|
|
|
|
| 20230921 - Filament data for 11 UTC |
|
Available data for 20230921: »06 UTC »07 UTC »08 UTC »09 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 594 1756 (N71E17 L=108) 1236 128 2 ( 549/1709- 640/1797) 28.3 E27-E07 N66-N75
2 1204 1716 (N42W40 L=165) 377 54 1 (1181/1695-1229/1736) 0.0 W36-W42 N39-N43
3 1590 1611 (N22W60 L=186) 546 122 0 (1548/1561-1619/1654) 74.1 W57-W63 N19-N26
4 1281 1621 (N34W38 L=163) 332 123 0 (1219/1605-1337/1643) -39.8 W34-W40 N30-N36
5 1427 1463 (N20W38 L=164) 552 263 0 (1318/1412-1534/1494) -42.3 W32-W43 N14-N25
6 347 1301 (N39E44 L= 82) 443 83 2 ( 319/1261- 372/1334) -45.0 E47-E41 N36-N42
7 807 1253 (N25E07 L=119) 608 197 1 ( 730/1222- 906/1298) -38.7 E11-E01 N21-N30
8 729 1020 (N14E17 L=108) 214 106 0 ( 702/ 982- 758/1063) 31.0 E19-E14 N12-N15
9 530 941 (N14E32 L= 94) 639 147 1 ( 464/ 921- 601/ 968) -24.0 E36-E26 N11-N16
10 364 909 (N15E46 L= 80) 315 88 1 ( 338/ 878- 387/ 946) 53.1 E48-E43 N13-N17
11 768 908 (N07E17 L=108) 293 101 3 ( 740/ 858- 798/ 941) -90.0 E18-E15 N03-N09
12 208 897 (N17E62 L= 64) 530 58 1 ( 185/ 864- 231/ 929) -63.4 E65-E59 N14-N18
13 1301 782 (S14W10 L=135) 281 74 0 (1284/ 742-1314/ 822) 78.7 W08-W10 S16-S11
14 280 755 (N07E58 L= 68) 818 122 1 ( 229/ 729- 338/ 783) -16.7 E62-E52 N05-N09
15 724 608 (S10E29 L= 97) 257 104 0 ( 699/ 561- 737/ 654) 80.5 E29-E27 S12-S06
16 1586 620 (S33W26 L=152) 425 76 1 (1558/ 581-1604/ 652) 76.0 W23-W27 S36-S30
17 524 522 (S11E46 L= 80) 438 68 1 ( 502/ 490- 550/ 559) 63.4 E47-E44 S12-S08
18 528 450 (S15E49 L= 76) 552 83 2 ( 496/ 410- 555/ 489) 71.6 E51-E46 S18-S12
19 508 365 (S21E57 L= 68) 640 112 0 ( 454/ 348- 568/ 391) 3.8 E65-E50 S21-S19
|
Download FITS filament maps as tar archive
» All Filament Data of 20230921 ...
|
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.
|
|
|
|