logo kso logo uni graz

20260612 - Filament data for 12 UTC
Available data for 20260612: »06 UTC   »07 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  537 1608 (N30E47 L=268)  1618    247        0 ( 506/1498- 570/1723) -35.5 E61-E39 N23-N38
      2 1601 1490 (N38W39 L=354)   429     55        1 (1572/1468-1635/1505)   0.0 W36-W43 N36-N39
      3 1206 1470 (N31W06 L=321)   679    249        1 (1147/1392-1291/1503)  37.9 W02-W12 N24-N33
      4  702 1428 (N21E27 L=288)   421    134        0 ( 657/1381- 752/1458)  51.3 E29-E23 N17-N23
      5  437 1313 (N10E43 L=272)   264     58        1 ( 425/1281- 454/1345)  76.0 E44-E41 N08-N12
      6 1835 1287 (N27W62 L= 17)   505     72        0 (1804/1262-1866/1306) -12.5 W57-W66 N25-N28
      7  455 1174 (N02E39 L=276)   663    171        0 ( 419/1097- 500/1241) -36.9 E42-E34 S01-N06
      8 1786 1184 (N20W53 L=  8)   457     88        1 (1750/1151-1809/1228)  68.2 W49-W56 N17-N22
      9  225 1101 (S05E58 L=257)   844    174        2 ( 198/1022- 260/1178) -60.9 E62-E53 S09-N00
     10  274  878 (S18E52 L=263)   560     83        2 ( 252/ 831- 303/ 910)  50.2 E54-E48 S21-S15
     11 1308  856 (S06W19 L=334)   488    179        0 (1232/ 812-1379/ 884)   0.0 W14-W24 S07-S04
     12  662  672 (S26E19 L=296)   426     75        2 ( 624/ 644- 690/ 707)  31.0 E22-E17 S27-S23
     13 1541  508 (S25W45 L=  0)   414    119        0 (1519/ 476-1572/ 551) -68.2 W43-W49 S26-S21
     14  956  444 (S37W04 L=319)   295     53        0 ( 920/ 431- 988/ 457)  21.8 W01-W06 S38-S36
     15 1147  405 (S37W19 L=334)   406     79        1 (1113/ 381-1170/ 443) -45.0 W16-W21 S39-S34
  
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.