logo kso logo uni graz

20260403 - Filament data for 12 UTC
Available data for 20260403: »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1248 1746 (N45E11 L=149)   411     81        0 (1215/1728-1284/1761)  21.8 E13-E08 N42-N46
      2 1431 1667 (N46W06 L=166)   362     81        0 (1400/1649-1472/1687)  33.7 W03-W09 N43-N47
      3  789 1528 (N15E28 L=132)   304     83        1 ( 761/1508- 831/1558)   0.0 E30-E25 N13-N17
      4 1034 1406 (N15E10 L=150)   516    295        0 ( 993/1283-1076/1537) -49.8 E16-E05 N08-N21
      5 1546 1358 (N28W22 L=182)   559     91        0 (1498/1322-1578/1392)  -8.1 W17-W24 N26-N29
      6  655 1306 (S01E29 L=132)   300     82        1 ( 626/1279- 692/1340) -11.3 E30-E25 S01-N01
      7  494 1033 (S20E32 L=129)   240     44        0 ( 479/1003- 513/1060)  90.0 E32-E30 S21-S17
      8 1414  978 (N02W23 L=183)   261     77        0 (1385/ 958-1449/1001)  33.7 W20-W24 N01-N03
      9  624  905 (S24E20 L=140)   280     63        1 ( 587/ 885- 665/ 920)  21.8 E22-E17 S25-S22
     10  698  764 (S30E12 L=149)   772    244        0 ( 583/ 729- 821/ 791)  31.0 E19-E04 S34-S25
     11 1026  594 (S30W14 L=174)   708    326        0 ( 938/ 497-1131/ 691)  76.8 W11-W16 S38-S21
     12 1240  654 (S20W24 L=184)   296     86        0 (1202/ 629-1286/ 672)  59.0 W22-W26 S22-S17
     13 1297  562 (S23W31 L=192)   304     81        1 (1262/ 531-1330/ 588)  78.7 W29-W32 S25-S20
     14 1071  460 (S36W23 L=183)   374    100        0 (1025/ 432-1107/ 497)  81.9 W20-W24 S39-S32
     15 1208  310 (S40W42 L=203)   478    103        0 (1180/ 280-1254/ 348)  -5.7 W37-W47 S41-S38
  
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.