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| 20251028 - Filament data for 10 UTC |
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Available data for 20251028: »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
1 665 1752 (N62E04 L= 66) 521 89 0 ( 640/1708- 692/1777) -90.0 E07-W00 N57-N65
2 1486 1702 (N29W56 L=126) 1561 242 1 (1391/1616-1550/1777) -85.2 W51-W61 N23-N35
3 1585 1605 (N21W56 L=126) 364 36 0 (1563/1589-1614/1621) -9.5 W53-W59 N19-N22
4 1293 1508 (N24W30 L=100) 308 78 0 (1249/1491-1335/1522) -31.0 W27-W32 N22-N25
5 1077 1417 (N25W14 L= 84) 1126 230 1 ( 965/1377-1175/1439) -26.6 W07-W20 N21-N29
6 1383 1190 (N05W24 L= 94) 399 167 1 (1321/1165-1438/1239) -7.1 W20-W28 N03-N07
7 1828 1155 (S10W56 L=126) 377 55 2 (1810/1123-1848/1184) 45.0 W54-W58 S11-S08
8 1746 1086 (S11W46 L=116) 356 64 2 (1716/1057-1778/1116) -51.3 W44-W48 S13-S08
9 1870 1071 (S16W59 L=129) 484 86 1 (1845/1032-1899/1101) 14.0 W55-W63 S17-S14
10 666 1035 (N14E20 L= 50) 224 81 0 ( 626/1020- 700/1057) -11.3 E22-E17 N12-N14
11 924 974 (N04E07 L= 63) 270 55 0 ( 893/ 953- 945/ 999) 14.0 E08-E04 N03-N05
12 1854 805 (S31W54 L=124) 591 115 0 (1826/ 760-1885/ 861) 35.5 W50-W58 S33-S28
13 709 729 (S04E25 L= 45) 1094 337 1 ( 559/ 643- 807/ 836) 13.4 E37-E16 S06-N00
14 228 715 (N05E63 L= 7) 665 105 0 ( 186/ 679- 282/ 750) -32.0 E67-E57 N01-N07
15 358 505 (S10E60 L= 10) 540 62 2 ( 341/ 476- 380/ 545) 33.7 E62-E56 S11-S07
16 1509 489 (S41W18 L= 88) 631 122 1 (1459/ 444-1550/ 534) 26.6 W13-W21 S43-S38
17 418 397 (S18E62 L= 8) 610 51 1 ( 393/ 374- 438/ 422) 56.3 E65-E58 S19-S16
18 1236 333 (S44E07 L= 63) 401 113 0 (1186/ 314-1294/ 347) -26.6 E10-E02 S45-S41
19 1017 249 (S43E27 L= 43) 698 120 1 ( 955/ 230-1079/ 277) -10.3 E32-E21 S44-S40
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Download FITS filament maps as tar archive
» All Filament Data of 20251028 ...
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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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