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| 20251008 - Filament data for 12 UTC |
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Available data for 20251008: »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
1 846 1815 (N62W23 L=356) 341 66 0 ( 827/1778- 863/1839) 40.6 W18-W26 N58-N64
2 1320 1773 (N39W52 L= 25) 887 128 2 (1242/1753-1384/1786) -24.4 W46-W58 N36-N42
3 642 1713 (N61E07 L=326) 328 31 2 ( 621/1692- 667/1735) -18.4 E09-E03 N59-N63
4 1661 1655 (N20W71 L= 43) 562 75 1 (1632/1626-1700/1680) -51.3 W68-W73 N17-N22
5 1313 1630 (N31W39 L= 12) 550 135 1 (1250/1597-1372/1673) 0.0 W33-W45 N30-N32
6 1359 1544 (N25W37 L= 10) 594 151 0 (1280/1526-1430/1562) -26.6 W31-W41 N22-N27
7 861 1532 (N40W05 L=338) 453 108 1 ( 825/1502- 904/1551) 0.0 W01-W08 N37-N41
8 1402 1431 (N18W34 L= 7) 246 96 0 (1382/1385-1425/1475) 71.6 W33-W35 N14-N20
9 420 1384 (N43E34 L=299) 684 111 1 ( 369/1349- 476/1425) -28.6 E39-E28 N39-N46
10 1039 1323 (N22W09 L=342) 612 204 0 ( 966/1267-1105/1354) -40.6 W04-W12 N17-N25
11 1813 1259 (S04W58 L= 31) 812 90 2 (1784/1207-1846/1302) 18.4 W53-W64 S06-S02
12 154 1025 (N26E66 L=267) 1384 187 2 ( 109/ 947- 216/1096) -32.0 E74-E58 N20-N30
13 1598 947 (S14W31 L= 4) 276 45 0 (1574/ 925-1615/ 974) 18.4 W29-W32 S15-S12
14 1683 889 (S20W37 L= 9) 327 97 0 (1642/ 872-1731/ 910) -29.7 W33-W40 S21-S17
15 1328 710 (S19W09 L=342) 707 212 0 (1271/ 610-1366/ 793) 48.4 W03-W12 S23-S14
16 770 648 (S08E24 L=308) 758 211 0 ( 743/ 553- 807/ 750) 48.0 E28-E19 S13-S03
17 1755 565 (S45W44 L= 16) 492 59 1 (1720/ 552-1789/ 587) -20.0 W38-W49 S47-S42
18 768 438 (S21E33 L=300) 259 89 0 ( 755/ 392- 790/ 478) 45.0 E35-E29 S23-S18
19 859 276 (S34E36 L=296) 2713 436 5 ( 691/ 189-1028/ 396) 8.5 E58-E18 S38-S30
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Download FITS filament maps as tar archive
» All Filament Data of 20251008 ...
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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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