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| 20231002 - Filament data for 09 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 1517 1638 (N25W56 L= 38) 717 89 0 (1480/1603-1544/1669) 59.0 W53-W59 N22-N27
2 1520 1528 (N19W48 L= 30) 339 73 0 (1503/1492-1536/1569) 29.7 W45-W52 N17-N21
3 1287 1496 (N25W31 L= 13) 357 119 0 (1231/1474-1340/1519) -50.2 W28-W33 N22-N28
4 1163 1388 (N23W19 L= 1) 673 261 2 (1050/1341-1252/1425) -32.5 W11-W22 N17-N26
5 225 1392 (N49E66 L=276) 612 87 0 ( 197/1352- 262/1416) 16.7 E70-E58 N46-N50
6 911 1239 (N21E01 L=341) 504 152 3 ( 872/1190- 965/1309) -90.0 E02-W01 N17-N26
7 397 1251 (N35E38 L=304) 1068 177 4 ( 322/1203- 481/1300) -31.0 E45-E30 N31-N40
8 554 1131 (N24E26 L=316) 357 87 1 ( 523/1094- 589/1170) -63.4 E27-E24 N21-N27
9 164 1018 (N25E66 L=275) 697 69 1 ( 147/ 986- 179/1057) -90.0 E69-E64 N23-N27
10 189 932 (N20E64 L=278) 2415 210 7 ( 136/ 845- 232/1038) 45.0 E72-E57 N14-N25
11 1444 880 (S13W20 L= 2) 965 328 0 (1382/ 757-1505/1031) 40.6 W13-W27 S18-S06
12 1729 930 (S19W42 L= 24) 813 172 1 (1706/ 841-1744/1020) 63.4 W39-W45 S24-S14
13 683 903 (N08E23 L=319) 532 175 0 ( 621/ 840- 744/ 968) -73.3 E25-E19 N03-N13
14 399 879 (N13E43 L=299) 264 70 1 ( 368/ 852- 420/ 897) -45.0 E45-E41 N11-N14
15 1287 744 (S16W07 L=349) 223 102 0 (1224/ 727-1316/ 767) -9.5 W03-W09 S17-S14
16 1192 623 (S21E01 L=341) 328 133 0 (1159/ 599-1248/ 663) -45.0 E03-W02 S22-S17
17 1434 597 (S30W13 L=355) 696 153 2 (1384/ 540-1484/ 649) 26.6 W09-W17 S32-S26
18 1128 294 (S42E18 L=324) 404 80 0 (1095/ 261-1161/ 334) 24.0 E22-E13 S44-S39
19 942 259 (S39E33 L=309) 647 131 0 ( 912/ 203- 966/ 324) 57.5 E38-E29 S43-S32
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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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