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20140610 - Filament data for 06 UTC
Available data for 20140610: »05 UTC   »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  407 1485 (N20E52 L=183)  1128    194        2 ( 372/1429- 449/1547) -31.0 E57-E46 N17-N23
      2  293 1467 (N17E63 L=172)   718    149        0 ( 278/1399- 309/1525) -63.4 E65-E60 N13-N21
      3  923 1421 (N23E12 L=223)   487    163        1 ( 900/1351- 954/1508) -84.8 E13-E10 N18-N29
      4  551 1343 (N13E36 L=200)   318    116        0 ( 514/1306- 586/1372) -26.6 E38-E32 N11-N14
      5  901 1226 (N11E10 L=225)   218     43        1 ( 883/1201- 919/1257) -56.3 E11-E09 N09-N12
      6  289 1196 (N01E54 L=181)   381     56        1 ( 269/1168- 308/1218) -14.0 E56-E52 N00-N02
      7 1646 1144 (N16W40 L=275)   733    196        3 (1588/1098-1680/1207) -50.2 W35-W43 N12-N19
      8 1434 1145 (N13W24 L=259)   524    191        0 (1333/1128-1505/1172)   9.5 W17-W29 N11-N15
      9 1516  925 (N01W32 L=268)  1155    239        1 (1484/ 839-1581/1036)  76.0 W30-W36 S04-N08
     10  445  822 (S20E36 L=199)   362    116        0 ( 411/ 794- 503/ 856) -15.9 E39-E31 S21-S17
     11 1328  815 (S08W22 L=257)   368    111        1 (1282/ 779-1376/ 844) -15.9 W18-W25 S10-S06
     12 1207  732 (S15W15 L=251)   625    133        3 (1123/ 686-1283/ 802)  45.0 W10-W19 S18-S09
     13 1608  685 (S13W45 L=280)  1333    208        7 (1566/ 617-1650/ 756)  84.3 W40-W47 S17-S07
     14 1272  653 (S19W21 L=256)   870    275        2 (1187/ 560-1380/ 727)  53.1 W17-W27 S26-S13
     15 1147  585 (S25W15 L=250)   218     66        2 (1135/ 557-1161/ 617) -56.3 W13-W15 S26-S23
     16 1329  457 (S31W31 L=266)   552     97        2 (1276/ 436-1370/ 483)  26.6 W27-W33 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.