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20260328 - Filament data for 11 UTC
Available data for 20260328: »08 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  884 1756 (N32E34 L=206)   816    127        0 ( 838/1709- 932/1805) -83.7 E36-E31 N28-N37
      2  574 1758 (N25E57 L=183)   418     53        0 ( 562/1723- 585/1789) -29.7 E62-E54 N22-N26
      3  425 1630 (N13E60 L=180)  2902    307        6 ( 371/1528- 488/1702) -85.6 E67-E53 N05-N18
      4  500 1567 (N11E49 L=191)   983    161        1 ( 443/1500- 567/1623)  66.0 E53-E46 N05-N14
      5  668 1547 (N13E36 L=204)   564    126        0 ( 636/1487- 710/1608) -33.7 E40-E31 N10-N16
      6 1220 1384 (N19W01 L=241)   271     81        1 (1199/1341-1242/1420) -68.2 E01-W02 N15-N20
      7  197 1022 (S27E59 L=181)  2456    246        9 ( 145/ 938- 237/1119)  53.1 E67-E54 S32-S20
      8  285  998 (S26E49 L=191)   582    139        0 ( 259/ 931- 314/1061)  69.4 E51-E46 S30-S22
      9  831  877 (S20E07 L=233)   363     92        2 ( 806/ 826- 862/ 913) -78.7 E08-E04 S22-S17
     10 1809  845 (N08W55 L=295)   543     81        0 (1785/ 802-1832/ 888) -23.2 W51-W59 N06-N09
     11  872  780 (S24E02 L=238)   206     63        0 ( 851/ 751- 900/ 808) -18.4 E03-W00 S25-S22
     12  388  718 (S41E37 L=204)   397     55        1 ( 353/ 701- 422/ 747)   7.1 E40-E32 S42-S39
     13 1202  660 (S21W21 L=261)   813    218        1 (1098/ 630-1310/ 695)  42.0 W15-W26 S25-S16
     14  631  656 (S38E14 L=226)   738    146        1 ( 559/ 636- 700/ 692)  15.3 E19-E08 S40-S35
     15 1746  672 (S03W57 L=297)   378     55        1 (1725/ 648-1778/ 689)  45.0 W54-W59 S04-S01
     16 1521  419 (S23W55 L=295)  1233    250        1 (1409/ 400-1632/ 444)  31.0 W46-W64 S27-S18
  
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.