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| 20140802 - Filament data for 11 UTC |
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Available data for 20140802: »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 1535 1556 (N31W47 L=298) 346 58 1 (1506/1534-1560/1571) -26.6 W44-W49 N29-N32
2 1023 1339 (N25W04 L=255) 223 51 2 (1001/1316-1048/1366) -63.4 W02-W05 N23-N27
3 1835 1292 (N09W66 L=317) 1905 322 7 (1783/1185-1877/1363) -84.8 W59-W72 N02-N13
4 556 1158 (N19E29 L=222) 1960 467 5 ( 383/1065- 711/1273) -31.0 E43-E18 N11-N27
5 1357 1192 (N12W23 L=274) 309 96 1 (1328/1148-1385/1232) 38.7 W20-W25 N09-N13
6 1857 1059 (S05W62 L=313) 1037 132 2 (1827/1013-1884/1104) 35.5 W57-W66 S07-S02
7 388 1027 (N12E43 L=208) 492 99 0 ( 345/ 987- 411/1059) -38.7 E46-E41 N09-N13
8 187 928 (N06E65 L=186) 443 33 2 ( 169/ 904- 203/ 950) 63.4 E66-E62 N05-N07
9 1633 750 (S20W38 L=289) 2343 408 6 (1515/ 615-1717/ 889) 43.0 W28-W45 S27-S12
10 831 738 (S10E15 L=236) 374 121 0 ( 809/ 687- 854/ 803) 81.9 E17-E14 S12-S05
11 964 776 (S09E07 L=244) 421 114 1 ( 914/ 752-1033/ 800) -8.1 E09-E02 S10-S06
12 1003 699 (S14E05 L=246) 959 330 2 ( 872/ 614-1109/ 793) 28.1 E14-W01 S18-S08
13 675 708 (S10E26 L=225) 364 77 1 ( 642/ 676- 708/ 745) -53.1 E27-E23 S12-S07
14 739 667 (S13E22 L=229) 310 83 1 ( 712/ 630- 779/ 688) 31.0 E24-E19 S15-S11
15 1393 630 (S24W20 L=271) 486 184 2 (1341/ 566-1419/ 686) -71.6 W16-W21 S28-S19
16 1299 601 (S24W13 L=264) 261 54 0 (1281/ 577-1318/ 631) -76.0 W11-W14 S26-S22
17 568 586 (S17E36 L=215) 538 121 2 ( 511/ 548- 614/ 618) -33.7 E40-E33 S19-S14
18 460 564 (S18E45 L=206) 380 78 2 ( 436/ 526- 484/ 604) 80.5 E46-E44 S20-S14
19 557 501 (S23E40 L=211) 304 55 1 ( 539/ 481- 583/ 523) 14.0 E41-E37 S23-S20
20 866 467 (S28E18 L=233) 293 117 0 ( 848/ 419- 879/ 513) 60.3 E20-E16 S31-S24
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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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