E36 N14-N20
      3  312 1567 (N11E66 L=157)  1234      0        0 ( 270/1520- 356/1604)  50.2 E72-E61 N07-N13
      4  854 1524 (N17E22 L=201)   411    116        1 ( 818/1479- 902/1550)  68.2 E24-E20 N14-N19
      5  562 1461 (N08E38 L=185)   435    118        1 ( 524/1435- 598/1511)  63.4 E41-E36 N05-N11
      6 1825 1269 (N29W50 L=273)   460     76        1 (1805/1228-1841/1302) -78.7 W47-W51 N26-N31
      7  482 1089 (S15E34 L=189)   293     93        1 ( 440/1076- 525/1103)   9.5 E37-E31 S16-S13
      8  538 1039 (S17E29 L=194)   296    117        1 ( 512/ 994- 560/1096)  90.0 E30-E27 S19-S13
      9  620  980 (S18E23 L=200)   486    181        4 ( 598/ 903- 663/1062) -71.6 E25-E19 S22-S13
     10 1492  599 (S18W41 L=264)  1186    305        1 (1359/ 534-1616/ 675)  51.3 W34-W46 S25-S10
     11  729  594 (S39E08 L=215)   302     59        1 ( 706/ 562- 745/ 627) -63.4 E09-E06 S41-S36
     12  874  569 (S37W03 L=226)   215     44        0 ( 854/ 551- 898/ 590)   0.0 W01-W04 S38-S35
     13  987  559 (S34W11 L=234)   328     76        0 ( 959/ 539-1028/ 588)   0.0 W08-W13 S35-S33
     14 1657  534 (S16W57 L=280)   567    134        1 (1602/ 493-1711/ 578)  63.4 W53-W59 S20-S12
     15 1305  372 (S36W41 L=264)   477     91        1 (1260/ 357-1356/ 389)  33.7 W37-W45 S38-S34
     16 1560  329 (S30W66 L=289)  2514    219        6 (1470/ 302-1653/ 364)  32.7 W54-W79 S33-S24
  
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.