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| 20250918 - Filament data for 10 UTC |
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Available data for 20250918: »06 UTC »07 UTC »08 UTC »09 UTC »10 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 1406 1784 (N38W62 L=299) 417 66 0 (1390/1753-1435/1804) 5.7 W56-W66 N37-N39
2 1719 1488 (N12W62 L=300) 1503 196 4 (1616/1450-1805/1538) -34.5 W54-W71 N07-N18
3 1030 1360 (N26W09 L=247) 659 202 2 ( 938/1315-1109/1414) -52.1 W04-W13 N21-N31
4 1069 1264 (N19W09 L=247) 415 171 0 ( 986/1235-1145/1283) -11.3 W03-W13 N17-N20
5 1619 1148 (S02W39 L=276) 751 155 0 (1593/1068-1645/1209) 45.0 W35-W41 S06-N01
6 1083 1077 (N09W05 L=242) 283 141 0 (1048/1017-1117/1141) 35.5 W01-W08 N06-N11
7 329 1069 (N25E46 L=192) 307 50 1 ( 298/1044- 351/1094) -36.9 E48-E43 N22-N26
8 267 910 (N16E54 L=184) 573 108 0 ( 232/ 862- 298/ 946) -51.3 E57-E51 N13-N18
9 1868 876 (S26W57 L=294) 827 112 3 (1822/ 848-1901/ 910) 7.1 W50-W62 S27-S23
10 200 854 (N14E63 L=175) 703 98 3 ( 176/ 813- 221/ 902) -68.2 E66-E60 N11-N16
11 471 851 (N09E38 L=200) 412 64 0 ( 444/ 812- 499/ 886) -68.2 E39-E36 N06-N11
12 249 786 (N09E59 L=179) 577 65 1 ( 218/ 759- 292/ 807) 0.0 E62-E54 N07-N10
13 444 541 (S08E50 L=187) 650 163 0 ( 395/ 474- 471/ 596) -90.0 E53-E48 S12-S04
14 1402 401 (S42W08 L=246) 3367 666 1 (1140/ 244-1650/ 575) 9.3 E18-W31 S48-S36
15 1197 522 (S27E03 L=235) 365 70 0 (1178/ 485-1219/ 569) 80.5 E04-E02 S29-S23
16 654 478 (S16E38 L=200) 807 187 2 ( 612/ 410- 711/ 546) 84.3 E40-E34 S21-S11
17 789 431 (S22E31 L=207) 510 110 0 ( 740/ 403- 820/ 473) 8.1 E34-E27 S23-S19
18 380 365 (S19E72 L=166) 949 50 1 ( 359/ 336- 399/ 392) 16.4 E83-E66 S22-S17
19 766 227 (S37E47 L=191) 459 67 0 ( 749/ 195- 782/ 265) 33.7 E51-E42 S39-S33
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Download FITS filament maps as tar archive
» All Filament Data of 20250918 ...
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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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