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20260221 - Filament data for 10 UTC
Available data for 20260221: »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 1393 1556 (N33W11 L=353)   305     83        1 (1369/1519-1420/1593)  74.1 W10-W13 N30-N37
      2  636 1495 (N13E34 L=308)   876    168        3 ( 597/1423- 684/1567)  90.0 E35-E32 N07-N17
      3 1242 1518 (N27W02 L=344)   303     65        1 (1211/1492-1274/1541)   0.0 W00-W04 N25-N28
      4  354 1481 (N08E55 L=286)   391     84        0 ( 312/1454- 389/1497)  -5.7 E60-E50 N06-N08
      5  294 1274 (S05E53 L=288)   837    173        2 ( 260/1196- 350/1317)  58.0 E55-E49 S10-S02
      6 1725 1107 (N14W42 L= 24)   917    258        2 (1650/1012-1761/1207) -36.9 W34-W46 N09-N18
      7  577 1172 (S07E29 L=312)   204     69        0 ( 560/1132- 598/1205)  76.0 E30-E28 S09-S05
      8  338  963 (S23E44 L=297)  1228    368        2 ( 232/ 856- 462/1089)  43.4 E55-E35 S30-S13
      9  704  933 (S19E17 L=325)   196    100        1 ( 664/ 917- 760/ 946)  18.4 E19-E13 S20-S17
     10 1346  916 (S06W21 L=  2)   270     74        0 (1303/ 891-1376/ 942) -11.3 W17-W22 S07-S04
     11 1631  800 (S05W42 L= 24)   259     82        1 (1613/ 759-1645/ 840) -78.7 W41-W43 S07-S02
     12 1371  676 (S18W29 L= 11)   982    346        1 (1213/ 608-1506/ 765)  47.0 W21-W35 S25-S10
     13 1750  659 (S09W58 L= 40)   636    139        0 (1712/ 604-1791/ 721)  82.9 W56-W60 S12-S04
     14 1795  556 (S13W70 L= 52)  1042     72        2 (1761/ 526-1831/ 581)   9.5 W64-W76 S14-S10
     15 1569  485 (S24W52 L= 34)   486    136        1 (1530/ 437-1618/ 538)  81.9 W50-W55 S26-S19
     16 1631  458 (S23W60 L= 41)   886    177        1 (1555/ 410-1697/ 512)  56.3 W55-W63 S27-S18
  
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.