|
|
|
|
| 20231013 - Filament data for 06 UTC |
|
Available data for 20231013: »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 1524 1687 (N27W61 L=259) 741 77 3 (1489/1658-1557/1718) 68.2 W56-W64 N24-N29
2 1286 1617 (N31W38 L=236) 1691 379 1 (1146/1569-1457/1672) -43.2 W29-W47 N24-N39
3 975 1593 (N40W16 L=214) 447 102 0 ( 924/1569-1020/1614) -7.1 W11-W19 N38-N41
4 1459 1445 (N17W39 L=238) 821 296 2 (1296/1425-1562/1479) -21.3 W28-W46 N12-N20
5 1636 1373 (N07W48 L=247) 515 71 0 (1609/1344-1662/1409) -78.7 W46-W50 N04-N09
6 1054 1330 (N22W10 L=209) 650 181 1 ( 970/1305-1134/1367) -15.3 W05-W16 N20-N24
7 1529 1296 (N07W38 L=236) 275 68 0 (1494/1276-1563/1317) -45.0 W35-W39 N04-N08
8 1108 1240 (N16W11 L=209) 311 165 0 (1041/1213-1182/1258) -14.0 W06-W14 N13-N16
9 505 993 (N17E32 L=166) 737 286 1 ( 399/ 959- 645/1017) -22.4 E40-E23 N11-N19
10 344 940 (N17E46 L=152) 279 22 0 ( 325/ 915- 361/ 959) 63.4 E47-E44 N16-N18
11 1748 906 (S22W43 L=242) 339 75 0 (1708/ 891-1786/ 920) -20.6 W39-W47 S23-S20
12 327 777 (N08E52 L=146) 961 164 3 ( 297/ 724- 376/ 842) -66.8 E55-E48 N05-N12
13 1460 786 (S20W19 L=217) 292 97 0 (1435/ 743-1485/ 825) 38.7 W16-W21 S21-S17
14 1357 696 (S22W10 L=209) 248 95 0 (1339/ 653-1376/ 745) 45.0 W08-W12 S23-S18
15 1104 640 (S18E06 L=192) 383 127 3 (1065/ 594-1138/ 703) 74.1 E08-E04 S20-S13
16 1553 417 (S50W21 L=219) 419 84 0 (1516/ 391-1579/ 450) 8.1 W16-W23 S51-S47
17 1356 304 (S51E01 L=197) 1074 184 0 (1291/ 268-1437/ 345) -8.1 E07-W07 S53-S48
18 481 307 (S24E68 L=130) 621 36 1 ( 461/ 285- 502/ 331) 38.7 E72-E63 S25-S21
|
Download FITS filament maps as tar archive
» All Filament Data of 20231013 ...
|
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.
|
|
|
|