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| 20251003 - Filament data for 12 UTC |
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Available data for 20251003: »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
1 882 1826 (N61W27 L= 66) 1149 196 3 ( 823/1773- 928/1892) 12.5 W16-W43 N56-N65
2 1247 1734 (N40W43 L= 82) 283 54 1 (1224/1711-1275/1758) -90.0 W41-W45 N37-N41
3 1537 1715 (N28W64 L=103) 612 59 2 (1509/1693-1564/1739) -56.3 W60-W67 N26-N29
4 1461 1548 (N22W44 L= 83) 1192 278 5 (1312/1509-1576/1587) -36.3 W36-W51 N17-N29
5 1769 1389 (N04W60 L= 99) 864 190 1 (1747/1306-1796/1482) 45.0 W57-W66 N00-N08
6 1249 1265 (N14W19 L= 58) 234 103 0 (1232/1217-1262/1313) 59.0 W16-W20 N11-N16
7 1008 1268 (N20W06 L= 44) 194 83 0 ( 991/1233-1040/1301) 36.9 W03-W08 N18-N21
8 1162 1217 (N13W13 L= 51) 1017 411 6 (1020/1156-1316/1296) -38.2 W04-W20 N06-N19
9 529 1230 (N30E26 L= 13) 370 105 0 ( 477/1211- 577/1256) 0.0 E30-E21 N29-N31
10 1915 1212 (S11W71 L=109) 654 95 1 (1889/1182-1939/1237) -63.4 W65-W75 S12-S08
11 931 1162 (N17E02 L= 37) 381 157 0 ( 851/1149-1009/1175) -32.0 E06-W02 N13-N19
12 406 1130 (N27E37 L= 1) 811 212 0 ( 306/1106- 509/1157) -22.4 E46-E29 N23-N30
13 1181 902 (S04W05 L= 44) 352 89 0 (1144/ 879-1225/ 921) 0.0 W03-W08 S05-S02
14 956 809 (S03E09 L= 29) 456 192 0 ( 896/ 761-1041/ 856) 11.3 E13-E03 S04-S02
15 944 685 (S10E13 L= 25) 395 129 0 ( 906/ 621- 975/ 745) 83.7 E14-E12 S14-S05
16 483 383 (S18E57 L=342) 1820 310 2 ( 457/ 272- 520/ 538) 34.7 E72-E45 S26-S08
17 1546 498 (S41W20 L= 59) 774 84 3 (1496/ 467-1590/ 526) 0.0 W15-W24 S42-S38
18 777 468 (S19E31 L= 8) 1048 294 1 ( 665/ 428- 898/ 525) -31.6 E35-E22 S23-S13
19 1157 262 (S45E18 L= 21) 1666 320 3 (1034/ 178-1298/ 349) 8.1 E32-E03 S49-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20251003 ...
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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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