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| 20240908 - Filament data for 09 UTC |
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Available data for 20240908: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 923 1649 (N47W13 L=161) 354 116 0 ( 889/1605- 966/1691) 21.8 W08-W18 N45-N49
2 1007 1384 (N28W08 L=156) 574 191 1 ( 917/1318-1067/1438) 9.5 W01-W13 N26-N30
3 1148 1239 (N16W12 L=160) 209 105 0 (1096/1223-1190/1264) -9.5 W09-W15 N15-N17
4 1858 1104 (S12W59 L=207) 3927 482 10 (1785/ 873-1931/1261) 39.3 W47-W72 S22-S04
5 702 1196 (N24E16 L=132) 871 219 1 ( 610/1137- 787/1252) 4.4 E22-E09 N22-N26
6 416 1107 (N25E38 L=110) 464 108 0 ( 365/1064- 461/1144) 12.5 E42-E33 N23-N26
7 516 1003 (N17E32 L=116) 272 88 0 ( 484/ 961- 546/1032) -68.2 E33-E30 N13-N18
8 1560 993 (S08W31 L=179) 250 58 2 (1531/ 965-1588/1016) -45.0 W29-W32 S09-S06
9 1486 814 (S16W22 L=170) 2465 529 5 (1299/ 702-1630/ 954) 8.7 W08-W34 S20-S11
10 1438 872 (S12W20 L=168) 408 88 2 (1417/ 830-1456/ 915) -90.0 W18-W21 S14-S08
11 525 601 (S07E41 L=107) 959 256 1 ( 418/ 532- 614/ 686) -50.7 E46-E36 S12-N00
12 1543 611 (S31W23 L=171) 686 195 0 (1463/ 561-1611/ 679) 13.0 W16-W29 S32-S28
13 1258 523 (S28W02 L=150) 290 105 0 (1244/ 466-1275/ 572) 63.4 W00-W03 S32-S25
14 1146 447 (S30E08 L=140) 2199 501 6 (1054/ 314-1229/ 559) 41.2 E17-E01 S39-S23
15 811 424 (S23E29 L=119) 622 164 2 ( 764/ 369- 850/ 497) 32.5 E35-E24 S26-S19
16 1102 415 (S31E12 L=136) 513 171 0 (1024/ 391-1150/ 467) 0.0 E16-E06 S33-S28
17 647 373 (S23E44 L=104) 1155 238 2 ( 591/ 296- 724/ 460) 85.9 E47-E40 S30-S16
18 1414 364 (S46W09 L=157) 551 91 1 (1372/ 336-1454/ 393) 0.0 W05-W13 S48-S43
19 1040 145 (S54E36 L=112) 979 91 2 ( 999/ 115-1079/ 175) -14.0 E42-E29 S58-S49
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Download FITS filament maps as tar archive
» All Filament Data of 20240908 ...
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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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