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| 20251001 - Filament data for 06 UTC |
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Available data for 20251001: »06 UTC »07 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
1 614 1680 (N60E12 L= 57) 1801 407 1 ( 441/1597- 759/1780) 5.1 E36-W10 N56-N64
2 1165 1329 (N20W17 L= 85) 513 151 2 (1087/1304-1238/1347) -26.6 W12-W20 N17-N22
3 1860 1211 (S08W62 L=131) 1755 232 4 (1806/1142-1898/1285) -73.3 W56-W69 S12-S02
4 1459 1174 (N03W29 L= 97) 409 149 0 (1442/1113-1475/1260) 49.4 W26-W32 N00-N07
5 407 1210 (N32E37 L= 32) 344 64 1 ( 369/1190- 441/1232) -33.7 E40-E33 N30-N34
6 229 1121 (N30E56 L= 12) 566 126 1 ( 182/1102- 285/1151) -8.7 E62-E49 N28-N32
7 1872 1075 (S16W59 L=128) 2867 168 5 (1792/1008-1932/1136) -36.3 W51-W68 S21-S10
8 810 1047 (N13E11 L= 57) 480 179 0 ( 754/ 981- 879/1079) 6.3 E16-E07 N10-N14
9 1712 966 (S16W41 L=109) 910 235 1 (1679/ 855-1737/1055) 81.3 W38-W42 S23-S10
10 647 1015 (N15E22 L= 46) 365 146 0 ( 588/ 992- 701/1043) -29.7 E25-E18 N14-N18
11 1805 939 (S21W49 L=117) 950 164 3 (1765/ 868-1856/1010) 41.2 W44-W55 S24-S17
12 497 976 (N16E33 L= 35) 355 128 0 ( 435/ 949- 558/1002) -32.0 E37-E29 N13-N19
13 221 825 (N13E61 L= 7) 780 88 5 ( 194/ 787- 247/ 862) -78.7 E65-E56 N10-N15
14 549 634 (S04E39 L= 29) 348 65 0 ( 524/ 610- 581/ 662) -14.0 E40-E36 S05-S02
15 1701 574 (S41W36 L=105) 2044 205 4 (1630/ 518-1761/ 658) 19.7 W28-W42 S45-S36
16 553 515 (S11E43 L= 25) 463 144 0 ( 515/ 447- 589/ 569) 82.9 E44-E41 S15-S07
17 439 396 (S17E61 L= 8) 1847 171 5 ( 374/ 344- 502/ 452) -66.0 E66-E54 S21-S11
18 1268 354 (S41E05 L= 63) 1661 288 5 (1161/ 292-1406/ 431) 0.0 E15-W07 S44-S38
19 960 184 (S45E38 L= 30) 1218 131 2 ( 905/ 151-1022/ 224) 4.1 E45-E30 S48-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20251001 ...
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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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