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| 20251028 - Filament data for 08 UTC |
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Available data for 20251028: »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
1 652 1754 (N63E06 L= 65) 445 54 1 ( 627/1726- 681/1775) 0.0 E09-E01 N60-N64
2 1490 1686 (N28W55 L=126) 1145 192 2 (1432/1605-1539/1759) 50.7 W49-W58 N23-N34
3 373 1639 (N62E51 L= 20) 640 98 0 ( 331/1614- 407/1663) 3.8 E61-E42 N60-N64
4 1578 1601 (N21W55 L=127) 453 37 0 (1549/1586-1611/1617) -18.4 W52-W58 N19-N22
5 1285 1498 (N24W29 L=100) 239 52 1 (1250/1482-1315/1510) -36.9 W27-W31 N22-N25
6 1057 1400 (N25W12 L= 83) 1294 235 3 ( 956/1336-1164/1430) -30.3 W06-W18 N21-N28
7 1373 1183 (N05W23 L= 95) 406 155 0 (1307/1159-1423/1223) -7.1 W19-W27 N03-N07
8 1736 1078 (S11W45 L=117) 296 63 0 (1709/1056-1766/1105) -45.0 W43-W47 S13-S09
9 1853 1040 (S17W56 L=127) 769 128 1 (1832/ 978-1891/1096) 32.0 W52-W62 S20-S14
10 649 1027 (N14E21 L= 50) 241 87 1 ( 601/1009- 688/1046) -9.5 E24-E18 N12-N14
11 907 966 (N04E08 L= 63) 291 33 0 ( 882/ 943- 930/ 990) 33.7 E09-E06 N03-N05
12 1827 761 (S33W51 L=122) 1060 206 0 (1777/ 669-1878/ 856) 45.0 W45-W57 S38-S28
13 694 722 (S04E26 L= 45) 1091 312 1 ( 562/ 643- 791/ 827) 14.0 E37-E17 S06-N00
14 206 721 (N05E66 L= 6) 526 48 0 ( 180/ 699- 232/ 745) -31.0 E68-E62 N03-N07
15 1661 568 (S41W33 L=104) 328 46 0 (1647/ 544-1677/ 597) -76.0 W31-W34 S42-S38
16 349 509 (S09E61 L= 10) 590 78 1 ( 326/ 470- 369/ 543) 33.7 E65-E56 S11-S07
17 1491 483 (S41W16 L= 88) 473 130 0 (1447/ 439-1535/ 534) 26.6 W12-W20 S42-S38
18 407 400 (S17E63 L= 8) 696 85 3 ( 374/ 377- 435/ 427) -76.0 E67-E58 S19-S15
19 1006 245 (S43E28 L= 43) 708 110 1 ( 949/ 227-1067/ 272) -5.2 E33-E22 S44-S40
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Download FITS filament maps as tar archive
» All Filament Data of 20251028 ...
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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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