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| 20250722 - Filament data for 08 UTC |
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Available data for 20250722: »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 1163 1563 (N38W15 L=301) 516 128 2 (1099/1528-1223/1604) 20.0 W09-W20 N36-N40
2 378 1573 (N43E59 L=226) 667 113 1 ( 328/1553- 430/1592) 3.6 E68-E52 N41-N44
3 1705 1449 (N25W57 L=343) 357 83 0 (1672/1435-1751/1460) -14.0 W53-W62 N23-N25
4 832 1250 (N20E11 L=275) 289 98 2 ( 794/1216- 876/1283) -45.0 E13-E08 N17-N22
5 1378 1173 (N11W23 L=309) 632 250 0 (1295/1092-1454/1212) -41.6 W18-W27 N05-N14
6 298 1098 (N12E51 L=235) 429 100 1 ( 263/1064- 336/1139) -29.7 E54-E47 N10-N14
7 1055 968 (N01W02 L=287) 938 356 0 (1003/ 816-1102/1125) -81.0 W00-W03 S08-N11
8 714 1065 (N09E19 L=266) 238 107 1 ( 697/1018- 756/1097) 45.0 E20-E16 N06-N11
9 1814 1009 (S03W57 L=342) 678 162 0 (1756/ 965-1854/1073) 20.0 W50-W61 S05-N00
10 184 1013 (N07E64 L=222) 435 82 1 ( 165/ 988- 208/1042) -36.9 E66-E60 N05-N08
11 1814 852 (S13W57 L=342) 405 72 1 (1797/ 817-1838/ 875) 36.9 W54-W59 S14-S11
12 205 733 (S11E66 L=219) 1796 262 4 ( 183/ 639- 228/ 863) 60.3 E75-E61 S17-S02
13 553 645 (S16E34 L=251) 320 23 0 ( 535/ 623- 576/ 669) -71.6 E35-E32 S17-S14
14 529 598 (S19E37 L=248) 460 62 1 ( 502/ 563- 565/ 635) -53.1 E38-E34 S21-S16
15 849 504 (S27E16 L=270) 342 102 0 ( 823/ 455- 879/ 554) 54.5 E18-E12 S30-S23
16 464 502 (S26E46 L=239) 400 105 1 ( 443/ 446- 482/ 542) 66.8 E47-E43 S30-S23
17 1454 490 (S33W28 L=314) 469 81 1 (1425/ 457-1483/ 526) 59.0 W26-W30 S35-S30
18 1404 358 (S44W27 L=312) 3070 315 7 (1278/ 292-1527/ 419) 7.4 W15-W39 S48-S37
19 846 261 (S47E24 L=262) 3390 505 9 ( 644/ 201-1077/ 328) 7.8 E53-E01 S53-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20250722 ...
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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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