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| 20140113 - Filament data for 10 UTC |
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Available data for 20140113: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 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 1463 1440 (N24W27 L= 53) 978 238 4 (1359/1380-1574/1515) -25.0 W20-W35 N20-N28
2 1276 1446 (N23W14 L= 40) 373 104 0 (1222/1408-1316/1466) -26.6 W10-W16 N20-N24
3 336 1398 (N17E50 L=336) 439 98 2 ( 306/1354- 364/1438) 59.0 E51-E48 N13-N19
4 917 1322 (N13E08 L= 18) 228 71 0 ( 894/1289- 950/1356) -53.1 E09-E05 N11-N15
5 1329 1174 (N06W18 L= 43) 552 185 2 (1251/1133-1404/1234) -11.3 W12-W22 N03-N09
6 638 1188 (N04E24 L= 1) 266 109 0 ( 593/1174- 695/1208) 0.0 E27-E20 N03-N05
7 1016 1127 (N02E01 L= 25) 174 73 0 ( 984/1102-1055/1143) 33.7 E02-W01 N00-N02
8 1932 1103 (N07W70 L= 95) 1318 210 3 (1899/1071-1966/1137) -16.7 W64-W77 N05-N09
9 468 1059 (S04E35 L=350) 451 72 2 ( 448/1017- 491/1098) 68.2 E36-E33 S06-S01
10 834 941 (S10E11 L= 15) 388 232 1 ( 735/ 885- 935/ 983) 26.6 E17-E05 S13-S07
11 314 859 (S16E48 L=338) 788 199 2 ( 257/ 814- 384/ 906) 18.4 E53-E41 S18-S13
12 1785 691 (S19W58 L= 83) 3254 574 12 (1725/ 539-1857/ 881) 82.2 W51-W62 S28-S06
13 1902 816 (S10W69 L= 95) 928 242 3 (1861/ 781-1946/ 863) 29.1 W62-W76 S12-S06
14 1003 615 (S30W01 L= 26) 2916 602 6 ( 706/ 453-1372/ 780) 28.1 E22-W23 S42-S17
15 750 709 (S25E17 L= 9) 375 107 0 ( 705/ 676- 791/ 743) 9.2 E19-E13 S26-S22
16 1719 706 (S19W51 L= 76) 314 45 2 (1694/ 685-1737/ 728) 33.7 W48-W52 S19-S17
17 403 612 (S32E44 L=342) 714 144 0 ( 337/ 591- 458/ 638) -5.7 E49-E39 S32-S29
18 310 577 (S34E54 L=332) 1394 305 5 ( 273/ 514- 354/ 636) 76.0 E59-E49 S37-S29
19 1300 416 (S41W26 L= 52) 675 109 2 (1258/ 377-1343/ 466) 81.9 W22-W28 S44-S37
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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.
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