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| 20231002 - Filament data for 10 UTC |
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Available data for 20231002: »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
1 999 1753 (N51W29 L= 11) 338 52 2 ( 978/1726-1024/1782) 29.7 W25-W32 N49-N53
2 1519 1643 (N25W57 L= 38) 777 98 1 (1475/1604-1550/1672) -80.5 W54-W59 N22-N28
3 1529 1538 (N20W49 L= 31) 419 114 0 (1496/1497-1547/1596) 32.0 W45-W54 N17-N22
4 1290 1503 (N26W31 L= 13) 431 108 0 (1238/1481-1342/1524) -56.3 W28-W34 N22-N28
5 1171 1389 (N23W19 L= 1) 756 270 1 (1059/1339-1268/1429) -30.3 W11-W23 N17-N26
6 961 1317 (N25W05 L=346) 213 104 0 ( 940/1279- 986/1364) 38.7 W02-W07 N22-N26
7 913 1250 (N22E00 L=341) 555 176 1 ( 871/1197- 972/1322) -84.3 E03-W01 N17-N27
8 402 1253 (N35E37 L=304) 1121 197 4 ( 325/1206- 488/1307) -29.4 E45-E29 N31-N40
9 564 1130 (N24E26 L=316) 328 84 0 ( 536/1098- 597/1166) -59.0 E27-E23 N21-N26
10 167 1019 (N25E66 L=275) 710 67 2 ( 149/ 988- 183/1059) -63.4 E69-E63 N23-N27
11 1738 944 (S19W43 L= 24) 986 228 1 (1712/ 841-1766/1051) 57.5 W39-W47 S24-S13
12 193 931 (N20E63 L=278) 2387 224 3 ( 138/ 850- 246/1038) 45.0 E72-E55 N15-N25
13 1450 877 (S13W20 L= 2) 881 297 0 (1392/ 768-1508/1019) 40.2 W14-W27 S18-S06
14 687 911 (N09E22 L=319) 495 166 0 ( 630/ 854- 749/ 972) -60.9 E24-E19 N04-N13
15 401 882 (N13E43 L=299) 324 79 0 ( 367/ 853- 426/ 901) -45.0 E45-E40 N11-N14
16 1201 626 (S21E01 L=341) 317 129 0 (1168/ 604-1253/ 666) -53.1 E02-W02 S22-S17
17 1448 606 (S30W14 L=356) 556 102 1 (1415/ 558-1487/ 644) 33.7 W11-W17 S32-S26
18 968 450 (S25E20 L=321) 452 189 0 ( 917/ 391-1033/ 519) 22.6 E25-E13 S28-S22
19 948 259 (S39E33 L=309) 624 123 0 ( 919/ 204- 971/ 321) 51.3 E37-E29 S43-S33
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Download FITS filament maps as tar archive
» All Filament Data of 20231002 ...
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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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