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20260306 - Filament data for 13 UTC
Available data for 20260306: »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  669 1792 (N31E50 L=119)   957    130        2 ( 602/1766- 741/1816)  29.1 E55-E44 N28-N33
      2  600 1552 (N13E40 L=129)   287     37        0 ( 582/1526- 621/1577)  90.0 E41-E38 N11-N15
      3  474 1395 (N02E43 L=126)   356     58        0 ( 454/1358- 496/1431) -56.3 E44-E40 N00-N03
      4 1370 1385 (N22W11 L=180)   856      0        0 (1286/1349-1443/1412)  33.7 W06-W16 N17-N24
      5 1219 1287 (N12W04 L=173)   192     99        0 (1197/1248-1233/1320) -63.4 W02-W05 N09-N13
      6 1436 1253 (N16W18 L=187)   221     44        0 (1416/1228-1461/1273)  56.3 W16-W19 N14-N17
      7 1027 1182 (N01E04 L=165)   174     80        0 (1017/1139-1045/1222) -45.0 E04-E01 N00-N03
      8  300 1187 (S13E51 L=118)   275     27        0 ( 276/1171- 321/1200) -11.3 E53-E48 S14-S12
      9 1634 1104 (N13W34 L=203)   244     70        0 (1614/1069-1655/1134) -26.6 W32-W36 N11-N14
     10 1700 1062 (N13W40 L=209)   257     67        1 (1677/1027-1722/1096) -45.0 W37-W42 N11-N14
     11 1918  946 (N15W66 L=235)   571     49        0 (1905/ 914-1933/ 977) -76.0 W63-W68 N12-N16
     12  169  935 (S30E63 L=106)   530     71        0 ( 133/ 919- 206/ 951)   4.8 E69-E57 S30-S28
     13  675  870 (S24E17 L=152)   245    112        0 ( 616/ 853- 729/ 886)   8.1 E20-E13 S24-S22
     14  548  663 (S40E23 L=146)   476     67        0 ( 510/ 639- 595/ 691)  23.2 E26-E19 S41-S36
     15 1386  632 (S19W32 L=201)   296    124        0 (1352/ 593-1425/ 684) -15.9 W28-W36 S20-S16
     16 1482  276 (S35W65 L=234)  1816    143        3 (1417/ 236-1553/ 322)   4.4 W54-W80 S36-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.