logo kso logo uni graz

20260208 - Filament data for 10 UTC
Available data for 20260208: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  550 1806 (N37E60 L= 93)   608     61        1 ( 536/1767- 561/1841) -25.0 E69-E54 N33-N40
      2  994 1608 (N28E13 L=140)   453    128        0 ( 930/1570-1037/1639)  -7.1 E17-E09 N26-N30
      3  921 1271 (N06E10 L=143)  1438    329        0 ( 781/1178-1047/1349) -18.4 E19-E01 N02-N08
      4 1490 1262 (N16W24 L=177)   298     97        0 (1442/1240-1535/1283)  33.7 W21-W27 N13-N17
      5 1584 1203 (N14W31 L=184)   316     45        1 (1557/1174-1601/1235)  90.0 W29-W32 N12-N16
      6 1766 1173 (N17W46 L=199)  1196    146        4 (1702/1118-1827/1216) -15.3 W40-W52 N14-N18
      7  254 1093 (S13E53 L=100)   725    198        1 ( 197/1013- 301/1174)  55.0 E59-E49 S17-S07
      8 1703 1078 (N09W42 L=195)   499    148        0 (1684/1025-1743/1152) -50.2 W39-W45 N07-N13
      9  367 1039 (S15E43 L=110)   444     98        0 ( 317/1007- 405/1075)  39.8 E46-E39 S17-S12
     10  335  757 (S32E46 L=107)  2567    436        3 ( 159/ 621- 500/ 856)  17.1 E82-E30 S41-S24
     11 1200  809 (S16W14 L=167)   212     80        0 (1154/ 796-1240/ 821)  11.3 W11-W16 S16-S14
     12 1394  688 (S19W29 L=182)   365    117        1 (1372/ 654-1439/ 739) -31.0 W26-W32 S20-S16
     13 1025  578 (S33W09 L=162)   841    224        2 ( 948/ 499-1131/ 640)  50.7 W04-W14 S38-S27
     14 1554  457 (S29W51 L=204)   500    108        2 (1495/ 440-1607/ 475)  20.6 W46-W56 S30-S26
     15 1675  414 (S28W68 L=221)   450     53        0 (1643/ 398-1702/ 434)  31.0 W63-W70 S28-S25
  
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.