|
|
|
|
| 20241225 - Latest Filament data |
|
Available data for 20241225: »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 1096 1549 (N30W08 L=170) 735 181 0 (1022/1484-1165/1600) -45.0 W03-W11 N25-N33
2 478 1483 (N29E37 L=125) 849 152 3 ( 422/1443- 552/1537) -28.3 E42-E29 N26-N33
3 271 1299 (N19E52 L=109) 3530 371 9 ( 180/1164- 348/1438) 76.8 E61-E44 N11-N28
4 1595 1327 (N13W39 L=201) 301 107 0 (1546/1311-1645/1354) -23.2 W35-W42 N12-N15
5 1494 1209 (N07W30 L=192) 255 80 0 (1453/1196-1534/1223) -11.3 W27-W32 N05-N07
6 1276 1099 (N01W15 L=177) 718 327 2 (1147/1048-1411/1131) -3.6 W07-W23 S02-N03
7 1269 982 (S06W14 L=176) 176 58 0 (1239/ 965-1296/1004) -26.6 W12-W16 S06-S04
8 1836 970 (S08W57 L=218) 314 55 0 (1823/ 933-1847/ 997) 63.4 W55-W58 S10-S06
9 694 901 (S08E21 L=141) 208 132 0 ( 629/ 877- 741/ 932) -29.7 E24-E17 S09-S05
10 460 849 (S09E37 L=125) 940 291 0 ( 408/ 721- 523/ 931) 42.5 E43-E31 S16-S04
11 1226 873 (S12W11 L=173) 458 101 1 (1184/ 841-1286/ 903) 0.0 W08-W15 S13-S10
12 1046 828 (S14W00 L=162) 1454 394 4 ( 909/ 759-1165/ 902) -19.7 E07-W07 S18-S10
13 200 788 (S11E62 L=100) 1745 233 4 ( 102/ 745- 273/ 840) 6.1 E80-E52 S13-S08
14 521 775 (S14E34 L=128) 220 89 0 ( 493/ 729- 541/ 807) 38.7 E36-E31 S16-S12
15 1096 644 (S26W03 L=164) 227 64 1 (1068/ 615-1124/ 678) 36.9 W00-W04 S27-S23
16 1471 525 (S35W31 L=192) 298 86 0 (1433/ 499-1503/ 560) 45.0 W27-W33 S37-S33
17 398 502 (S30E53 L=109) 551 52 1 ( 369/ 485- 432/ 527) -21.8 E56-E49 S31-S28
18 346 440 (S34E64 L= 98) 1103 137 3 ( 325/ 370- 374/ 507) 26.6 E75-E57 S38-S29
19 1668 469 (S40W53 L=215) 1066 113 1 (1602/ 443-1726/ 493) 0.0 W45-W62 S42-S38
|
Download FITS filament maps as tar archive
» All Filament Data of 20241225 ...
|
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.
|
|
|
|