logo kso logo uni graz

20260308 - Filament data for 10 UTC
Available data for 20260308: »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC   »15 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  707 1824 (N34E51 L= 94)  1574    158        1 ( 642/1776- 770/1867) -10.8 E63-E42 N30-N36
      2  533 1619 (N16E48 L= 96)   836    122        1 ( 469/1597- 594/1636)  24.0 E52-E43 N13-N17
      3  913 1410 (N12E16 L=128)   269     67        0 ( 887/1380- 952/1439)  68.2 E17-E14 N09-N14
      4  820 1266 (N01E17 L=127)   409     72        0 ( 793/1224- 845/1306) -76.0 E18-E15 S01-N03
      5 1694 1218 (N22W37 L=181)   900    180        0 (1618/1170-1755/1248)  38.7 W31-W42 N16-N24
      6 1801  999 (N13W50 L=194)  2872    334        5 (1681/ 886-1890/1124) -20.2 W40-W62 N05-N21
      7  631 1068 (S14E24 L=120)   440     77        1 ( 608/1030- 657/1108) -76.0 E25-E21 S15-S11
      8 1579  948 (N03W34 L=178)   433    127        1 (1531/ 921-1621/ 987)   8.1 W29-W36 N01-N05
      9 1386  914 (S04W23 L=167)   426    124        0 (1361/ 855-1416/ 970) -81.9 W21-W24 S07-N00
     10  314  839 (S34E46 L= 99)  1923    316        2 ( 178/ 782- 460/ 888)  17.4 E64-E32 S39-S28
     11 1116  734 (S21W13 L=157)   245     75        0 (1074/ 721-1160/ 748)  31.0 W10-W15 S22-S19
     12 1541  505 (S21W49 L=194)   432    108        0 (1504/ 462-1563/ 555) -63.4 W46-W51 S23-S17
     13  797  528 (S42E00 L=144)   261     27        0 ( 775/ 506- 820/ 551)  71.6 E01-W01 S43-S39
     14  716  494 (S46E06 L=139)   260     43        0 ( 696/ 477- 744/ 513)   0.0 E07-E03 S47-S45
     15 1612  461 (S20W58 L=202)   584    120        1 (1570/ 424-1650/ 510) -71.6 W55-W61 S23-S17
  
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.