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20260303 - Filament data for 10 UTC
Available data for 20260303: »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  744 1594 (N19E32 L=178)  1030    204        2 ( 658/1556- 828/1631)  15.3 E36-E25 N15-N22
      2  562 1405 (N04E37 L=173)   624    121        2 ( 531/1342- 587/1465) -54.5 E38-E33 N00-N08
      3 1041 1430 (N16E09 L=201)   322     92        1 (1008/1405-1078/1457)  53.1 E10-E06 N13-N18
      4  744 1402 (N08E25 L=185)   371    111        0 ( 697/1380- 785/1438)  45.0 E28-E23 N06-N10
      5 1534 1404 (N28W22 L=232)   277     93        0 (1482/1389-1574/1425)  33.7 W18-W24 N26-N30
      6  427 1292 (S05E43 L=167)   870    283        0 ( 403/1175- 451/1424) -63.4 E47-E39 S11-N03
      7  217 1025 (S23E57 L=153)   552    127        0 ( 168/ 990- 261/1073)  31.0 E63-E52 S25-S19
      8  123 1005 (S25E71 L=140)   631     99        0 ( 102/ 972- 157/1046) -29.7 E74-E64 S27-S22
      9  701  982 (S17E18 L=192)   709    314        3 ( 619/ 881- 757/1044) -45.0 E23-E14 S22-S13
     10  805  916 (S18E10 L=200)   378    157        1 ( 773/ 858- 848/ 988) -50.2 E11-E06 S21-S14
     11 1265  734 (S17W21 L=231)   228     32        0 (1245/ 712-1283/ 757)  71.6 W20-W22 S18-S15
     12 1582  507 (S20W52 L=262)  1839    353        1 (1410/ 450-1719/ 583)  36.4 W41-W60 S27-S12
     13 1038  504 (S36W16 L=226)   209     23        0 (1019/ 487-1055/ 525)  71.6 W14-W17 S37-S34
     14 1142  484 (S35W24 L=234)   431     88        0 (1103/ 461-1191/ 509)   0.0 W20-W27 S35-S33
     15 1367  304 (S38W52 L=262)   334     44        0 (1348/ 286-1394/ 327)  14.0 W49-W54 S39-S36
  
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.