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20250117 - Filament data for 12 UTC
Available data for 20250117: »12 UTC   »13 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  772 1538 (N25E20 L=199)   811    201        1 ( 706/1456- 825/1606) -39.3 E26-E15 N20-N29
      2  304 1406 (N15E54 L=165)  3383    438       12 ( 188/1321- 427/1522)  31.4 E67-E45 N10-N23
      3  183 1300 (N09E65 L=155)  2007    177        2 ( 137/1217- 231/1375) -35.5 E74-E58 N03-N13
      4 1295 1315 (N14W15 L=234)   186     38        1 (1277/1289-1314/1339) -56.3 W13-W15 N12-N15
      5  672 1119 (S01E22 L=197)   253     63        0 ( 657/1079- 688/1154)  76.0 E22-E20 S03-N01
      6  124 1081 (S04E69 L=150)   493     67        1 (  93/1059- 161/1098)  10.3 E74-E63 S05-S03
      7  482  996 (S09E34 L=185)   458    111        2 ( 455/ 955- 504/1041) -68.2 E35-E32 S11-S06
      8  360  977 (S10E43 L=176)   241     53        0 ( 344/ 952- 382/1001)  45.0 E44-E41 S11-S09
      9  947  965 (S09E04 L=215)   236    101        0 ( 904/ 942- 995/ 983) -11.3 E06-E01 S09-S07
     10  389  885 (S16E41 L=178)   968    253        2 ( 325/ 819- 446/ 955)  53.1 E46-E36 S19-S11
     11  229  872 (S17E57 L=163)  2570    414        3 ( 132/ 780- 315/ 949)  24.2 E72-E47 S22-S12
     12 1063  813 (S17W04 L=223)   176     75        0 (1021/ 801-1104/ 828)  21.8 W01-W06 S17-S15
     13 1189  528 (S34W16 L=235)   670    193        3 (1091/ 474-1250/ 565) -14.0 W08-W20 S37-S32
     14 1427  499 (S34W34 L=254)   269     84        1 (1386/ 480-1473/ 519)  26.6 W31-W37 S34-S31
     15  870  474 (S40E07 L=212)   625    172        2 ( 802/ 442- 967/ 506)  14.0 E12-W00 S42-S37
     16 1347  258 (S52W43 L=262)  1710    238        1 (1233/ 231-1449/ 287)   4.1 W29-W57 S54-S49
Download FITS filament maps as tar archive

» All Filament Data of 20250117 ... 		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.

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