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20251208 - Filament data for 12 UTC
Available data for 20251208: »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 1242 1681 (N38W27 L=276)  1140    195        6 (1152/1616-1324/1720) -45.0 W21-W31 N32-N41
      2  814 1375 (N23E09 L=240)   413    107        1 ( 749/1357- 874/1397) -20.6 E12-E04 N21-N24
      3 1826 1267 (N04W60 L=308)   469      0        0 (1799/1244-1850/1290)   9.5 W56-W62 N02-N05
      4  941 1232 (N13E02 L=246)   292     89        0 ( 915/1190- 971/1273) -68.2 E03-W00 N10-N15
      5 1317 1197 (N06W20 L=268)   291    128        0 (1257/1180-1376/1223)  -7.1 W15-W23 N05-N07
      6  361 1090 (N12E42 L=206)   396     94        1 ( 346/1045- 385/1146) -80.5 E42-E39 N09-N15
      7 1677  984 (S10W41 L=290)   774    148        4 (1626/ 947-1732/1022) -26.6 W37-W45 S12-S07
      8 1580  929 (S12W33 L=282)   274    147        0 (1529/ 894-1612/ 955)  21.8 W29-W35 S14-S10
      9 1666  879 (S17W40 L=288)   541    123        2 (1618/ 846-1725/ 908)   6.3 W36-W45 S18-S15
     10 1281  793 (S17W13 L=261)   920    253        2 (1244/ 674-1322/ 906) -85.9 W10-W14 S24-S10
     11  694  807 (S09E23 L=226)   194     60        1 ( 668/ 779- 719/ 836)  33.7 E24-E20 S09-S07
     12 1495  722 (S24W27 L=275)   259     70        0 (1474/ 689-1521/ 752)  45.0 W25-W28 S26-S22
     13  798  676 (S18E18 L=230)   217     62        1 ( 776/ 645- 825/ 700)  45.0 E19-E16 S19-S16
     14  760  522 (S27E25 L=224)   447    155        1 ( 718/ 454- 794/ 584) -83.7 E25-E23 S31-S22
     15  966  531 (S29E11 L=238)   417     72        3 ( 930/ 499-1001/ 564)  21.8 E13-E08 S31-S27
     16  447  384 (S32E57 L=191)  1789    160        5 ( 370/ 326- 514/ 426) -31.0 E64-E51 S36-S27
  
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.