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| 20241228 - Filament data for 08 UTC |
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Available data for 20241228: »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 1530 1611 (N33W42 L=166) 941 132 1 (1480/1558-1577/1643) -50.2 W37-W45 N29-N35
2 713 1558 (N32E20 L=105) 882 252 0 ( 630/1462- 780/1629) -40.2 E27-E14 N25-N37
3 988 1538 (N29E00 L=124) 901 269 4 ( 887/1482-1126/1583) -18.4 E07-W08 N25-N32
4 863 1334 (N17E09 L=116) 367 192 0 ( 798/1260- 908/1381) -53.1 E12-E06 N11-N19
5 1272 1314 (N14W16 L=141) 366 108 4 (1235/1268-1316/1351) -56.3 W14-W18 N10-N16
6 850 1219 (N10E10 L=115) 333 116 1 ( 831/1160- 871/1275) 81.9 E10-E08 N06-N13
7 1800 1077 (S01W53 L=178) 2480 540 6 (1692/ 954-1896/1158) -23.6 W43-W64 S08-N03
8 392 970 (S03E41 L= 84) 366 54 3 ( 369/ 936- 413/1003) -63.4 E42-E39 S04-N00
9 1343 922 (S10W19 L=144) 247 132 0 (1281/ 882-1391/ 951) -35.5 W15-W22 S12-S07
10 453 863 (S09E37 L= 87) 1493 279 10 ( 366/ 811- 581/ 937) -21.8 E43-E28 S12-S04
11 1646 851 (S15W41 L=165) 2532 417 5 (1487/ 744-1766/ 928) 18.4 W28-W50 S21-S10
12 235 771 (S14E58 L= 66) 1600 346 3 ( 133/ 633- 305/ 892) -64.8 E69-E53 S22-S05
13 1723 685 (S25W50 L=175) 697 198 1 (1644/ 611-1784/ 754) 42.0 W44-W55 S29-S20
14 476 680 (S21E39 L= 86) 341 75 2 ( 460/ 645- 493/ 724) 78.7 E40-E36 S22-S17
15 1012 642 (S26E02 L=122) 355 120 0 ( 978/ 605-1033/ 698) 51.3 E04-W00 S28-S22
16 241 607 (S23E65 L= 59) 845 79 1 ( 199/ 588- 283/ 631) -4.8 E72-E60 S24-S21
17 661 455 (S36E31 L= 94) 315 64 1 ( 645/ 422- 679/ 491) 78.7 E32-E28 S38-S33
18 592 380 (S42E40 L= 84) 1016 155 3 ( 530/ 324- 648/ 437) 29.7 E49-E33 S45-S37
19 921 222 (S58E17 L=108) 1543 309 3 ( 771/ 182-1054/ 269) -12.1 E30-E02 S62-S51
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Download FITS filament maps as tar archive
» All Filament Data of 20241228 ...
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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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