logo kso logo uni graz

20141012 - Filament data for 11 UTC
Available data for 20141012: »06 UTC   »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 1665 1515 (N13W58 L= 91)   530     90        2 (1626/1482-1691/1555)  68.2 W54-W59 N10-N15
      2 1211 1341 (N18W20 L= 53)   680    219        2 (1113/1316-1323/1380) -28.6 W14-W25 N14-N21
      3 1622 1278 (N02W43 L= 76)   758    234        1 (1543/1226-1698/1331)   0.0 W35-W51 N01-N03
      4 1847 1125 (S13W57 L= 90)   397    100        1 (1834/1083-1864/1176)  45.0 W54-W59 S15-S10
      5  760 1076 (N16E14 L= 20)   195     74        0 ( 721/1054- 798/1090) -45.0 E15-E11 N13-N17
      6 1689 1043 (S12W41 L= 74)   308     61        2 (1664/1012-1709/1071)  56.3 W38-W42 S13-S10
      7 1300  951 (S05W13 L= 46)   962    340        0 (1230/ 886-1442/1070) -56.3 W10-W21 S11-N02
      8  363  915 (N16E44 L=349)   264     53        0 ( 342/ 893- 388/ 941) -56.3 E45-E42 N14-N17
      9 1808  825 (S29W47 L= 80)  1740    250        1 (1719/ 756-1859/ 925)  19.7 W37-W53 S32-S24
     10 1425  680 (S25W14 L= 47)   955    288        3 (1387/ 531-1462/ 790)  61.9 W08-W17 S33-S18
     11  344  713 (N05E52 L=341)   672    159        1 ( 284/ 674- 413/ 748) -33.7 E56-E47 N01-N07
     12 1039  652 (S15E09 L= 24)   287     83        0 ( 996/ 630-1078/ 672) -21.8 E12-E07 S16-S13
     13 1074  598 (S19E09 L= 24)   240     61        0 (1049/ 568-1093/ 631)  36.9 E11-E07 S20-S17
     14  298  478 (S09E71 L=322)   949    120        1 ( 269/ 440- 322/ 508) -68.2 E74-E67 S11-S06
     15 1091  405 (S32E15 L= 18)   246     45        0 (1072/ 388-1113/ 432) -90.0 E16-E13 S33-S29
  
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.