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| 20241229 - Filament data for 07 UTC |
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Available data for 20241229: »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
1 584 1673 (N42E35 L= 77) 636 65 0 ( 567/1626- 605/1718) -74.1 E37-E31 N38-N45
2 1628 1623 (N34W53 L=165) 1662 112 3 (1572/1585-1678/1658) -11.3 W47-W59 N31-N37
3 1226 1525 (N28W16 L=128) 1946 436 4 (1059/1458-1438/1597) -19.8 W04-W30 N22-N33
4 300 1515 (N32E59 L= 53) 580 43 1 ( 270/1494- 328/1536) -11.3 E64-E54 N30-N33
5 744 1465 (N26E17 L= 95) 252 62 0 ( 730/1430- 761/1498) 76.0 E18-E16 N23-N27
6 304 1350 (N20E51 L= 61) 356 69 2 ( 292/1309- 319/1390) -71.6 E53-E48 N17-N23
7 1066 1246 (N10W03 L=115) 343 108 1 (1047/1189-1088/1295) 71.6 W01-W04 N07-N13
8 1815 872 (S13W56 L=168) 7883 510 21 (1646/ 740-1931/1035) 33.1 W41-W71 S21-S03
9 579 944 (S06E28 L= 84) 643 185 3 ( 549/ 864- 606/1021) -77.5 E29-E26 S10-S01
10 1604 974 (S07W37 L=149) 238 67 0 (1569/ 963-1643/ 987) 0.0 W34-W40 S07-S06
11 517 943 (S06E32 L= 80) 243 73 1 ( 499/ 909- 542/ 975) -76.0 E33-E30 S07-S03
12 1718 900 (S12W47 L=159) 359 42 1 (1695/ 874-1746/ 917) 45.0 W44-W49 S13-S10
13 193 820 (S11E63 L= 49) 3470 321 6 ( 134/ 709- 269/ 912) 50.2 E72-E52 S17-S05
14 681 859 (S11E22 L= 90) 361 166 0 ( 610/ 841- 763/ 880) 5.7 E26-E16 S12-S10
15 382 722 (S18E46 L= 66) 2219 427 3 ( 292/ 616- 449/ 872) -86.4 E58-E39 S24-S08
16 1211 670 (S25W11 L=123) 456 155 1 (1163/ 608-1253/ 747) 58.0 W07-W13 S28-S20
17 1805 646 (S27W62 L=174) 479 47 0 (1781/ 619-1831/ 676) 56.3 W59-W65 S28-S25
18 755 423 (S40E24 L= 88) 2762 564 6 ( 568/ 285-1017/ 565) 19.8 E52-E02 S49-S30
19 1112 218 (S60W05 L=117) 922 96 1 (1076/ 181-1158/ 246) 29.1 W00-W10 S64-S57
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Download FITS filament maps as tar archive
» All Filament Data of 20241229 ...
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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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