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| 20240924 - Filament data for 11 UTC |
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Available data for 20240924: »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 1564 1698 (N27W65 L= 1) 550 77 1 (1520/1682-1604/1714) -18.4 W60-W70 N24-N28
2 1163 1443 (N26W21 L=316) 559 192 2 (1091/1417-1268/1462) -31.0 W16-W26 N22-N28
3 884 1392 (N31W02 L=298) 481 163 0 ( 813/1363- 968/1414) -18.4 E02-W07 N29-N32
4 437 1350 (N41E33 L=263) 587 133 0 ( 374/1322- 502/1371) 0.0 E39-E26 N39-N42
5 785 1167 (N21E10 L=286) 782 376 3 ( 635/1100- 950/1206) -11.3 E20-W00 N17-N23
6 1866 1110 (S14W60 L=355) 1579 202 0 (1792/1041-1902/1191) 10.0 W49-W66 S16-S09
7 1128 1096 (N08W07 L=303) 249 156 0 (1067/1033-1181/1136) -69.4 W05-W09 N03-N11
8 626 958 (N13E25 L=271) 948 258 5 ( 592/ 842- 680/1073) 81.9 E26-E22 N05-N19
9 1697 919 (S18W38 L=334) 294 62 0 (1673/ 891-1716/ 950) 45.0 W36-W40 S19-S16
10 359 563 (S04E57 L=238) 4147 547 15 ( 288/ 368- 454/ 831) 53.1 E71-E45 S17-N11
11 434 781 (N07E42 L=253) 552 96 2 ( 392/ 745- 474/ 811) -38.7 E45-E40 N04-N09
12 1642 749 (S27W31 L=327) 580 167 0 (1614/ 663-1675/ 811) 45.0 W27-W34 S31-S23
13 1165 604 (S20E03 L=292) 373 91 1 (1138/ 579-1196/ 636) 11.3 E05-W00 S22-S18
14 437 527 (S08E52 L=244) 298 36 1 ( 418/ 507- 459/ 550) -45.0 E53-E50 S09-S06
15 666 498 (S14E36 L=259) 874 234 2 ( 599/ 442- 780/ 541) -4.1 E42-E28 S17-S11
16 1092 469 (S27E12 L=284) 500 122 2 (1068/ 413-1114/ 532) 71.6 E14-E09 S31-S22
17 722 412 (S21E37 L=259) 815 242 2 ( 622/ 364- 799/ 473) -8.7 E43-E29 S24-S17
18 700 359 (S24E41 L=254) 311 85 1 ( 674/ 333- 734/ 393) -78.7 E43-E40 S26-S21
19 941 192 (S44E39 L=257) 848 96 2 ( 912/ 151- 968/ 225) 22.6 E45-E33 S47-S40
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Download FITS filament maps as tar archive
» All Filament Data of 20240924 ...
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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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