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| 20141124 - Filament data for 07 UTC |
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Available data for 20141124: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1679 1620 (N23W63 L=251) 2160 336 3 (1596/1574-1771/1681) -39.8 W57-W73 N18-N28
2 1290 1469 (N22W26 L=214) 2386 526 6 (1076/1423-1543/1498) -14.0 W12-W44 N17-N26
3 1802 1462 (N11W68 L=256) 939 145 4 (1776/1437-1838/1485) -14.0 W64-W73 N09-N12
4 1707 1298 (N04W50 L=239) 559 62 1 (1677/1260-1738/1333) -68.2 W48-W52 N01-N06
5 1182 1285 (N14W14 L=203) 258 82 0 (1149/1266-1231/1315) -36.9 W12-W17 N11-N15
6 259 1206 (N27E50 L=139) 1467 384 4 ( 172/1102- 360/1297) -39.5 E59-E41 N18-N33
7 908 1206 (N14E03 L=185) 527 100 1 ( 857/1156- 955/1254) -60.3 E05-E01 N10-N17
8 1914 1122 (S11W67 L=256) 714 184 2 (1888/1102-1942/1151) 8.1 W63-W72 S11-S09
9 1881 1001 (S17W60 L=249) 4522 601 10 (1815/ 862-1936/1131) -83.3 W54-W66 S25-S08
10 1809 983 (S16W52 L=240) 767 79 2 (1784/ 943-1832/1025) 78.7 W49-W54 S18-S13
11 1674 962 (S15W40 L=228) 742 164 0 (1633/ 896-1700/1023) 76.0 W37-W42 S18-S10
12 409 778 (S01E44 L=145) 580 146 1 ( 388/ 696- 441/ 845) 76.0 E45-E42 S06-N02
13 233 648 (S06E66 L=123) 1957 303 3 ( 191/ 586- 282/ 706) 28.3 E76-E60 S09-S02
14 1339 687 (S24W13 L=201) 281 107 0 (1282/ 665-1385/ 701) -26.6 W09-W15 S26-S22
15 1363 565 (S33W13 L=201) 1005 193 2 (1276/ 489-1426/ 652) 28.3 W05-W18 S36-S28
16 340 590 (S11E56 L=132) 416 112 1 ( 318/ 557- 362/ 623) 26.6 E59-E53 S12-S09
17 772 525 (S23E27 L=162) 327 116 0 ( 721/ 491- 811/ 564) 15.9 E30-E23 S24-S20
18 864 440 (S30E24 L=165) 1270 376 4 ( 763/ 325- 978/ 555) 28.6 E35-E12 S36-S24
19 374 483 (S18E58 L=130) 2319 327 5 ( 302/ 405- 448/ 537) -48.0 E64-E52 S24-S14
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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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