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| 20251104 - Latest Filament data |
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Available data for 20251104: »06 UTC »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
1 910 1891 (N65W34 L= 10) 1009 72 1 ( 869/1854- 948/1928) 6.0 W26-W46 N61-N67
2 826 1833 (N62W17 L=353) 351 46 0 ( 806/1812- 851/1856) -90.0 W14-W20 N59-N65
3 1107 1689 (N41W27 L= 3) 1632 386 3 ( 949/1650-1285/1729) -26.6 W14-W37 N32-N45
4 723 1575 (N44E05 L=330) 281 61 1 ( 700/1552- 745/1601) 26.6 E07-E02 N42-N45
5 1660 1442 (N11W52 L= 28) 556 92 0 (1631/1393-1688/1483) -90.0 W50-W53 N07-N13
6 1404 1209 (N05W26 L= 2) 445 91 0 (1367/1159-1439/1250) -80.5 W24-W27 N01-N07
7 440 1130 (N23E34 L=302) 281 54 1 ( 410/1107- 468/1156) 0.0 E36-E31 N21-N24
8 197 1064 (N24E58 L=277) 2077 214 5 ( 149/ 996- 243/1141) -55.0 E64-E52 N19-N29
9 1759 1083 (S11W48 L= 23) 413 72 0 (1732/1046-1783/1121) -68.2 W46-W49 S13-S08
10 1413 941 (S10W20 L=356) 1119 319 0 (1355/ 798-1446/1086) 51.8 W13-W24 S16-S02
11 613 989 (N11E25 L=311) 896 253 2 ( 515/ 929- 713/1077) -52.4 E29-E19 N05-N18
12 269 1011 (N19E51 L=285) 585 102 1 ( 250/ 960- 300/1058) -90.0 E52-E47 N16-N22
13 198 946 (N17E59 L=276) 537 80 1 ( 165/ 925- 239/ 970) -18.4 E63-E54 N15-N18
14 215 750 (N05E63 L=273) 3132 305 6 ( 147/ 653- 266/ 857) 36.3 E75-E54 N00-N11
15 1834 649 (S41W56 L= 32) 1045 116 0 (1784/ 625-1890/ 674) -16.3 W47-W71 S44-S37
16 1683 556 (S42W37 L= 12) 1171 250 0 (1586/ 479-1761/ 641) 18.4 W26-W45 S45-S38
17 1067 510 (S27E11 L=325) 290 61 0 (1039/ 477-1091/ 541) 31.0 E13-E08 S28-S24
18 646 219 (S36E59 L=277) 831 85 1 ( 610/ 188- 675/ 261) 13.2 E68-E51 S38-S33
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Download FITS filament maps as tar archive
» All Filament Data of 20251104 ...
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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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