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20251223 - Filament data for 12 UTC
Available data for 20251223: »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  358 1435 (N28E47 L=  4)  1301    259        1 ( 266/1403- 470/1486)  -7.8 E58-E36 N24-N31
      2 1830 1264 (N09W59 L=110)   435     15        0 (1809/1243-1851/1285) -71.6 W56-W61 N07-N10
      3  437 1186 (N11E37 L= 14)   273     48        0 ( 423/1160- 456/1221)  90.0 E37-E35 N09-N13
      4  392 1124 (N08E40 L= 11)   377     86        2 ( 354/1095- 438/1144)  -8.1 E43-E36 N06-N08
      5  484 1057 (N03E33 L= 18)   501    111        1 ( 436/1023- 514/1109)  45.0 E37-E31 N01-N06
      6  307 1039 (N03E47 L=  4)   440     75        1 ( 286/ 997- 329/1084) -80.5 E49-E45 N00-N06
      7  336  950 (S02E45 L=  6)   292     65        1 ( 299/ 929- 364/ 972) -21.8 E48-E43 S03-N00
      8  209  859 (S06E59 L=352)   710    115        3 ( 177/ 799- 227/ 908)  80.5 E62-E56 S09-S03
      9  403  776 (S13E43 L=  8)  1335    380        3 ( 322/ 629- 492/ 907)  43.3 E52-E34 S21-S05
     10  257  776 (S12E56 L=355)  1077    113        5 ( 233/ 709- 284/ 843)  69.4 E59-E53 S15-S07
     11  713  723 (S18E21 L= 30)   210     88        0 ( 670/ 702- 755/ 746)   9.5 E24-E18 S19-S16
     12  855  636 (S24E13 L= 38)   861    220        1 ( 751/ 572- 945/ 690)  21.8 E21-E06 S27-S21
     13 1843  620 (S30W68 L=119)   554     65        1 (1806/ 604-1879/ 638)   4.8 W62-W75 S31-S28
     14  245  534 (S26E70 L=341)  1165    117        1 ( 203/ 516- 293/ 570)   0.0 E82-E62 S27-S24
     15 1623  423 (S43W50 L=101)   680     85        2 (1585/ 398-1658/ 466)  59.0 W45-W54 S45-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.