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20260104 - Filament data for 09 UTC
Available data for 20260104: »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 1334 1752 (N46W27 L=281)   606     96        1 (1286/1734-1391/1769)   0.0 W21-W31 N44-N47
      2 1122 1640 (N36W07 L=261)   927    177        1 (1046/1585-1185/1685) -37.9 W01-W10 N32-N39
      3 1424 1489 (N26W27 L=281)   266     95        0 (1381/1464-1466/1505) -18.4 W23-W29 N24-N26
      4  230 1402 (N21E62 L=193)   570     85        0 ( 202/1368- 263/1438) -26.6 E67-E56 N18-N23
      5  304 1210 (N08E49 L=206)   769     92        0 ( 263/1181- 352/1245) -26.6 E52-E44 N06-N10
      6 1555  977 (S05W33 L=288)   300    110        0 (1510/ 929-1595/1006)  39.8 W30-W36 S08-S03
      7 1576  920 (S09W35 L=289)   241     27        0 (1552/ 900-1599/ 939)  33.7 W33-W36 S09-S07
      8 1608  840 (S13W38 L=293)  1186    261        6 (1544/ 727-1662/ 930)  72.9 W34-W41 S20-S07
      9 1156  750 (S20W08 L=263)   961    344        1 (1127/ 604-1182/ 901)  86.8 W06-W10 S28-S10
     10  879  789 (S17E09 L=245)   371    119        1 ( 828/ 745- 922/ 833)  45.0 E12-E06 S20-S14
     11  275  722 (S21E55 L=199)  1266    214        3 ( 194/ 645- 325/ 776) -42.0 E63-E49 S25-S16
     12  262  581 (S29E64 L=191)  1706    103        3 ( 224/ 533- 303/ 637)  35.0 E69-E57 S32-S25
     13 1299  315 (S50W27 L=281)   474     78        0 (1259/ 287-1336/ 342) -16.7 W21-W31 S52-S47
     14 1294  197 (S61W36 L=291)   410     31        1 (1272/ 176-1312/ 221) -35.5 W32-W41 S63-S58
     15  684  162 (S65E55 L=199)   635     60        0 ( 660/ 137- 708/ 187)   9.2 E74-E43 S67-S62
  
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.