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20260130 - Filament data for 09 UTC
Available data for 20260130: »09 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  529 1743 (N34E53 L=219)   779     63        0 ( 500/1713- 558/1772) -18.4 E59-E47 N32-N36
      2  811 1713 (N35E27 L=245)   779    150        0 ( 749/1661- 872/1764) -24.8 E33-E20 N31-N38
      3 1146 1452 (N21W02 L=274)   788    259        1 (1045/1390-1245/1542) -24.8 E05-W08 N18-N25
      4  273 1489 (N15E63 L=209)   443     73        0 ( 238/1478- 310/1503)   0.0 E67-E58 N14-N15
      5  639 1351 (N09E28 L=244)   398    100        1 ( 594/1314- 673/1388) -33.7 E31-E25 N06-N10
      6 1831 1271 (N22W55 L=327)   352     46        0 (1808/1250-1852/1290) -14.0 W52-W57 N20-N23
      7 1614 1215 (N14W35 L=307)   477    133        0 (1578/1155-1648/1277)  66.0 W32-W37 N09-N18
      8 1257 1233 (N09W11 L=283)   341    128        1 (1196/1209-1318/1255)   0.0 W07-W14 N08-N10
      9 1737 1197 (N15W45 L=317)   293     37        0 (1713/1176-1759/1218)   0.0 W42-W46 N14-N16
     10  868  893 (S15E08 L=264)  1284    370        2 ( 782/ 732- 951/1041)  74.1 E11-E04 S26-S05
     11  272  800 (S27E52 L=220)   592    133        1 ( 239/ 738- 297/ 860)  41.2 E57-E49 S30-S23
     12  180  784 (S28E65 L=207)   615     63        2 ( 158/ 752- 207/ 816)  18.4 E69-E59 S30-S26
     13 1293  662 (S23W22 L=295)   668    215        0 (1194/ 630-1394/ 706)  32.5 W16-W28 S26-S19
     14  643  648 (S33E21 L=251)   408     92        1 ( 592/ 631- 688/ 672)   0.0 E24-E17 S34-S31
     15 1760  619 (S17W60 L=332)   624     85        1 (1733/ 577-1789/ 658)  68.2 W57-W63 S19-S14
     16 1736  476 (S25W68 L=340)   592     60        2 (1704/ 457-1775/ 495)   4.8 W63-W75 S26-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.