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| 20260616 - Filament data for 09 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 1248 1507 (N34W10 L=274) 1225 229 2 (1166/1421-1307/1574) -35.0 W03-W14 N28-N38
2 329 1396 (N16E56 L=208) 1287 328 0 ( 291/1242- 358/1527) -63.4 E62-E50 N06-N24
3 516 1435 (N20E40 L=223) 498 93 1 ( 492/1387- 549/1478) -50.2 E43-E37 N17-N23
4 1765 1376 (N31W56 L=320) 719 99 1 (1744/1321-1780/1420) 74.1 W53-W59 N27-N34
5 420 1167 (N03E41 L=223) 460 115 0 ( 369/1143- 476/1184) 0.0 E45-E36 N01-N03
6 1545 1159 (N15W32 L=296) 267 50 0 (1526/1131-1571/1182) 45.0 W31-W34 N13-N16
7 1820 1106 (N14W57 L=321) 463 107 0 (1804/1058-1833/1155) 80.5 W55-W59 N11-N17
8 192 1073 (S06E62 L=202) 890 103 1 ( 164/1018- 214/1120) -56.3 E66-E59 S08-S02
9 1389 1074 (N08W22 L=286) 443 123 1 (1371/1008-1425/1109) -80.5 W20-W24 N03-N10
10 482 1022 (S05E35 L=229) 256 115 0 ( 469/ 963- 499/1068) -71.6 E35-E33 S08-S02
11 907 1009 (S01E07 L=257) 295 67 0 ( 889/ 969- 925/1038) -71.6 E08-E05 S03-N00
12 387 931 (S12E41 L=222) 731 194 0 ( 317/ 892- 455/ 996) -18.4 E47-E35 S13-S08
13 687 741 (S20E19 L=245) 1031 323 0 ( 637/ 677- 769/ 830) -83.7 E21-E13 S23-S14
14 1027 733 (S17W03 L=267) 469 111 1 ( 989/ 695-1075/ 768) 56.3 W01-W06 S19-S13
15 1816 662 (S13W67 L=331) 1613 156 5 (1783/ 612-1861/ 715) -31.0 W62-W76 S15-S09
16 888 628 (S25E04 L=260) 287 67 0 ( 862/ 595- 917/ 657) 59.0 E05-E02 S27-S22
17 700 611 (S28E17 L=247) 349 86 0 ( 661/ 597- 755/ 628) 0.0 E20-E13 S29-S27
18 326 577 (S36E53 L=211) 1268 199 1 ( 239/ 533- 421/ 611) -2.4 E67-E42 S38-S34
19 1270 496 (S29W24 L=288) 985 280 2 (1141/ 468-1383/ 542) 13.2 W14-W31 S31-S25
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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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