logo kso logo uni graz

20150103 - Filament data for 12 UTC
Available data for 20150103: »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  793 1541 (N29E16 L=  3)   791    204        2 ( 714/1469- 873/1596) -36.9 E21-E09 N24-N33
      2 1508 1356 (N17W32 L= 50)   263     74        0 (1479/1323-1535/1378)  45.0 W29-W33 N14-N18
      3  152 1306 (N16E67 L=311)   835     92        1 ( 134/1267- 172/1349)  90.0 E69-E65 N14-N19
      4  469 1068 (N00E35 L=344)   462    145        1 ( 411/1040- 526/1099)  -7.1 E39-E31 S01-N02
      5  453  889 (S10E37 L=342)   918    214        3 ( 431/ 779- 477/ 999)  77.0 E39-E34 S16-S03
      6 1827  890 (S10W57 L= 76)   388     59        1 (1810/ 865-1850/ 915)  26.6 W55-W59 S11-S08
      7  301  859 (S12E50 L=329)   284     50        1 ( 277/ 834- 325/ 881)  14.0 E52-E47 S13-S10
      8  225  790 (S15E59 L=320)  1574    246        7 ( 185/ 732- 260/ 863) -76.0 E62-E55 S18-S10
      9 1428  824 (S15W25 L= 44)   337    103        0 (1367/ 805-1469/ 852)   8.1 W21-W28 S16-S13
     10 1740  715 (S21W51 L= 70)   500    121        1 (1695/ 659-1773/ 772)  60.3 W48-W53 S24-S17
     11  805  672 (S24E15 L=  4)   421     76        1 ( 786/ 634- 834/ 721)  78.7 E15-E12 S26-S21
     12 1128  642 (S27W07 L= 25)   276     87        0 (1103/ 605-1143/ 693)  80.5 W05-W07 S29-S23
     13  288  602 (S27E57 L=322)   484     85        1 ( 272/ 567- 309/ 639)  78.7 E58-E54 S29-S24
     14  510  569 (S30E38 L=341)   542    142        0 ( 470/ 527- 545/ 621)  32.0 E41-E33 S33-S27
     15  264  538 (S31E62 L=317)   517    106        0 ( 243/ 512- 289/ 559)   9.5 E64-E58 S32-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.