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| 20241007 - Filament data for 09 UTC |
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Available data for 20241007: »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 1633 1602 (N18W62 L=187) 450 22 0 (1613/1577-1651/1623) 11.3 W59-W65 N17-N19
2 1728 1545 (N12W67 L=192) 1559 165 6 (1674/1483-1784/1612) -90.0 W64-W72 N07-N16
3 1841 1366 (S01W67 L=193) 484 64 1 (1816/1340-1864/1389) 0.0 W63-W72 S01-N00
4 1231 1353 (N18W21 L=146) 533 127 0 (1171/1334-1299/1371) -26.6 W17-W25 N15-N20
5 1046 1274 (N19W08 L=133) 371 135 0 ( 986/1237-1094/1305) -51.3 W04-W10 N15-N21
6 1865 1135 (S13W60 L=185) 6159 387 14 (1787/1019-1953/1278) 82.4 W50-W78 S19-S04
7 424 1043 (N22E37 L= 88) 1756 371 2 ( 305/ 904- 537/1175) -56.3 E46-E31 N11-N32
8 1437 918 (S11W20 L=145) 808 365 0 (1397/ 759-1458/1096) 59.5 W14-W25 S18-S01
9 685 1053 (N17E19 L=107) 433 170 0 ( 619/1028- 786/1086) -31.0 E22-E12 N12-N19
10 1811 940 (S22W49 L=174) 347 68 1 (1792/ 919-1839/ 972) -90.0 W46-W52 S23-S19
11 1554 646 (S31W22 L=147) 3439 551 4 (1426/ 445-1702/ 879) 33.2 W08-W37 S40-S21
12 941 772 (S05E11 L=114) 227 63 1 ( 904/ 757- 970/ 791) -14.0 E13-E09 S06-S04
13 1345 776 (S16W11 L=136) 228 63 0 (1313/ 755-1378/ 790) -53.1 W09-W12 S18-S14
14 765 699 (S05E23 L=102) 415 136 0 ( 751/ 617- 784/ 757) 63.4 E25-E21 S09-S01
15 1179 633 (S20E02 L=123) 519 217 0 (1130/ 541-1227/ 715) 37.9 E07-W02 S23-S15
16 597 660 (S03E35 L= 91) 422 75 1 ( 557/ 628- 637/ 694) -68.2 E37-E32 S05-N00
17 483 665 (S00E42 L= 83) 367 122 1 ( 430/ 643- 535/ 684) -7.1 E46-E38 S02-N00
18 943 529 (S19E19 L=106) 923 337 2 ( 911/ 368- 999/ 674) 43.3 E27-E10 S29-S12
19 1006 392 (S30E21 L=104) 252 60 0 ( 965/ 379-1045/ 402) -31.0 E23-E18 S31-S28
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Download FITS filament maps as tar archive
» All Filament Data of 20241007 ...
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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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