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| 20241022 - Filament data for 06 UTC |
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Available data for 20241022: »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 1773 1550 (N11W74 L= 3) 838 94 3 (1746/1519-1802/1591) -90.0 W71-W79 N08-N13
2 1172 1500 (N27W23 L=312) 422 51 0 (1141/1470-1209/1526) 9.5 W20-W26 N25-N28
3 1572 1505 (N15W50 L=338) 1069 146 1 (1498/1476-1645/1525) -17.1 W43-W56 N13-N17
4 242 1331 (N43E55 L=233) 830 145 0 ( 192/1299- 318/1352) 0.0 E63-E44 N41-N44
5 1243 1251 (N12W18 L=307) 1398 452 0 (1075/1141-1423/1312) -46.7 W09-W25 N00-N18
6 1701 1257 (S01W48 L=337) 948 153 2 (1633/1219-1751/1285) -5.2 W41-W52 S03-N00
7 1825 1174 (S10W57 L=346) 1402 176 7 (1792/1076-1864/1237) 32.5 W51-W63 S14-S06
8 740 1109 (N17E14 L=275) 452 138 1 ( 717/1054- 771/1177) 82.9 E15-E12 N13-N21
9 1681 781 (S27W35 L=324) 2615 583 3 (1530/ 536-1821/ 993) 31.5 W19-W51 S39-S19
10 645 876 (N07E25 L=264) 619 90 3 ( 597/ 837- 701/ 912) -26.6 E28-E22 N04-N08
11 1310 678 (S22W07 L=296) 511 141 0 (1256/ 633-1362/ 736) 24.0 W02-W11 S23-S19
12 227 680 (N04E66 L=223) 1234 153 2 ( 165/ 653- 278/ 716) 0.0 E76-E58 N02-N05
13 666 576 (S11E33 L=256) 1240 333 1 ( 599/ 523- 749/ 671) -79.7 E36-E27 S15-S04
14 326 484 (S09E66 L=223) 7738 351 9 ( 246/ 361- 422/ 608) 80.0 E77-E59 S18-S01
15 575 432 (S17E46 L=242) 1338 298 5 ( 479/ 364- 684/ 527) -63.4 E51-E41 S23-S09
16 1147 502 (S28E08 L=281) 241 51 0 (1125/ 479-1168/ 523) 14.0 E09-E05 S29-S26
17 466 383 (S18E59 L=230) 1751 164 4 ( 422/ 308- 498/ 469) 36.3 E68-E52 S23-S12
18 1396 376 (S46W05 L=294) 416 93 0 (1373/ 334-1420/ 418) 56.3 W02-W07 S49-S43
19 965 301 (S36E28 L=260) 886 105 2 ( 922/ 264-1006/ 344) 20.6 E32-E24 S39-S33
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Download FITS filament maps as tar archive
» All Filament Data of 20241022 ...
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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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