|
|
|
|
| 20251007 - Filament data for 11 UTC |
|
Available data for 20251007: »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
1 982 1889 (N62W47 L= 33) 430 83 0 ( 948/1855-1018/1915) 3.4 W37-W55 N60-N62
2 597 1685 (N61E13 L=333) 902 188 2 ( 507/1647- 683/1719) -2.4 E26-E01 N58-N62
3 1664 1584 (N17W63 L= 50) 3198 302 9 (1537/1530-1783/1633) -31.8 W54-W77 N10-N23
4 1162 1544 (N31W25 L= 12) 426 122 0 (1101/1516-1217/1584) 0.0 W20-W30 N30-N32
5 1605 1520 (N16W53 L= 40) 345 45 1 (1569/1509-1637/1536) -9.5 W50-W56 N14-N17
6 1758 1434 (N06W62 L= 48) 2311 274 6 (1696/1340-1820/1517) 65.6 W57-W69 N00-N11
7 689 1450 (N40E10 L=337) 567 127 4 ( 622/1425- 754/1472) -21.8 E14-E04 N36-N41
8 1251 1445 (N23W26 L= 12) 304 93 0 (1202/1429-1304/1464) -15.9 W22-W29 N21-N24
9 292 1350 (N44E49 L=297) 978 146 2 ( 253/1307- 345/1415) -42.0 E56-E42 N39-N48
10 1241 1301 (N16W20 L= 6) 232 80 0 (1229/1258-1254/1345) 53.1 W18-W21 N13-N17
11 1835 1283 (S04W62 L= 49) 1461 119 3 (1778/1244-1882/1324) 0.0 W54-W70 S05-N00
12 824 1224 (N22E06 L=340) 560 229 0 ( 770/1149- 896/1255) 20.6 E10-E02 N18-N24
13 1677 1155 (S05W43 L= 29) 645 146 0 (1653/1082-1715/1220) 36.9 W39-W47 S08-S02
14 875 1107 (N15E06 L=340) 324 99 1 ( 850/1055- 899/1155) 38.7 E08-E03 N12-N16
15 1130 615 (S19E05 L=342) 665 211 0 (1072/ 517-1170/ 703) 36.0 E11-W00 S24-S14
16 583 579 (S08E38 L=308) 896 189 0 ( 557/ 497- 610/ 686) 45.0 E43-E33 S12-S02
17 1702 538 (S45W37 L= 23) 1462 187 2 (1616/ 484-1783/ 594) 0.0 W26-W48 S46-S41
18 765 246 (S34E46 L=301) 2171 297 3 ( 639/ 166- 868/ 326) 10.7 E69-E32 S38-S30
|
Download FITS filament maps as tar archive
» All Filament Data of 20251007 ...
|
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.
|
|
|
|