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| 20240219 - Filament data for 11 UTC |
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Available data for 20240219: »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
1 459 1699 (N25E61 L=235) 606 70 2 ( 435/1677- 488/1730) 26.6 E64-E57 N23-N27
2 1123 1633 (N33E08 L=288) 613 179 0 (1073/1558-1166/1702) -38.7 E13-E03 N28-N36
3 957 1633 (N29E18 L=277) 322 82 1 ( 927/1594- 997/1660) 80.5 E20-E16 N25-N31
4 533 1561 (N16E44 L=251) 940 172 2 ( 502/1510- 584/1644) -36.0 E50-E38 N13-N21
5 1545 1587 (N41W25 L=321) 943 175 1 (1461/1547-1615/1610) 4.1 W17-W31 N38-N43
6 298 1559 (N14E69 L=227) 1761 109 6 ( 257/1510- 340/1604) -71.6 E75-E64 N10-N16
7 1780 1468 (N40W51 L=347) 545 69 1 (1744/1445-1815/1487) 5.7 W46-W56 N39-N42
8 1174 1287 (N11W03 L=299) 634 210 1 (1141/1199-1220/1380) 90.0 W01-W05 N05-N17
9 1338 1261 (N13W13 L=309) 376 129 1 (1318/1211-1357/1325) -66.8 W12-W15 N10-N17
10 1531 1113 (N09W28 L=324) 570 189 0 (1476/1046-1571/1192) 73.3 W25-W30 N04-N14
11 1217 1085 (N00W10 L=305) 528 198 1 (1136/1043-1297/1138) -5.2 W04-W15 N00-N01
12 1921 1052 (N17W67 L= 2) 604 73 1 (1895/1026-1957/1070) 22.6 W62-W75 N14-N19
13 1867 996 (N12W60 L=355) 534 88 2 (1849/ 948-1884/1039) -59.0 W57-W61 N08-N14
14 1118 920 (S11W08 L=303) 500 300 1 ( 993/ 864-1238/ 947) 31.6 W01-W14 S16-S08
15 1921 905 (N09W70 L= 6) 945 99 2 (1887/ 863-1946/ 943) 41.2 W65-W75 N05-N12
16 673 888 (S21E19 L=277) 399 138 0 ( 617/ 855- 719/ 934) 45.0 E22-E15 S24-S17
17 1230 717 (S20W19 L=315) 559 178 1 (1176/ 649-1287/ 787) 78.7 W17-W21 S24-S14
18 1444 636 (S19W36 L=331) 439 192 0 (1366/ 576-1508/ 673) 56.3 W32-W39 S24-S15
19 1248 406 (S38W34 L=329) 388 92 1 (1208/ 388-1295/ 436) 15.9 W30-W37 S39-S36
20 1571 382 (S30W62 L=357) 625 135 0 (1508/ 352-1621/ 421) 45.0 W56-W64 S32-S26
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Download FITS filament maps as tar archive
» All Filament Data of 20240219 ...
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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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