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| 20240814 - Filament data for 05 UTC |
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Available data for 20240814: »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1283 1802 (N51W51 L=171) 1591 229 1 (1177/1759-1382/1839) -5.9 W36-W66 N48-N52
2 1718 1324 (N10W54 L=174) 1284 349 1 (1579/1274-1861/1402) -6.2 W42-W79 N08-N13
3 1639 1140 (N02W42 L=162) 265 91 0 (1599/1113-1674/1170) 8.1 W38-W45 N00-N02
4 631 1074 (N16E24 L= 96) 463 183 2 ( 578/1004- 692/1148) -63.4 E27-E20 N10-N20
5 1826 1039 (S09W57 L=177) 1526 180 3 (1770/ 975-1863/1095) -45.0 W51-W62 S13-S05
6 1706 1034 (S06W45 L=165) 332 79 0 (1689/1000-1723/1072) 63.4 W43-W46 S07-S03
7 1712 965 (S10W44 L=165) 879 155 3 (1664/ 921-1754/1012) 23.2 W40-W48 S13-S07
8 1811 956 (S13W54 L=174) 400 82 0 (1764/ 934-1843/ 976) -26.6 W49-W58 S14-S10
9 1719 804 (S21W44 L=164) 1271 302 4 (1629/ 656-1801/ 894) 30.5 W35-W52 S28-S14
10 702 825 (S00E23 L= 97) 308 167 1 ( 678/ 748- 745/ 882) -90.0 E23-E21 S05-N03
11 1126 745 (S12W01 L=122) 632 238 2 (1047/ 703-1173/ 808) 20.6 E03-W05 S14-S08
12 460 696 (S05E43 L= 78) 272 86 1 ( 430/ 655- 490/ 722) 29.7 E46-E39 S07-S03
13 334 671 (S06E55 L= 66) 370 67 1 ( 305/ 643- 365/ 700) -36.9 E56-E51 S07-S03
14 840 592 (S17E19 L=101) 253 83 1 ( 806/ 571- 887/ 618) -11.3 E21-E16 S17-S15
15 379 479 (S19E60 L= 60) 1415 213 3 ( 336/ 395- 451/ 567) 85.6 E63-E57 S25-S12
16 909 519 (S23E17 L=104) 313 79 2 ( 891/ 476- 936/ 554) 68.2 E18-E14 S25-S20
17 1035 427 (S32E11 L=109) 704 145 2 ( 976/ 397-1109/ 456) 5.7 E15-E05 S32-S29
18 620 403 (S27E42 L= 79) 823 87 3 ( 588/ 350- 654/ 441) 49.4 E44-E38 S30-S23
19 1283 267 (S52W04 L=125) 635 108 0 (1245/ 243-1319/ 298) 20.6 W00-W08 S54-S49
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Download FITS filament maps as tar archive
» All Filament Data of 20240814 ...
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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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