|
|
|
|
| 20230304 - Latest Filament data |
|
Available data for 20230304: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1031 1801 (N42E25 L=236) 350 61 0 (1008/1775-1064/1823) 90.0 E26-E23 N39-N45
2 689 1762 (N30E46 L=214) 1579 183 5 ( 620/1706- 757/1817) 73.3 E50-E42 N25-N36
3 837 1687 (N28E31 L=230) 1409 292 1 ( 754/1649- 946/1756) 22.6 E37-E23 N24-N32
4 423 1572 (N12E55 L=205) 617 146 0 ( 387/1548- 481/1610) 5.7 E59-E49 N10-N14
5 1547 1447 (N32W23 L=284) 1651 424 0 (1422/1300-1697/1602) -25.6 W11-W37 N26-N39
6 500 1527 (N11E47 L=214) 451 88 0 ( 467/1502- 532/1548) 53.1 E49-E43 N08-N12
7 1650 1466 (N37W32 L=293) 376 97 0 (1606/1431-1686/1500) -7.1 W27-W35 N35-N38
8 583 1408 (N05E36 L=225) 913 105 2 ( 557/1350- 611/1454) 90.0 E38-E33 N01-N08
9 1808 1328 (N33W49 L=310) 516 48 0 (1777/1309-1834/1347) 0.0 W45-W53 N32-N35
10 566 1147 (S10E30 L=231) 901 256 3 ( 475/1071- 671/1221) 50.2 E34-E24 S16-S04
11 1218 1150 (N04W08 L=268) 401 89 0 (1172/1125-1261/1179) 45.0 W05-W09 N02-N07
12 163 1000 (S25E66 L=195) 1965 170 4 ( 131/ 921- 189/1084) 78.7 E71-E61 S30-S20
13 343 917 (S28E44 L=217) 739 213 3 ( 255/ 865- 419/ 972) 26.6 E53-E37 S31-S23
14 1202 873 (S11W14 L=274) 415 147 0 (1114/ 850-1259/ 892) 18.4 W08-W17 S13-S09
15 561 779 (S32E24 L=237) 2435 523 4 ( 366/ 650- 787/ 866) 30.5 E42-E08 S44-S24
16 1601 501 (S20W55 L=316) 858 189 0 (1523/ 456-1681/ 559) 55.0 W51-W59 S24-S14
17 1311 520 (S28W33 L=294) 547 182 0 (1230/ 502-1395/ 544) 14.0 W26-W38 S29-S25
18 1489 353 (S31W58 L=319) 2534 287 4 (1352/ 325-1618/ 390) 23.5 W46-W69 S36-S25
|
Download FITS filament maps as tar archive
» All Filament Data of 20230304 ...
|
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.
|
|
|
|