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20260901 - Filament data for 08 UTC
Available data for 20260901: »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  627 1577 (N51E18 L=308)   260     71        0 ( 606/1549- 658/1607)  31.0 E19-E14 N48-N52
      2 1157 1533 (N34W22 L=348)   833    227        2 (1036/1487-1240/1566) -28.3 W14-W27 N29-N38
      3  530 1537 (N50E28 L=298)   293     36        0 ( 508/1517- 554/1556)  11.3 E30-E25 N48-N51
      4  817 1372 (N32E05 L=321)   755    176        1 ( 754/1312- 882/1448) -70.0 E08-E01 N27-N38
      5 1388 1385 (N19W31 L=357)  1137    259        1 (1283/1320-1495/1434) -42.3 W25-W36 N12-N24
      6 1686 1321 (N08W50 L= 16)  1237    220        3 (1635/1216-1718/1396)  38.7 W43-W55 N02-N12
      7  208 1080 (N24E60 L=266)  1095    143        2 ( 145/1050- 280/1118)  -9.0 E70-E51 N22-N27
      8 1810 1034 (S12W53 L= 19)   499     49        1 (1787/1007-1831/1058) -76.0 W50-W55 S13-S09
      9  489  896 (N10E36 L=290)   278     77        1 ( 462/ 853- 509/ 926) -78.7 E37-E34 N06-N11
     10  176  856 (N11E67 L=259)   430     51        1 ( 162/ 829- 196/ 884) -90.0 E68-E64 N09-N12
     11  889  823 (S02E12 L=314)   701    233        2 ( 825/ 733- 982/ 875)  21.8 E16-E06 S06-N00
     12 1440  706 (S21W18 L=344)  1275    402        2 (1280/ 603-1614/ 792)   6.6 W06-W32 S23-S18
     13 1439  500 (S35W16 L=342)  1693    327        3 (1300/ 404-1571/ 572)   7.4 W03-W27 S39-S33
     14  752  482 (S20E30 L=296)   266    100        2 ( 720/ 434- 773/ 528)  74.1 E31-E28 S23-S16
     15  512  334 (S26E58 L=268)   548     51        1 ( 494/ 301- 536/ 362)  16.7 E63-E53 S28-S24
Download FITS filament maps as tar archive

» All Filament Data of 20260901 ... 		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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