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| 20221106 - Filament data for 13 UTC |
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Available data for 20221106: »06 UTC »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
1 855 1866 (N66W25 L= 41) 750 69 1 ( 836/1824- 875/1899) 28.1 W19-W34 N60-N70
2 1159 1831 (N49W44 L= 60) 1007 151 1 (1109/1780-1211/1889) 9.9 W35-W58 N46-N52
3 762 1822 (N65W09 L= 25) 590 65 1 ( 735/1788- 783/1851) 63.4 W06-W15 N60-N68
4 891 1759 (N54W16 L= 32) 521 99 0 ( 845/1732- 933/1791) 5.2 W11-W22 N52-N55
5 1066 1709 (N44W26 L= 42) 610 109 1 (1040/1662-1093/1763) 37.9 W21-W30 N40-N47
6 830 1704 (N51W08 L= 24) 339 65 1 ( 794/1687- 868/1719) -45.0 W05-W10 N48-N53
7 1420 1655 (N29W47 L= 63) 296 44 1 (1404/1632-1437/1680) 53.1 W45-W48 N27-N31
8 1340 1593 (N28W37 L= 53) 538 98 0 (1297/1558-1385/1637) -71.6 W35-W39 N25-N31
9 1423 1413 (N16W34 L= 50) 223 40 0 (1400/1391-1442/1441) 33.7 W32-W36 N14-N17
10 1472 1350 (N11W35 L= 51) 704 132 1 (1441/1288-1509/1405) 36.9 W31-W39 N07-N13
11 794 1345 (N28E06 L= 10) 487 174 0 ( 726/1275- 828/1383) -69.4 E09-E04 N23-N31
12 1144 1345 (N19W15 L= 31) 534 201 0 (1046/1305-1228/1378) -37.9 W09-W19 N14-N23
13 988 1293 (N20W04 L= 20) 240 111 0 ( 936/1273-1036/1310) -38.7 W01-W06 N17-N21
14 248 1073 (N24E53 L=323) 592 104 0 ( 221/1019- 275/1114) -54.5 E55-E50 N19-N26
15 204 932 (N16E60 L=316) 1196 240 3 ( 174/ 830- 236/1011) 84.3 E64-E55 N10-N20
16 1363 903 (S11W16 L= 32) 295 92 0 (1317/ 887-1417/ 922) -45.0 W13-W19 S13-S08
17 668 578 (S14E33 L=343) 467 78 0 ( 649/ 530- 684/ 626) 56.3 E35-E30 S16-S10
18 1150 368 (S39E11 L= 5) 1416 299 0 (1049/ 278-1254/ 465) 20.0 E22-W00 S44-S35
19 1397 244 (S61W05 L= 21) 530 43 0 (1371/ 227-1425/ 264) 0.0 W01-W09 S63-S58
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Download FITS filament maps as tar archive
» All Filament Data of 20221106 ...
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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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