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| 20141213 - Filament data for 12 UTC |
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Available data for 20141213: »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 1702 1480 (N19W54 L=350) 456 104 1 (1662/1429-1738/1530) -74.1 W52-W57 N15-N22
2 1637 1465 (N19W48 L=343) 324 45 0 (1612/1438-1665/1494) -63.4 W46-W49 N17-N21
3 269 1407 (N32E52 L=243) 462 101 3 ( 244/1375- 303/1433) 21.8 E54-E49 N29-N33
4 288 1371 (N29E50 L=246) 426 67 1 ( 262/1344- 313/1399) 56.3 E52-E47 N27-N30
5 472 1297 (N22E33 L=262) 393 115 1 ( 418/1270- 527/1319) 7.1 E37-E29 N20-N22
6 1386 1261 (N09W25 L=320) 208 91 0 (1358/1221-1413/1305) 38.7 W22-W27 N07-N11
7 1876 1134 (S03W63 L=359) 1311 194 4 (1836/1087-1914/1187) -56.3 W58-W68 S06-N00
8 166 1168 (N18E61 L=234) 504 58 0 ( 141/1148- 188/1185) -18.4 E64-E58 N16-N19
9 1448 1136 (N01W27 L=323) 380 60 1 (1425/1097-1465/1176) 56.3 W25-W28 N00-N03
10 1740 922 (S14W47 L=342) 471 105 0 (1707/ 870-1773/ 985) 49.4 W43-W50 S17-S10
11 1640 910 (S14W39 L=334) 266 66 1 (1626/ 879-1655/ 954) 63.4 W37-W39 S15-S11
12 1433 886 (S13W24 L=319) 208 62 1 (1409/ 855-1461/ 913) -45.0 W22-W25 S15-S11
13 329 877 (S02E48 L=248) 262 37 0 ( 311/ 849- 346/ 902) -56.3 E49-E46 S03-N00
14 1844 824 (S22W57 L=353) 648 142 0 (1801/ 773-1884/ 861) 32.0 W52-W61 S24-S19
15 1132 705 (S21W03 L=298) 945 130 3 (1060/ 604-1184/ 791) 51.3 E02-W06 S26-S16
16 392 686 (S13E47 L=249) 1336 247 4 ( 339/ 640- 466/ 731) -16.7 E51-E40 S16-S10
17 1636 669 (S29W39 L=334) 568 106 1 (1583/ 624-1683/ 713) 26.6 W34-W42 S31-S26
18 480 545 (S23E44 L=252) 835 250 1 ( 441/ 449- 506/ 645) 53.1 E48-E38 S29-S17
19 794 283 (S46E32 L=264) 662 87 2 ( 756/ 249- 822/ 318) 39.8 E35-E28 S49-S43
20 642 225 (S49E50 L=246) 679 108 1 ( 613/ 205- 667/ 254) 14.0 E54-E46 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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