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| 20241110 - Filament data for 13 UTC |
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Available data for 20241110: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1502 1613 (N24W49 L= 84) 3428 581 4 (1264/1479-1740/1681) -33.7 W31-W62 N10-N31
2 1714 1614 (N18W70 L=105) 3185 216 4 (1615/1547-1801/1677) -53.1 W62-W82 N12-N24
3 670 1573 (N45E10 L= 24) 268 38 1 ( 643/1556- 697/1589) -26.6 E12-E07 N43-N46
4 1389 1504 (N21W35 L= 70) 263 87 0 (1344/1491-1436/1515) -31.0 W32-W37 N19-N22
5 1728 1213 (S03W49 L= 83) 310 53 0 (1711/1183-1747/1239) 71.6 W47-W50 S04-S01
6 1730 1117 (S09W46 L= 81) 1504 359 3 (1639/1046-1792/1183) -36.0 W39-W51 S12-S03
7 442 1134 (N22E34 L= 1) 749 189 1 ( 353/1075- 505/1179) -39.3 E40-E29 N17-N26
8 915 865 (S03E10 L= 25) 1849 489 5 ( 774/ 685-1056/1002) -62.2 E15-E05 S15-N05
9 1347 908 (S11W16 L= 50) 835 258 3 (1267/ 794-1390/ 992) 38.7 W08-W19 S15-S05
10 1221 897 (S08W08 L= 43) 434 130 3 (1191/ 833-1242/ 961) 54.5 W05-W10 S11-S04
11 1272 928 (S08W12 L= 46) 236 48 1 (1254/ 903-1297/ 954) 45.0 W10-W13 S09-S06
12 382 904 (N10E42 L=352) 607 146 1 ( 324/ 873- 451/ 946) -29.1 E46-E37 N07-N13
13 1475 676 (S28W19 L= 54) 1158 270 4 (1383/ 635-1579/ 724) -23.2 W13-W27 S29-S23
14 587 677 (S07E34 L= 1) 255 34 1 ( 564/ 651- 608/ 697) -33.7 E35-E32 S07-S05
15 1156 410 (S37E08 L= 26) 3654 686 6 (1005/ 196-1258/ 695) 45.9 E30-W02 S49-S18
16 572 600 (S11E38 L=357) 727 143 3 ( 512/ 562- 647/ 634) -26.6 E41-E32 S13-S07
17 538 419 (S21E49 L=346) 2868 478 6 ( 389/ 316- 656/ 562) 13.1 E77-E34 S24-S14
18 1068 338 (S39E17 L= 17) 247 76 0 (1061/ 294-1079/ 380) 50.2 E19-E14 S42-S36
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Download FITS filament maps as tar archive
» All Filament Data of 20241110 ...
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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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