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| 20141130 - Filament data for 09 UTC |
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Available data for 20141130: »09 UTC »10 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 857 1580 (N38E01 L=107) 371 110 1 ( 814/1542- 908/1603) -9.5 E03-W03 N35-N39
2 1420 1343 (N13W30 L=138) 585 157 0 (1345/1297-1503/1380) -37.9 W25-W34 N08-N16
3 1323 1268 (N10W22 L=130) 196 67 0 (1310/1229-1337/1305) -90.0 W21-W22 N07-N12
4 1789 1252 (N01W56 L=164) 559 107 1 (1762/1212-1822/1298) -78.7 W54-W60 S01-N04
5 849 1177 (N13E08 L=100) 191 83 0 ( 830/1144- 881/1222) -78.7 E08-E06 N10-N15
6 1624 1073 (S06W38 L=146) 880 258 3 (1559/ 946-1658/1193) 56.3 W31-W41 S12-N00
7 1807 1137 (S06W55 L=163) 562 213 1 (1741/1109-1868/1164) -18.4 W49-W61 S08-S03
8 1863 1003 (S15W59 L=167) 1908 333 10 (1816/ 916-1900/1087) -90.0 W53-W63 S20-S09
9 444 1045 (N12E36 L= 72) 640 192 2 ( 366/1021- 530/1072) -9.5 E41-E29 N09-N13
10 1400 1034 (S05W22 L=130) 496 155 3 (1344/ 993-1467/1070) -35.5 W19-W26 S08-S02
11 1773 1032 (S11W50 L=158) 347 48 0 (1756/1002-1794/1064) 71.6 W48-W51 S12-S09
12 1715 974 (S14W44 L=152) 262 87 3 (1698/ 947-1743/1005) -53.1 W42-W46 S15-S11
13 830 945 (S00E13 L= 95) 224 77 1 ( 806/ 908- 856/ 980) -63.4 E13-E11 S02-N02
14 615 926 (N02E26 L= 82) 218 55 2 ( 595/ 894- 639/ 948) 45.0 E27-E24 N00-N03
15 1759 908 (S18W47 L=155) 474 100 2 (1718/ 881-1799/ 939) 0.0 W43-W51 S19-S16
16 1753 804 (S25W46 L=154) 1258 390 3 (1619/ 773-1857/ 871) 2.7 W34-W56 S26-S22
17 1286 762 (S19W11 L=119) 293 100 3 (1263/ 722-1312/ 796) -68.2 W10-W12 S21-S16
18 1780 691 (S33W49 L=157) 1929 354 2 (1651/ 602-1880/ 792) 17.7 W37-W59 S36-S27
19 861 671 (S17E16 L= 92) 255 103 0 ( 814/ 636- 894/ 693) -31.0 E19-E14 S19-S15
20 255 605 (S11E65 L= 43) 535 112 1 ( 234/ 577- 276/ 636) 23.2 E68-E60 S12-S09
21 310 533 (S16E62 L= 46) 1470 253 2 ( 270/ 446- 352/ 598) 73.3 E66-E58 S22-S12
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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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