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| 20250809 - Filament data for 06 UTC |
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Available data for 20250809: »06 UTC »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
1 961 1770 (N58W12 L= 61) 455 61 1 ( 928/1743- 998/1788) 0.0 W08-W17 N55-N59
2 1672 1542 (N25W61 L=110) 457 77 1 (1651/1517-1701/1577) -90.0 W58-W63 N23-N27
3 1181 1484 (N32W19 L= 67) 280 136 0 (1123/1434-1227/1507) -50.2 W14-W20 N27-N34
4 238 1340 (N34E63 L=346) 3729 431 3 ( 163/1141- 338/1503) 66.5 E69-E56 N21-N44
5 992 1409 (N30W04 L= 52) 461 187 1 ( 933/1373-1074/1467) -45.0 W00-W08 N26-N34
6 1685 1308 (N12W50 L= 98) 930 214 2 (1650/1254-1754/1392) 76.0 W46-W56 N08-N16
7 1222 1362 (N24W18 L= 66) 199 75 1 (1191/1336-1255/1386) -53.1 W16-W19 N21-N25
8 347 1197 (N24E46 L= 2) 503 157 2 ( 296/1152- 382/1273) -41.6 E52-E42 N21-N29
9 652 1054 (N13E23 L= 26) 402 143 1 ( 580/1025- 709/1075) -20.6 E27-E19 N10-N14
10 1838 942 (S13W57 L=106) 1107 152 3 (1804/ 900-1870/1001) 39.8 W53-W61 S15-S09
11 256 917 (N08E56 L=353) 912 152 5 ( 206/ 850- 297/ 971) -36.9 E61-E52 N03-N11
12 644 938 (N06E25 L= 24) 227 76 0 ( 613/ 912- 664/ 969) 36.9 E26-E22 N04-N07
13 1395 794 (S13W20 L= 68) 393 93 1 (1355/ 768-1447/ 830) 9.5 W16-W23 S14-S11
14 508 577 (S15E42 L= 7) 846 235 2 ( 437/ 498- 550/ 675) 37.6 E50-E36 S19-S08
15 262 603 (S12E65 L=343) 725 68 2 ( 244/ 565- 283/ 645) 59.0 E68-E62 S14-S09
16 1395 393 (S42W18 L= 66) 465 67 2 (1364/ 371-1431/ 411) 0.0 W15-W21 S43-S39
17 1217 301 (S46W02 L= 51) 854 107 2 (1179/ 269-1273/ 330) 14.0 E01-W07 S48-S42
18 1049 253 (S47E14 L= 35) 344 21 0 (1028/ 232-1068/ 273) -63.4 E14-E11 S49-S45
19 1012 194 (S53E21 L= 28) 723 65 0 ( 984/ 168-1044/ 223) -59.0 E23-E17 S56-S49
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Download FITS filament maps as tar archive
» All Filament Data of 20250809 ...
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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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