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| 20140115 - Filament data for 08 UTC |
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Available data for 20140115: »08 UTC »09 UTC »10 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 1043 1538 (N28E02 L=358) 333 79 1 (1017/1506-1082/1561) -33.7 E03-W00 N25-N29
2 1752 1408 (N25W51 L= 51) 1552 296 3 (1679/1325-1859/1480) -25.0 W44-W61 N20-N29
3 1421 1259 (N12W23 L= 24) 548 191 1 (1330/1210-1491/1304) -26.6 W17-W28 N09-N14
4 1669 1146 (N07W41 L= 42) 693 195 3 (1600/1092-1745/1221) -18.4 W35-W47 N04-N11
5 1100 1146 (N03W04 L= 4) 235 90 1 (1052/1119-1141/1172) 31.0 W01-W06 N01-N04
6 1473 1108 (N03W27 L= 27) 293 149 1 (1406/1071-1522/1164) 41.2 W22-W30 N00-N07
7 841 1017 (S06E11 L=349) 382 146 1 ( 808/ 941- 874/1101) 73.3 E12-E09 S10-N00
8 1747 1080 (N04W48 L= 48) 280 66 2 (1721/1064-1776/1101) 11.3 W45-W50 N03-N05
9 215 1018 (S07E57 L=303) 663 120 4 ( 187/ 975- 250/1073) 63.4 E60-E53 S09-S03
10 286 979 (S10E50 L=310) 304 75 1 ( 260/ 949- 313/ 998) 36.9 E52-E47 S11-S08
11 457 891 (S15E36 L=324) 290 108 0 ( 440/ 841- 474/ 954) -81.9 E37-E35 S17-S10
12 1223 908 (S10W13 L= 13) 204 126 0 (1163/ 892-1292/ 920) 15.9 W09-W16 S11-S09
13 199 796 (S20E60 L=300) 1027 264 1 ( 183/ 699- 237/ 899) 59.7 E63-E55 S26-S14
14 669 868 (S15E21 L=339) 461 102 2 ( 622/ 845- 732/ 896) 15.9 E24-E17 S16-S13
15 946 816 (S17E04 L=357) 218 113 0 ( 902/ 791- 992/ 858) -18.4 E06-W00 S18-S15
16 1746 774 (S14W52 L= 52) 423 100 3 (1718/ 727-1774/ 824) 71.6 W50-W53 S16-S10
17 1413 785 (S16W26 L= 26) 281 104 0 (1383/ 752-1458/ 807) 31.0 W24-W29 S18-S14
18 1091 666 (S26W07 L= 7) 253 80 1 (1054/ 628-1126/ 702) 51.3 W04-W08 S28-S23
19 1299 562 (S31W22 L= 23) 2650 666 7 ( 987/ 430-1596/ 694) 28.8 W01-W41 S42-S20
20 497 552 (S36E37 L=323) 263 166 0 ( 459/ 511- 534/ 603) 13.2 E41-E33 S39-S32
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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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