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| 20150421 - Filament data for 10 UTC |
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Available data for 20150421: »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
1 994 1859 (N48E36 L= 0) 512 55 0 ( 967/1842-1022/1879) 76.0 E39-E33 N44-N49
2 1031 1766 (N41E26 L= 11) 1415 300 4 ( 989/1691-1069/1837) -52.4 E32-E20 N34-N47
3 1090 1634 (N33E15 L= 21) 893 151 3 (1056/1578-1147/1698) -21.8 E19-E09 N29-N37
4 497 1589 (N14E51 L=345) 1320 400 2 ( 448/1444- 551/1693) -37.9 E59-E40 N06-N20
5 416 1597 (N13E59 L=337) 443 103 0 ( 398/1563- 437/1635) -68.2 E60-E57 N10-N15
6 336 1527 (N07E63 L=333) 2183 276 7 ( 273/1467- 372/1612) -78.7 E68-E58 N02-N12
7 1712 1461 (N43W37 L= 74) 405 73 0 (1682/1444-1744/1479) 15.9 W33-W40 N41-N44
8 1527 1310 (N26W22 L= 59) 356 104 1 (1508/1258-1544/1359) -74.1 W20-W24 N21-N28
9 988 1247 (N06E08 L= 29) 263 49 0 ( 969/1216-1011/1278) 90.0 E08-E07 N04-N08
10 347 1224 (S10E48 L=348) 374 67 1 ( 322/1192- 369/1261) 68.2 E49-E47 S12-S07
11 1259 1054 (N03W12 L= 49) 390 156 1 (1193/1033-1306/1082) 45.0 W08-W15 N00-N05
12 1340 1036 (N04W17 L= 54) 213 17 0 (1321/1015-1357/1058) 71.6 W16-W18 N02-N05
13 1784 912 (N11W52 L= 89) 3644 729 5 (1671/ 736-1862/1034) -28.8 W39-W65 N01-N18
14 1696 875 (N06W45 L= 82) 354 60 0 (1676/ 842-1720/ 906) -58.4 W43-W46 N03-N08
15 495 817 (S31E28 L= 9) 248 46 1 ( 470/ 793- 516/ 840) 63.4 E29-E26 S32-S28
16 872 755 (S24E01 L= 35) 619 171 0 ( 788/ 728- 961/ 795) 48.8 E06-W02 S27-S19
17 1026 600 (S29W13 L= 50) 346 61 1 ( 986/ 579-1062/ 624) 11.3 W10-W15 S30-S27
18 796 538 (S40W01 L= 37) 492 133 0 ( 726/ 524- 859/ 552) 26.6 E04-W04 S41-S37
19 1298 230 (S42W53 L= 89) 578 67 0 (1259/ 214-1330/ 242) 45.0 W49-W55 S43-S40
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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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