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| 20251110 - Filament data for 12 UTC |
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Available data for 20251110: »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 1366 1864 (N44W65 L=322) 950 70 2 (1339/1830-1386/1903) 7.8 W57-W79 N42-N46
2 1270 1840 (N46W52 L=309) 431 31 1 (1255/1811-1286/1864) 29.7 W48-W56 N43-N47
3 1318 1644 (N32W37 L=295) 808 113 0 (1267/1619-1380/1673) -56.3 W34-W40 N28-N34
4 1705 1486 (N13W58 L=316) 2120 227 4 (1610/1426-1810/1557) -38.2 W51-W67 N06-N18
5 432 1520 (N47E34 L=223) 689 88 1 ( 391/1488- 483/1542) -10.3 E39-E28 N45-N49
6 1288 1473 (N22W27 L=285) 339 107 0 (1244/1437-1323/1496) -59.0 W25-W28 N19-N24
7 768 1399 (N31E07 L=250) 1042 303 1 ( 613/1378- 903/1414) -18.4 E17-W01 N27-N34
8 1259 1354 (N16W21 L=279) 345 174 0 (1186/1323-1333/1388) 0.0 W16-W26 N15-N17
9 1013 1117 (N09W01 L=259) 975 350 2 ( 893/1091-1190/1153) -17.4 E05-W11 N04-N11
10 1668 1062 (S09W40 L=297) 750 175 0 (1623/ 993-1711/1134) -68.2 W37-W42 S14-S04
11 1828 1022 (S16W53 L=311) 453 85 2 (1811/ 974-1844/1064) 51.3 W51-W55 S18-S13
12 238 942 (N15E55 L=203) 1113 202 1 ( 167/ 852- 303/1005) -39.8 E62-E49 N08-N19
13 434 781 (N02E41 L=216) 462 84 2 ( 405/ 752- 471/ 807) 0.0 E43-E38 N00-N03
14 884 732 (S10E15 L=243) 334 57 2 ( 861/ 696- 907/ 761) -90.0 E16-E12 S12-S08
15 1539 605 (S34W24 L=281) 750 136 1 (1477/ 571-1597/ 646) 5.7 W18-W28 S35-S31
16 866 604 (S17E19 L=238) 293 80 2 ( 837/ 575- 907/ 640) -53.1 E20-E17 S19-S14
17 515 428 (S20E50 L=208) 961 149 3 ( 472/ 372- 564/ 477) -90.0 E53-E46 S24-S16
18 512 321 (S27E59 L=199) 1494 246 5 ( 414/ 282- 603/ 393) 0.0 E79-E46 S29-S23
19 886 205 (S45E39 L=218) 1461 169 1 ( 817/ 160- 944/ 261) 14.0 E49-E29 S47-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20251110 ...
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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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