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20260826 - Filament data for 09 UTC
Available data for 20260826: »05 UTC   »06 UTC   »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 1065 1643 (N44W20 L= 65)   277     12        0 (1044/1624-1084/1663)  11.3 W17-W22 N42-N45
      2 1433 1521 (N27W40 L= 85)   293     95        0 (1393/1496-1481/1535)  -8.1 W36-W43 N25-N27
      3 1324 1396 (N22W27 L= 72)   388    115        0 (1269/1379-1379/1411) -15.9 W23-W30 N20-N23
      4 1605 1311 (N10W43 L= 88)  1320    315        1 (1493/1206-1702/1391) -59.0 W37-W48 N02-N17
      5  246 1266 (N34E58 L=347)  2749    271        4 ( 156/1153- 307/1369) -22.4 E84-E48 N26-N40
      6 1320 1140 (N08W20 L= 64)   206     71        0 (1283/1125-1357/1153)   0.0 W17-W22 N06-N08
      7 1203 1052 (N05W11 L= 55)   537    165        2 (1141/1003-1247/1116)  35.5 W06-W14 N03-N08
      8  320  991 (N17E48 L=356)   963    223        0 ( 257/ 918- 401/1065) -42.3 E54-E42 N11-N21
      9  241  975 (N16E57 L=348)   333     97        0 ( 217/ 955- 268/1006) -31.0 E59-E53 N15-N18
     10 1030  962 (N03E01 L= 44)   196     97        0 ( 992/ 933-1063/ 980) -56.3 E03-W00 N01-N04
     11  575  903 (N08E30 L= 15)   726    140        3 ( 542/ 842- 608/ 975)  54.5 E32-E26 N04-N11
     12  312  709 (S00E55 L=350)   938    207        0 ( 253/ 655- 400/ 738) -18.4 E61-E48 S04-N01
     13  909  579 (S17E16 L= 28)   338     83        2 ( 891/ 536- 928/ 625)  71.6 E17-E14 S20-S14
     14  443  412 (S21E58 L=347)   824    132        1 ( 393/ 393- 507/ 435)   0.0 E63-E49 S22-S19
     15  607  264 (S35E55 L=349)  1148    160        1 ( 537/ 229- 686/ 291)  -3.0 E70-E45 S37-S33
  
Download FITS filament maps as tar archive

» All Filament Data of 20260826 ...
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.