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| 20231006 - Latest Filament data |
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Available data for 20231006: »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 1369 1839 (N41W68 L=355) 643 71 1 (1342/1813-1403/1870) -3.0 W61-W80 N40-N42
2 1569 1582 (N20W56 L=342) 1723 410 6 (1406/1469-1693/1717) -77.2 W52-W61 N10-N32
3 972 1554 (N38W14 L=301) 1319 316 5 ( 861/1512-1085/1588) -21.8 W06-W21 N33-N42
4 340 1519 (N56E50 L=237) 1226 138 2 ( 294/1478- 407/1543) 6.7 E61-E38 N53-N58
5 1280 1481 (N24W30 L=316) 476 137 1 (1221/1449-1343/1513) -54.5 W27-W32 N20-N27
6 1716 1413 (N07W57 L=344) 999 147 2 (1684/1352-1747/1485) 28.6 W51-W62 N04-N10
7 1404 1359 (N14W32 L=319) 358 53 1 (1375/1339-1436/1387) -71.6 W29-W33 N12-N15
8 1170 1232 (N14W14 L=301) 384 102 3 (1125/1200-1220/1264) -53.1 W11-W16 N11-N16
9 206 1177 (N35E60 L=227) 834 123 1 ( 161/1135- 251/1218) -21.8 E68-E53 N31-N37
10 780 1136 (N19E11 L=276) 372 97 1 ( 734/1097- 816/1172) -63.4 E13-E09 N16-N22
11 1717 1075 (S11W44 L=331) 339 46 0 (1699/1044-1735/1101) 56.3 W42-W45 S12-S09
12 1863 975 (S22W57 L=344) 442 96 0 (1827/ 958-1895/1000) -11.3 W52-W62 S23-S19
13 767 927 (N08E17 L=270) 396 152 1 ( 713/ 903- 829/ 977) 7.1 E20-E12 N06-N08
14 1614 718 (S29W29 L=316) 1038 314 2 (1553/ 594-1705/ 841) 34.5 W22-W38 S35-S23
15 1388 589 (S29W10 L=297) 1012 222 1 (1311/ 524-1450/ 682) 26.6 W03-W15 S32-S24
16 1718 585 (S42W39 L=326) 1349 118 1 (1683/ 534-1749/ 643) 66.8 W34-W42 S46-S37
17 690 532 (S13E34 L=253) 306 81 2 ( 659/ 513- 729/ 555) -63.4 E36-E31 S15-S11
18 1079 236 (S45E26 L=261) 1609 248 3 ( 963/ 180-1173/ 290) 4.8 E39-E15 S47-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20231006 ...
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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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