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| 20240116 - Filament data for 11 UTC |
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Available data for 20240116: »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
1 728 1694 (N38E29 L=355) 2148 314 4 ( 569/1637- 860/1737) -9.8 E45-E16 N33-N40
2 1290 1649 (N38W15 L= 39) 313 83 0 (1250/1636-1331/1667) -18.4 W12-W18 N37-N39
3 1263 1541 (N30W13 L= 37) 289 91 0 (1215/1513-1301/1573) -26.6 W09-W15 N27-N31
4 1076 1371 (N17W01 L= 25) 904 231 1 (1018/1274-1124/1461) 76.0 E02-W03 N10-N22
5 271 1336 (N12E56 L=327) 337 47 0 ( 253/1310- 292/1365) -31.0 E58-E53 N09-N13
6 1280 1291 (N13W14 L= 38) 564 234 1 (1176/1239-1383/1339) -17.1 W07-W20 N10-N15
7 397 1304 (N10E44 L=340) 264 40 1 ( 380/1278- 423/1326) 18.4 E44-E41 N07-N10
8 488 1276 (N08E36 L=348) 301 125 1 ( 454/1245- 549/1293) 15.9 E38-E31 N06-N09
9 297 1174 (N01E50 L=333) 461 105 0 ( 258/1137- 334/1211) 26.6 E53-E47 N00-N03
10 552 1115 (S01E30 L=354) 376 94 0 ( 510/1078- 597/1153) 31.0 E32-E27 S03-N00
11 267 1006 (S09E52 L=331) 692 93 0 ( 250/ 948- 293/1054) 63.4 E54-E49 S11-S05
12 192 959 (S11E61 L=323) 431 65 2 ( 175/ 928- 209/ 993) 76.0 E63-E58 S13-S09
13 1307 972 (S06W17 L= 41) 186 19 1 (1287/ 951-1325/ 991) 63.4 W16-W18 S07-S04
14 157 908 (S14E66 L=317) 1048 130 4 ( 124/ 872- 212/ 963) -29.1 E71-E59 S16-S10
15 894 845 (S16E07 L= 17) 335 177 0 ( 813/ 820- 979/ 866) 11.3 E11-E01 S17-S14
16 225 629 (S32E68 L=316) 3020 220 1 ( 195/ 530- 263/ 738) 35.8 E83-E63 S37-S24
17 1840 672 (S18W68 L= 92) 682 139 3 (1815/ 633-1869/ 734) 74.1 W65-W71 S20-S13
18 1756 647 (S21W59 L= 82) 1588 173 2 (1719/ 558-1810/ 701) 78.7 W54-W63 S26-S16
19 1652 617 (S24W49 L= 73) 714 166 1 (1605/ 537-1696/ 681) -38.7 W43-W53 S28-S20
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Download FITS filament maps as tar archive
» All Filament Data of 20240116 ...
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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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