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| 20140928 - Filament data for 12 UTC |
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Available data for 20140928: »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1248 1572 (N31W32 L=249) 588 162 0 (1169/1547-1323/1597) -15.3 W26-W37 N28-N33
2 1696 1520 (N13W62 L=279) 1885 356 4 (1631/1461-1783/1558) -8.1 W52-W73 N09-N14
3 437 1164 (N29E34 L=183) 1207 285 3 ( 404/1035- 495/1304) 61.9 E37-E27 N21-N36
4 817 1266 (N26E06 L=212) 808 265 2 ( 687/1217- 928/1304) -37.6 E13-W01 N20-N30
5 1204 1251 (N14W16 L=234) 1930 428 2 ( 992/1209-1412/1283) -21.8 W03-W28 N08-N18
6 1721 1106 (S09W45 L=262) 272 88 1 (1695/1068-1745/1131) 45.0 W42-W47 S11-S08
7 1755 1070 (S12W47 L=264) 389 103 0 (1737/1017-1778/1119) 33.7 W44-W50 S14-S10
8 1662 1066 (S09W39 L=257) 287 82 1 (1644/1038-1688/1105) 71.6 W38-W41 S10-S07
9 805 909 (N06E15 L=202) 1074 281 1 ( 767/ 813- 870/1067) 70.3 E18-E10 N00-N14
10 1551 970 (S11W29 L=246) 242 53 0 (1519/ 949-1574/ 992) 14.0 W26-W30 S11-S09
11 1586 947 (S13W31 L=248) 414 113 2 (1542/ 918-1617/ 974) 9.5 W27-W33 S14-S11
12 1389 901 (S10W17 L=235) 267 67 0 (1370/ 867-1416/ 932) 26.6 W15-W19 S11-S08
13 1755 801 (S28W42 L=259) 589 98 0 (1724/ 766-1772/ 853) 31.0 W38-W43 S30-S25
14 1193 645 (S19E01 L=217) 2052 425 1 (1069/ 458-1272/ 805) 85.6 E05-W02 S32-S06
15 217 728 (N08E66 L=152) 487 76 1 ( 189/ 716- 246/ 748) -8.1 E69-E61 N06-N08
16 562 590 (S07E40 L=178) 395 96 1 ( 524/ 566- 611/ 610) -18.4 E42-E36 S08-S05
17 672 429 (S19E39 L=178) 428 86 0 ( 635/ 383- 701/ 457) -80.5 E41-E38 S22-S16
18 451 396 (S17E59 L=159) 672 194 0 ( 435/ 340- 465/ 453) 45.0 E62-E53 S20-S12
19 709 275 (S31E46 L=171) 975 204 0 ( 676/ 222- 733/ 338) 36.0 E52-E41 S34-S25
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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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