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20260211 - Filament data for 12 UTC
Available data for 20260211: »12 UTC   »13 UTC   »14 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  735 1836 (N41E45 L= 68)   463     64        0 ( 718/1804- 761/1860) -45.0 E48-E41 N38-N43
      2 1385 1564 (N33W13 L=126)   479     82        2 (1358/1514-1411/1602) -81.9 W11-W15 N29-N36
      3  443 1498 (N12E47 L= 65)   725    134        3 ( 405/1436- 479/1573) -77.5 E49-E45 N08-N17
      4 1517 1500 (N32W24 L=136)   735    129        1 (1472/1460-1572/1541)  26.6 W20-W28 N28-N35
      5  377 1451 (N09E51 L= 61)   390    106        1 ( 357/1417- 397/1501) -80.5 E52-E48 N06-N12
      6 1617 1403 (N28W32 L=145)   558     84        2 (1590/1366-1648/1439)  68.2 W29-W34 N25-N30
      7  334 1335 (N01E51 L= 62)   323     80        0 ( 299/1320- 375/1359) -15.9 E54-E47 N00-N02
      8  181 1124 (S12E62 L= 51)  1224    135        3 ( 126/1082- 253/1157)  19.7 E69-E54 S14-S09
      9  211 1030 (S18E58 L= 55)   357     49        1 ( 189/ 999- 235/1051)  56.3 E60-E54 S19-S16
     10  364  956 (S21E42 L= 70)   257    104        0 ( 350/ 905- 382/1001)  90.0 E43-E40 S23-S17
     11 1762  739 (S07W55 L=168)   522    113        2 (1718/ 693-1800/ 770)  33.7 W51-W59 S09-S04
     12  876  656 (S31E02 L=110)  1740    467        3 ( 670/ 590-1099/ 729)  31.6 E16-W10 S38-S22
     13 1724  616 (S15W57 L=170)   495    150        1 (1667/ 587-1777/ 665)  54.5 W52-W60 S17-S10
     14 1423  584 (S24W35 L=148)   752    237        1 (1322/ 560-1533/ 613)  28.3 W27-W42 S26-S19
     15 1769  508 (S19W70 L=183)   513     74        1 (1742/ 484-1785/ 540)  90.0 W67-W73 S20-S16
     16 1398  352 (S38W47 L=159)  2544    404        7 (1220/ 253-1554/ 462)  64.5 W39-W54 S48-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.