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20260304 - Filament data for 08 UTC
Available data for 20260304: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC   »15 UTC   »16 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  914 1544 (N20E20 L=178)   834    202        0 ( 827/1512- 996/1573)  32.0 E23-E14 N16-N22
      2 1372 1395 (N23W11 L=209)   261     88        0 (1338/1355-1397/1435)  80.5 W09-W12 N19-N25
      3  726 1391 (N07E26 L=172)   200     35        1 ( 709/1372- 744/1417)  71.6 E26-E24 N05-N08
      4 1766 1367 (N34W43 L=241)   342     44        1 (1749/1335-1778/1395)  90.0 W41-W44 N31-N36
      5  922 1331 (N07E13 L=185)   287    105        0 ( 875/1313- 965/1364)  45.0 E15-E11 N06-N10
      6 1674 1334 (N28W34 L=232)   301     87        0 (1627/1320-1705/1355)  33.7 W30-W36 N26-N30
      7  585 1318 (S00E33 L=166)   228     66        0 ( 570/1287- 603/1353) -45.0 E34-E31 S02-N01
      8  331  982 (S24E45 L=153)   309     62        1 ( 300/ 962- 363/ 999)  31.0 E47-E42 S25-S22
      9  311  826 (S34E46 L=152)   891    202        0 ( 249/ 739- 381/ 897)  38.7 E54-E39 S40-S28
     10  870  848 (S21E05 L=194)   202     74        0 ( 851/ 818- 900/ 885)  78.7 E05-E03 S22-S17
     11  975  845 (S18W02 L=200)   217     53        2 ( 945/ 815- 996/ 871) -71.6 W00-W03 S19-S16
     12 1514  610 (S17W42 L=240)   259     72        0 (1479/ 596-1556/ 622)  38.7 W39-W44 S18-S14
     13  236  597 (S50E65 L=133)   564     63        0 ( 203/ 578- 269/ 620)   9.0 E75-E56 S51-S48
     14 1664  443 (S20W65 L=263)  2349    314        4 (1521/ 391-1789/ 522)  41.6 W54-W74 S27-S11
     15 1115  458 (S37W23 L=222)   655    175        1 (1037/ 418-1184/ 504)   0.0 W16-W30 S38-S34
     16 1265  421 (S34W35 L=233)   432     59        0 (1240/ 395-1300/ 451)  -9.5 W32-W38 S35-S32
  
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.