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| 20260616 - Filament data for 10 UTC |
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Available data for 20260616: »06 UTC »07 UTC »08 UTC »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 1255 1509 (N34W10 L=274) 1051 219 4 (1184/1431-1312/1573) -41.6 W04-W14 N29-N38
2 349 1465 (N20E57 L=206) 786 159 1 ( 332/1390- 364/1535) -52.1 E61-E52 N15-N24
3 522 1430 (N20E40 L=223) 511 94 2 ( 498/1379- 553/1476) -50.2 E42-E36 N16-N23
4 1771 1375 (N31W56 L=320) 672 94 0 (1754/1326-1785/1421) 66.8 W54-W60 N27-N34
5 429 1166 (N03E40 L=223) 464 111 0 ( 378/1140- 483/1186) 0.0 E44-E36 N01-N04
6 1553 1159 (N15W33 L=296) 237 47 0 (1536/1131-1575/1180) 56.3 W31-W34 N13-N16
7 192 1073 (S06E62 L=201) 931 136 1 ( 147/1020- 233/1115) -18.4 E69-E56 S08-S03
8 1398 1078 (N08W23 L=286) 401 93 1 (1381/1027-1432/1110) 90.0 W21-W24 N05-N10
9 917 1011 (S01E06 L=257) 273 71 0 ( 902/ 972- 932/1045) -76.0 E07-E05 S03-N01
10 396 926 (S12E41 L=222) 656 164 0 ( 340/ 889- 461/ 994) -26.6 E45-E35 S13-S08
11 674 744 (S20E19 L=244) 630 218 0 ( 646/ 681- 720/ 823) 77.5 E21-E16 S23-S14
12 1037 728 (S17W04 L=267) 425 109 0 ( 996/ 695-1083/ 766) 45.0 W01-W06 S19-S13
13 1809 678 (S12W65 L=328) 474 57 0 (1790/ 647-1823/ 711) 90.0 W62-W66 S13-S09
14 1844 647 (S14W73 L=336) 1123 94 0 (1814/ 612-1875/ 674) 24.0 W68-W78 S15-S11
15 888 625 (S25E04 L=259) 314 67 1 ( 859/ 594- 921/ 658) 59.0 E06-E02 S27-S22
16 707 611 (S28E17 L=246) 339 84 0 ( 666/ 596- 760/ 630) -8.1 E19-E12 S29-S27
17 311 585 (S36E55 L=208) 1035 134 2 ( 243/ 547- 374/ 611) -6.7 E66-E47 S37-S33
18 1370 512 (S27W31 L=294) 257 5 0 (1352/ 494-1387/ 534) -71.6 W29-W32 S28-S25
19 1224 484 (S31W21 L=284) 614 163 0 (1149/ 466-1301/ 512) 0.0 W15-W26 S31-S29
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Download FITS filament maps as tar archive
» All Filament Data of 20260616 ...
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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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