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20251218 - Filament data for 07 UTC
Available data for 20251218: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1768 1426 (N17W59 L=178)  1481    186        2 (1695/1363-1833/1493) -38.7 W54-W64 N13-N22
      2 1116 1216 (N09W07 L=126)   945    287        1 (1083/1095-1162/1329)  77.9 W05-W10 N01-N15
      3  126 1233 (N19E72 L= 48)  1852    167        4 (  89/1167- 158/1321)  90.0 E78-E66 N15-N25
      4 1832 1264 (N07W60 L=180)   390      1        0 (1813/1244-1850/1283)  45.0 W58-W62 N05-N08
      5  177 1172 (N15E62 L= 58)   662     74        2 ( 150/1133- 208/1202)  45.0 E65-E57 N12-N16
      6  204 1071 (N08E58 L= 62)   330     38        1 ( 194/1044- 221/1103)  71.6 E58-E55 N06-N10
      7 1939  954 (S12W72 L=191)  2226    172        6 (1908/ 879-1973/1031)  77.5 W66-W80 S16-S07
      8 1147  828 (S14W06 L=125)   395    136        0 (1125/ 761-1165/ 896) -90.0 W04-W07 S18-S09
      9 1809  764 (S23W57 L=176)   768    121        1 (1783/ 709-1839/ 828)  69.4 W54-W59 S26-S18
     10 1572  738 (S23W35 L=154)   440    153        0 (1524/ 714-1635/ 783) -18.4 W30-W39 S24-S19
     11 1177  617 (S27W06 L=126)   599    205        0 (1096/ 563-1268/ 681)  22.6 W00-W12 S30-S23
     12  273  624 (S19E61 L= 59)   695     48        0 ( 250/ 590- 300/ 653)  76.0 E63-E57 S20-S16
     13  948  419 (S39E12 L=107)   336     62        1 ( 921/ 386- 969/ 447)  53.1 E14-E10 S41-S36
     14 1430  369 (S48W29 L=148)   295     70        0 (1395/ 354-1467/ 390) -20.6 W25-W33 S49-S45
     15  681  342 (S42E37 L= 83)   339     63        0 ( 645/ 326- 715/ 357)   0.0 E40-E33 S43-S40
  
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.