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| 20250724 - Filament data for 10 UTC |
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Available data for 20250724: »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1518 1653 (N40W52 L=310) 489 39 2 (1491/1627-1543/1674) -9.5 W48-W55 N38-N41
2 1066 1600 (N42W09 L=267) 757 189 0 ( 971/1578-1150/1615) -8.1 W01-W15 N39-N43
3 1336 1558 (N36W29 L=287) 381 113 1 (1276/1541-1385/1576) 0.0 W24-W33 N34-N37
4 1206 1352 (N24W15 L=273) 676 277 2 (1091/1283-1310/1410) -34.7 W07-W20 N18-N28
5 233 1353 (N29E65 L=193) 1012 101 3 ( 204/1312- 269/1401) -21.0 E73-E58 N26-N31
6 1748 1233 (N10W53 L=311) 1232 243 1 (1671/1142-1802/1288) -51.3 W46-W57 N04-N14
7 1172 1128 (N10W10 L=268) 338 89 2 (1148/1085-1211/1156) 36.9 W08-W12 N07-N11
8 461 1105 (N13E37 L=221) 250 77 0 ( 446/1068- 477/1150) -68.2 E38-E35 N10-N15
9 654 1104 (N12E23 L=235) 562 228 1 ( 553/1052- 740/1142) -26.6 E29-E17 N08-N14
10 831 928 (N01E12 L=245) 240 77 0 ( 810/ 891- 851/ 969) -76.0 E13-E11 S01-N03
11 1046 859 (S05W00 L=258) 289 102 1 (1033/ 809-1062/ 913) 80.5 W00-W01 S08-S01
12 260 760 (S08E58 L=200) 907 100 2 ( 224/ 718- 294/ 807) -50.2 E61-E54 S10-S04
13 310 674 (S13E55 L=203) 408 84 0 ( 282/ 655- 346/ 693) 0.0 E58-E51 S14-S12
14 923 622 (S19E10 L=248) 326 52 1 ( 906/ 589- 951/ 658) 78.7 E10-E07 S21-S16
15 341 587 (S19E55 L=203) 585 60 1 ( 312/ 554- 369/ 616) 76.0 E57-E52 S21-S17
16 1749 554 (S33W57 L=315) 549 47 0 (1727/ 526-1766/ 580) -39.8 W53-W61 S35-S30
17 1337 339 (S45W20 L=278) 472 60 1 (1318/ 310-1357/ 376) 90.0 W18-W22 S47-S41
18 1137 288 (S47W02 L=260) 1440 253 4 (1020/ 256-1251/ 323) 0.0 E08-W12 S49-S44
19 878 218 (S52E24 L=234) 1385 177 2 ( 797/ 197- 959/ 253) -11.3 E33-E15 S54-S48
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Download FITS filament maps as tar archive
» All Filament Data of 20250724 ...
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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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