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| 20141120 - Filament data for 10 UTC |
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Available data for 20141120: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 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 1634 1681 (N27W63 L=303) 750 112 2 (1610/1654-1659/1709) 36.9 W59-W65 N25-N28
2 1619 1510 (N17W51 L=291) 1091 159 3 (1569/1467-1680/1543) -10.3 W46-W57 N15-N19
3 1786 1467 (N11W66 L=306) 1274 333 1 (1726/1434-1837/1514) 2.7 W57-W78 N09-N12
4 1174 1418 (N22W18 L=257) 957 300 0 (1036/1383-1334/1464) -27.9 W10-W27 N18-N27
5 1753 1333 (N04W56 L=295) 322 119 1 (1720/1310-1787/1354) 0.0 W51-W59 N03-N05
6 653 1209 (N20E19 L=221) 2090 598 5 ( 426/1168- 952/1245) -17.9 E34-W00 N13-N24
7 1898 1111 (S12W65 L=304) 1538 245 7 (1870/1071-1940/1160) 9.5 W60-W72 S13-S08
8 971 1060 (N05E02 L=237) 229 34 1 ( 952/1036- 995/1082) 18.4 E03-W00 N04-N06
9 218 987 (N15E56 L=184) 682 184 1 ( 184/ 907- 262/1056) -68.2 E58-E53 N09-N19
10 1874 865 (S26W57 L=297) 2910 261 2 (1813/ 773-1921/ 975) 51.3 W50-W63 S30-S19
11 1382 866 (S14W18 L=257) 306 39 0 (1360/ 841-1403/ 895) 56.3 W16-W19 S15-S12
12 1159 852 (S10W04 L=244) 234 80 0 (1119/ 819-1192/ 876) 21.8 W01-W06 S11-S09
13 1291 769 (S18W11 L=250) 364 160 0 (1200/ 752-1364/ 797) -10.3 W04-W15 S18-S16
14 1186 686 (S21W03 L=242) 207 50 1 (1162/ 667-1219/ 700) -14.0 W00-W04 S21-S19
15 304 565 (S11E62 L=178) 603 97 2 ( 275/ 538- 336/ 594) -8.1 E65-E58 S12-S08
16 258 524 (S13E70 L=169) 2034 213 3 ( 225/ 482- 293/ 558) -78.7 E75-E65 S15-S10
17 1652 518 (S44W37 L=276) 619 98 1 (1621/ 489-1681/ 552) 0.0 W33-W39 S46-S41
18 1474 391 (S49W20 L=259) 1150 125 2 (1419/ 354-1514/ 444) 32.0 W14-W24 S53-S45
19 725 349 (S33E38 L=202) 1375 265 2 ( 661/ 268- 772/ 441) 38.2 E47-E31 S37-S26
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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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