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| 20140218 - Latest Filament data |
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Available data for 20140218: »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
1 483 1630 (N20E51 L=218) 932 258 3 ( 419/1600- 554/1670) -7.6 E58-E43 N18-N22
2 219 1153 (S12E58 L=211) 3344 714 9 ( 156/ 975- 260/1314) -81.5 E66-E51 S22-S02
3 170 1084 (S16E62 L=207) 861 169 6 ( 141/1025- 210/1115) 63.4 E66-E57 S20-S14
4 961 1033 (S08E04 L=266) 194 45 1 ( 942/1008- 978/1061) 76.0 E04-E03 S09-S05
5 404 988 (S20E39 L=230) 516 171 1 ( 356/ 913- 453/1054) 66.0 E42-E36 S24-S15
6 800 971 (S14E12 L=257) 371 148 2 ( 720/ 952- 868/ 987) 26.6 E16-E07 S16-S12
7 404 884 (S26E38 L=231) 282 110 1 ( 373/ 842- 433/ 930) 56.3 E40-E36 S28-S22
8 1332 832 (S11W22 L=292) 461 165 3 (1289/ 783-1401/ 883) -20.6 W19-W27 S13-S08
9 981 764 (S23W03 L=272) 2183 779 9 ( 671/ 675-1391/ 858) 21.8 E16-W27 S34-S14
10 1603 721 (S11W43 L=313) 259 100 2 (1563/ 698-1646/ 741) 38.7 W40-W45 S12-S08
11 1624 661 (S14W47 L=316) 283 111 1 (1581/ 640-1673/ 681) 33.7 W44-W50 S15-S11
12 1223 583 (S28W23 L=292) 288 83 1 (1175/ 565-1274/ 604) 18.4 W19-W26 S29-S26
13 1810 559 (S13W71 L=340) 1262 247 5 (1770/ 520-1856/ 596) 33.7 W66-W78 S15-S09
14 636 524 (S45E18 L=252) 558 121 4 ( 610/ 476- 668/ 582) -66.8 E20-E14 S48-S41
15 1592 543 (S21W50 L=319) 556 72 1 (1555/ 514-1631/ 576) 68.2 W47-W51 S23-S18
16 961 488 (S40W09 L=278) 437 151 2 ( 890/ 452-1043/ 523) 37.9 W04-W13 S44-S36
17 755 443 (S49E06 L=263) 291 30 1 ( 730/ 425- 778/ 467) 11.3 E08-E03 S49-S46
18 1228 394 (S40W32 L=301) 364 63 0 (1185/ 375-1259/ 411) 31.0 W28-W33 S40-S37
19 1274 240 (S48W46 L=316) 434 89 1 (1253/ 206-1289/ 265) -33.7 W43-W50 S50-S46
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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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