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| 20251110 - Latest Filament data |
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Available data for 20251110: »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 1370 1865 (N44W66 L=323) 950 72 1 (1344/1830-1391/1904) 10.8 W58-W79 N42-N46
2 1273 1841 (N46W52 L=309) 430 44 1 (1257/1814-1293/1864) 23.2 W48-W57 N43-N47
3 1329 1642 (N31W38 L=295) 712 105 0 (1277/1617-1388/1666) -39.8 W34-W41 N28-N34
4 1708 1490 (N13W59 L=316) 2079 226 6 (1617/1430-1811/1560) -45.0 W52-W67 N06-N18
5 440 1519 (N47E34 L=223) 768 91 1 ( 397/1488- 488/1544) 0.0 E38-E28 N44-N49
6 1290 1481 (N23W28 L=285) 294 96 0 (1250/1446-1324/1499) -53.1 W25-W29 N20-N24
7 783 1401 (N30E06 L=251) 856 246 1 ( 663/1380- 900/1417) -14.9 E14-W01 N27-N33
8 1263 1357 (N16W22 L=279) 338 178 0 (1187/1325-1340/1394) 0.0 W16-W27 N15-N17
9 1017 1118 (N09W02 L=259) 867 331 3 ( 901/1093-1196/1151) -17.4 E05-W11 N04-N11
10 1675 1064 (S10W41 L=298) 750 172 0 (1626/ 992-1717/1135) -68.2 W38-W42 S14-S04
11 216 975 (N17E57 L=200) 1635 335 3 ( 112/ 858- 306/1102) -40.4 E71-E49 N08-N25
12 1833 1024 (S16W54 L=311) 460 70 1 (1816/ 986-1849/1064) 36.9 W51-W56 S18-S13
13 439 788 (N02E41 L=216) 430 57 1 ( 414/ 755- 476/ 819) 11.3 E43-E38 N00-N04
14 884 747 (S09E14 L=243) 460 105 2 ( 841/ 701- 914/ 792) -71.6 E15-E12 S11-S05
15 1542 607 (S34W24 L=281) 753 131 1 (1484/ 570-1602/ 648) 5.7 W19-W29 S35-S31
16 869 611 (S17E19 L=238) 215 66 2 ( 846/ 589- 892/ 643) -76.0 E19-E17 S18-S14
17 518 427 (S20E50 L=207) 814 162 1 ( 478/ 374- 569/ 488) 82.9 E52-E47 S24-S16
18 513 322 (S27E59 L=198) 1468 249 3 ( 414/ 288- 602/ 386) 3.6 E78-E46 S29-S24
19 883 200 (S45E40 L=217) 1269 139 1 ( 820/ 163- 944/ 247) 3.6 E48-E32 S48-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20251110 ...
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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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