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| 20231229 - Filament data for 07 UTC |
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Available data for 20231229: »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 1150 1808 (N52W16 L=279) 425 41 0 (1132/1783-1169/1836) 63.4 W14-W18 N49-N55
2 1204 1754 (N47W19 L=282) 888 95 2 (1156/1718-1261/1792) -12.5 W14-W24 N43-N50
3 1586 1652 (N37W51 L=314) 1594 175 1 (1489/1630-1673/1673) 2.2 W40-W66 N35-N39
4 1561 1441 (N22W39 L=302) 7727 1039 10 (1127/1169-1903/1617) -25.4 W09-W69 N05-N35
5 1495 1344 (N16W32 L=295) 437 131 0 (1476/1288-1521/1404) 81.9 W30-W33 N12-N19
6 774 1349 (N18E15 L=248) 660 140 2 ( 707/1302- 832/1403) -36.9 E19-E11 N14-N21
7 1871 1313 (N14W69 L=331) 784 131 1 (1838/1283-1899/1346) -12.5 W64-W74 N12-N16
8 1712 1250 (N10W48 L=311) 319 63 0 (1701/1213-1728/1284) 76.0 W46-W49 N07-N11
9 1622 1250 (N10W40 L=303) 285 48 0 (1598/1227-1648/1277) 36.9 W38-W42 N08-N11
10 363 1197 (N11E44 L=219) 278 54 0 ( 336/1173- 391/1218) 26.6 E46-E41 N09-N11
11 925 1190 (N08E05 L=257) 212 56 0 ( 897/1163- 950/1215) -45.0 E07-E04 N05-N09
12 1866 871 (S13W64 L=326) 2759 277 1 (1803/ 753-1931/1002) 60.6 W57-W72 S20-S04
13 1573 795 (S18W36 L=299) 764 253 0 (1533/ 691-1638/ 903) 69.0 W33-W40 S24-S11
14 373 770 (S15E46 L=217) 643 169 0 ( 297/ 745- 448/ 794) -8.7 E52-E39 S16-S13
15 1243 594 (S30W14 L=276) 236 72 0 (1214/ 564-1276/ 624) 36.9 W11-W16 S32-S28
16 1739 522 (S36W63 L=325) 2420 273 0 (1632/ 473-1828/ 624) 29.1 W50-W72 S39-S28
17 1447 467 (S40W32 L=295) 673 111 2 (1401/ 429-1489/ 507) -11.3 W27-W37 S42-S36
18 1186 476 (S38W10 L=273) 278 38 2 (1167/ 450-1207/ 499) -76.0 W08-W11 S40-S36
19 1091 441 (S41W03 L=266) 479 74 1 (1053/ 420-1131/ 469) -18.4 W00-W06 S42-S38
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Download FITS filament maps as tar archive
» All Filament Data of 20231229 ...
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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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