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| 20240116 - Latest Filament data |
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Available data for 20240116: »07 UTC »08 UTC »09 UTC »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
1 747 1693 (N38E27 L=355) 1938 320 4 ( 590/1635- 884/1736) -8.1 E42-E14 N33-N40
2 1263 1672 (N40W13 L= 36) 596 196 0 (1175/1635-1346/1723) -21.0 W06-W19 N37-N43
3 1292 1535 (N29W15 L= 37) 261 99 0 (1246/1507-1330/1575) -33.7 W11-W17 N27-N32
4 350 1450 (N19E52 L=330) 360 62 1 ( 320/1433- 388/1464) 0.0 E55-E48 N17-N19
5 1100 1366 (N17W02 L= 25) 815 224 1 (1042/1269-1149/1451) 76.0 W00-W05 N10-N22
6 286 1336 (N12E55 L=327) 345 66 0 ( 267/1310- 309/1367) -33.7 E57-E51 N09-N13
7 1310 1287 (N13W16 L= 38) 684 238 0 (1206/1236-1411/1341) -13.0 W09-W22 N10-N15
8 513 1282 (N08E34 L=348) 232 100 0 ( 474/1258- 566/1295) 18.4 E37-E30 N06-N09
9 1079 1148 (N03W02 L= 25) 178 95 1 (1045/1111-1111/1196) -45.0 W00-W04 N01-N05
10 302 1163 (N01E50 L=332) 367 76 0 ( 273/1130- 333/1191) 31.0 E52-E47 S01-N02
11 568 1109 (S02E29 L=353) 426 129 0 ( 516/1049- 618/1156) 45.0 E32-E25 S05-N01
12 286 1003 (S09E51 L=332) 660 105 2 ( 262/ 943- 314/1052) 66.8 E53-E48 S12-S05
13 206 962 (S11E59 L=323) 459 52 1 ( 189/ 934- 224/ 996) 45.0 E61-E57 S12-S09
14 148 923 (S13E68 L=314) 588 131 0 ( 124/ 880- 163/ 991) 40.6 E72-E64 S15-S09
15 1328 969 (S06W19 L= 41) 192 14 0 (1310/ 949-1346/ 989) 45.0 W17-W19 S07-S04
16 966 844 (S16E02 L= 20) 600 275 0 ( 836/ 820-1091/ 865) 7.6 E10-W05 S17-S14
17 1797 657 (S19W63 L= 86) 3718 293 7 (1719/ 556-1879/ 782) 71.6 W56-W72 S26-S11
18 234 627 (S32E66 L=316) 2746 235 2 ( 200/ 526- 267/ 739) 34.4 E84-E60 S37-S24
19 1647 629 (S23W49 L= 71) 841 230 1 (1576/ 533-1695/ 717) -32.0 W39-W55 S28-S18
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Download FITS filament maps as tar archive
» All Filament Data of 20240116 ...
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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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