logo kso logo uni graz

20251207 - Filament data for 09 UTC
Available data for 20251207: »07 UTC   »08 UTC   »09 UTC   »10 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1066 1638 (N37W13 L=277)   537    115        1 (1004/1599-1114/1671) -45.0 W09-W16 N34-N41
      2 1220 1376 (N18W17 L=280)   192     90        0 (1178/1366-1267/1393) -21.8 W14-W19 N17-N19
      3  594 1319 (N23E24 L=240)   519    159        1 ( 523/1283- 662/1341) -26.6 E28-E18 N20-N25
      4 1829 1265 (N04W60 L=323)   349     59        1 (1802/1242-1850/1283) -21.8 W57-W62 N02-N04
      5  688 1210 (N15E18 L=246)   301     97        0 ( 668/1162- 711/1261) -80.5 E18-E16 N12-N18
      6 1054 1136 (N06W03 L=267)   211     99        0 (1006/1124-1103/1151)   0.0 W00-W06 N05-N06
      7  192 1016 (N10E59 L=205)   604     65        2 ( 171/ 975- 216/1052)  53.1 E61-E55 N08-N12
      8 1514  921 (S12W29 L=292)   247     68        1 (1487/ 897-1546/ 938)   0.0 W26-W31 S13-S11
      9 1205  896 (S10W09 L=272)   246    116        0 (1164/ 868-1254/ 919) -21.8 W06-W11 S11-S08
     10 1044  728 (S18E03 L=261)   417    139        2 (1014/ 669-1072/ 801) -90.0 E04-E01 S21-S13
     11 1785  668 (S32W54 L=318)   422     42        1 (1757/ 645-1810/ 684)   0.0 W50-W57 S33-S30
     12  302  589 (S16E59 L=204)   438     69        1 ( 275/ 552- 323/ 609) -76.0 E61-E56 S18-S14
     13  759  472 (S30E27 L=237)   461     95        0 ( 722/ 428- 797/ 509)  35.5 E30-E22 S32-S27
     14  594  456 (S28E40 L=224)   510    109        1 ( 563/ 412- 623/ 504) -90.0 E40-E37 S31-S24
     15  441  435 (S28E54 L=209)   937    170        4 ( 392/ 371- 473/ 477)  60.3 E60-E49 S31-S24
     16 1600  310 (S58W53 L=316)   785     82        2 (1561/ 295-1638/ 332)  -9.9 W43-W67 S60-S55
  
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.