logo kso logo uni graz

20130907 - Filament data for 09 UTC
Available data for 20130907: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC   »15 UTC   »16 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1391 1662 (N34W48 L=321)  2574    431        6 (1221/1577-1586/1711) -32.0 W35-W59 N23-N40
      2 1728 1493 (N13W65 L=338)   719     85        1 (1699/1465-1753/1541)  11.3 W60-W70 N11-N15
      3 1431 1423 (N19W36 L=310)   375     73        2 (1403/1389-1466/1458)  18.4 W33-W39 N17-N21
      4  882 1362 (N30E00 L=273)   565    126        0 ( 832/1327- 941/1383) -18.4 E03-W03 N28-N31
      5 1592 1334 (N10W44 L=317)  1003    221        2 (1517/1288-1654/1380) -26.6 W39-W50 N06-N14
      6 1210 1320 (N19W19 L=292)   205     83        0 (1176/1301-1251/1331) -11.3 W16-W21 N18-N20
      7 1775 1279 (N01W57 L=331)   775    107        2 (1740/1254-1825/1315) -29.7 W52-W62 S01-N03
      8 1815  954 (S18W52 L=326)   532     84        1 (1790/ 916-1830/1000)  63.4 W49-W54 S20-S15
      9  201  860 (N13E64 L=210)   626    103        1 ( 173/ 825- 245/ 902) -29.7 E67-E58 N10-N15
     10 1409  768 (S17W17 L=290)   218     39        1 (1382/ 749-1429/ 789)   0.0 W14-W18 S18-S15
     11 1772  721 (S32W46 L=320)   410     88        0 (1748/ 685-1794/ 766)  38.7 W43-W48 S33-S29
     12  209  677 (N02E70 L=203)  1043    149        1 ( 194/ 604- 234/ 736)  36.0 E75-E63 S03-N05
     13  485  685 (S01E42 L=232)   862    186        2 ( 392/ 653- 554/ 708) -14.0 E49-E37 S03-N01
     14  462  476 (S14E53 L=221)  1731    416        2 ( 368/ 348- 574/ 604) -84.3 E58-E48 S24-S04
     15  840  304 (S33E34 L=239)  1952    342        4 ( 774/ 212- 935/ 442)  79.2 E39-E28 S43-S22
  
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.