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20260311 - Filament data for 08 UTC
Available data for 20260311: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »13 UTC   »14 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1165 1662 (N34E10 L= 96)   522     92        1 (1125/1622-1208/1687) -15.9 E13-E06 N32-N36
      2  471 1609 (N14E53 L= 53)   873    144        4 ( 436/1573- 530/1665) -56.3 E58-E48 N11-N17
      3  405 1548 (N09E55 L= 51)   370     40        0 ( 382/1530- 430/1565)   0.0 E58-E53 N07-N09
      4  531 1513 (N09E43 L= 63)   270     37        1 ( 507/1499- 560/1530)  18.4 E45-E41 N08-N10
      5 1457 1481 (N31W14 L=120)   255     28        1 (1437/1462-1481/1504)  56.3 W12-W15 N29-N32
      6  365 1154 (S15E45 L= 61)  3065    617        6 ( 113/1096- 608/1218)  13.2 E74-E27 S19-S06
      7 1529 1154 (N13W26 L=132)   233     51        0 (1512/1130-1544/1187) -76.0 W24-W26 N11-N15
      8 1428 1016 (N03W23 L=129)   618    123        1 (1400/ 954-1455/1068) -80.5 W19-W24 N00-N06
      9 1908  831 (N09W69 L=175)  1906     92        2 (1884/ 779-1938/ 887)  90.0 W64-W74 N06-N13
     10  766  670 (S34E06 L=100)  1565    384        4 ( 580/ 633- 932/ 718)  25.6 E19-W04 S40-S28
     11  357  680 (S43E41 L= 65)  1163    203        3 ( 270/ 648- 465/ 705)  14.0 E53-E29 S46-S39
     12 1795  647 (S04W64 L=169)   457    101        0 (1774/ 602-1816/ 700) -71.6 W62-W65 S07-S01
     13 1209  339 (S40W38 L=144)   284     14        0 (1191/ 319-1227/ 361) -26.6 W36-W40 S41-S39
     14 1124  305 (S46W35 L=141)   692     86        1 (1096/ 273-1159/ 342) -20.6 W30-W38 S47-S42
     15 1016  286 (S51W30 L=136)   517     78        1 ( 982/ 262-1059/ 317)   7.1 W25-W33 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.