logo kso logo uni graz

20260311 - Filament data for 13 UTC
Available data for 20260311: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 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 1124 1745 (N39E16 L= 87)   270     60        1 (1092/1722-1153/1765)   0.0 E19-E13 N37-N40
      2 1190 1655 (N35E08 L= 95)   456     76        0 (1162/1626-1229/1677)  36.9 E10-E05 N31-N36
      3  481 1579 (N12E50 L= 53)  1154    193        5 ( 405/1525- 562/1643)  37.9 E55-E45 N08-N16
      4  580 1498 (N09E39 L= 64)   455     96        2 ( 541/1459- 623/1532)   0.0 E42-E36 N07-N11
      5  223 1299 (S09E62 L= 41)   447     75        1 ( 196/1270- 247/1330)  53.1 E64-E59 S10-S06
      6  393 1144 (S15E42 L= 61)  3296    682        9 ( 135/1087- 681/1200)  13.2 E71-E23 S19-S05
      7 1574 1129 (N13W29 L=132)   254     46        2 (1557/1101-1593/1155) -56.3 W27-W30 N11-N15
      8 1465  980 (N02W26 L=129)   572    108        2 (1424/ 931-1502/1040)  90.0 W23-W27 N00-N06
      9  133 1002 (S27E69 L= 34)   589     62        1 ( 112/ 969- 152/1034)  39.8 E73-E65 S29-S24
     10  349  675 (S44E42 L= 61)   650    107        2 ( 301/ 651- 392/ 706)  24.4 E48-E37 S46-S40
     11  883  659 (S31W02 L=105)   874    197        2 ( 784/ 640- 977/ 697)  24.4 E04-W07 S34-S28
     12  487  663 (S41E28 L= 75)   435     69        1 ( 448/ 646- 520/ 688)  33.7 E31-E24 S43-S39
     13  662  629 (S39E13 L= 90)   498     81        2 ( 617/ 606- 708/ 652)  15.9 E16-E09 S41-S37
     14  357  450 (S61E52 L= 51)   573     95        2 ( 318/ 431- 409/ 481)   0.0 E59-E41 S63-S59
     15 1141  291 (S46W38 L=141)   546     65        2 (1118/ 258-1172/ 324) -59.0 W34-W41 S48-S43
     16 1040  267 (S51W33 L=136)   572     86        3 (1006/ 238-1082/ 306)   7.1 W28-W37 S52-S48
  
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.