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| 20141125 - Filament data for 11 UTC |
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Available data for 20141125: »08 UTC »09 UTC »10 UTC »11 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1400 1546 (N25W36 L=209) 1321 206 2 (1305/1497-1479/1582) -14.0 W29-W41 N21-N27
2 1615 1525 (N19W51 L=224) 818 190 2 (1559/1493-1682/1552) -4.8 W45-W57 N17-N20
3 1632 1381 (N10W46 L=220) 348 86 0 (1592/1342-1660/1406) -59.0 W43-W48 N07-N12
4 234 1377 (N38E54 L=120) 547 149 0 ( 200/1353- 284/1394) -6.3 E57-E48 N36-N38
5 1126 1309 (N16W11 L=185) 985 201 4 (1031/1244-1212/1357) -48.0 W06-W15 N10-N20
6 449 1251 (N25E33 L=140) 1418 389 5 ( 320/1169- 577/1351) -38.7 E44-E24 N18-N34
7 161 1042 (N18E61 L=112) 780 127 2 ( 138/ 990- 181/1098) -74.1 E63-E59 N14-N21
8 364 1052 (N15E42 L=132) 653 196 1 ( 317/ 990- 430/1096) 45.0 E45-E36 N11-N17
9 1687 1076 (S08W43 L=216) 389 88 1 (1649/1055-1719/1093) -21.8 W39-W45 S09-S06
10 1821 983 (S16W53 L=226) 1011 269 7 (1781/ 903-1849/1084) 79.7 W48-W57 S21-S10
11 1716 988 (S14W44 L=217) 414 101 0 (1686/ 938-1734/1036) 51.3 W40-W45 S16-S11
12 607 885 (N01E27 L=146) 281 89 0 ( 593/ 832- 621/ 931) 63.4 E28-E26 S01-N03
13 945 842 (S07E08 L=165) 203 144 0 ( 877/ 819-1025/ 853) -26.6 E11-E03 S10-S06
14 394 698 (S06E47 L=126) 706 170 0 ( 336/ 637- 442/ 735) -60.3 E52-E44 S10-S03
15 588 684 (S10E33 L=140) 251 69 2 ( 575/ 655- 609/ 723) 78.7 E34-E32 S12-S07
16 1535 619 (S33W26 L=200) 1255 276 4 (1413/ 543-1604/ 715) 20.6 W16-W32 S36-S27
17 975 587 (S23E12 L=161) 352 90 1 ( 926/ 561-1016/ 622) 15.9 E15-E08 S24-S21
18 1038 486 (S31E11 L=163) 1431 370 2 ( 900/ 375-1185/ 619) 22.6 E23-W01 S36-S25
19 488 514 (S19E46 L=127) 720 144 3 ( 443/ 475- 538/ 558) -51.3 E48-E43 S21-S15
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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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