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| 20140418 - Filament data for 06 UTC |
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Available data for 20140418: »06 UTC »07 UTC »08 UTC »09 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 461 1583 (N13E54 L=162) 680 170 1 ( 440/1519- 480/1651) -56.3 E58-E51 N08-N17
2 1106 1519 (N25E10 L=206) 239 114 0 (1082/1473-1136/1569) 90.0 E10-E08 N21-N29
3 741 1373 (N07E26 L=190) 242 48 2 ( 712/1352- 772/1393) 45.0 E27-E24 N05-N08
4 425 1297 (S05E44 L=172) 612 162 1 ( 401/1206- 468/1349) -83.7 E45-E41 S10-S01
5 568 1145 (S10E30 L=186) 1676 519 1 ( 397/ 992- 647/1341) 84.8 E39-E24 S22-N00
6 1374 1232 (N16W14 L=230) 417 166 1 (1318/1166-1401/1306) 84.8 W12-W15 N10-N21
7 1662 1189 (N23W35 L=251) 672 86 1 (1629/1148-1685/1235) -68.2 W32-W37 N19-N25
8 136 1100 (S22E67 L=149) 1186 244 1 ( 100/1043- 169/1147) 49.4 E69-E63 S25-S18
9 369 1094 (S18E43 L=173) 357 126 0 ( 324/1056- 414/1134) 50.2 E46-E40 S20-S14
10 1267 1000 (S00W14 L=230) 201 58 1 (1246/ 971-1289/1033) -33.7 W12-W15 S01-N01
11 899 941 (S13E05 L=211) 323 145 0 ( 833/ 899- 978/ 965) 40.6 E07-W00 S17-S10
12 1787 919 (N12W52 L=268) 322 43 1 (1771/ 891-1803/ 945) -45.0 W50-W53 N10-N13
13 559 845 (S28E24 L=192) 239 34 1 ( 543/ 823- 581/ 865) -18.4 E25-E22 S29-S26
14 319 736 (S41E43 L=173) 378 38 1 ( 298/ 711- 342/ 763) -36.9 E45-E40 S42-S39
15 990 676 (S26W08 L=224) 457 146 1 ( 974/ 609-1020/ 749) -54.5 W05-W11 S29-S21
16 1161 605 (S25W21 L=237) 405 146 0 (1101/ 586-1234/ 632) 18.4 W16-W25 S26-S21
17 1093 508 (S32W21 L=237) 521 119 1 (1041/ 458-1128/ 550) -12.5 W16-W25 S34-S30
18 1658 523 (S13W58 L=274) 421 61 1 (1634/ 500-1680/ 548) 71.6 W55-W61 S14-S11
19 1147 227 (S48W44 L=260) 1309 222 1 (1114/ 167-1178/ 283) -17.4 W36-W52 S51-S44
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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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