|
|
|
|
| 20250411 - Filament data for 13 UTC |
|
Available data for 20250411: »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
1 748 1864 (N38E56 L=136) 771 53 1 ( 719/1837- 786/1884) -6.3 E62-E51 N35-N39
2 685 1814 (N32E54 L=138) 614 52 2 ( 665/1781- 709/1846) -45.0 E58-E50 N29-N35
3 835 1609 (N22E29 L=163) 775 251 3 ( 790/1494- 896/1712) -38.7 E36-E21 N16-N28
4 419 1536 (N08E54 L=137) 2956 345 7 ( 345/1404- 530/1623) 75.1 E61-E49 N00-N15
5 1131 1527 (N26E09 L=183) 379 116 1 (1114/1466-1151/1582) -54.5 E10-E05 N22-N29
6 1225 1295 (N14W04 L=195) 323 123 0 (1187/1239-1239/1344) -45.0 W00-W05 N11-N16
7 763 1302 (N02E22 L=170) 200 67 1 ( 743/1270- 782/1336) -76.0 E22-E21 N00-N04
8 431 1063 (S19E37 L=154) 1645 323 4 ( 302/ 944- 530/1163) 50.5 E46-E31 S27-S10
9 137 1116 (S21E70 L=122) 655 103 3 ( 111/1078- 171/1156) 29.1 E75-E64 S23-S18
10 546 836 (S29E24 L=167) 2711 674 3 ( 254/ 724- 843/ 917) 29.9 E53-E06 S43-S16
11 1636 834 (N02W42 L=233) 270 68 0 (1623/ 803-1654/ 872) -45.0 W39-W43 N00-N03
12 1515 754 (S06W36 L=228) 295 94 0 (1493/ 706-1535/ 794) -38.7 W33-W38 S08-S04
13 1185 613 (S24W22 L=214) 374 124 1 (1124/ 595-1248/ 635) 50.2 W18-W25 S26-S20
14 1693 568 (S10W58 L=250) 415 69 1 (1678/ 524-1712/ 598) -45.0 W55-W61 S12-S08
15 1633 528 (S14W56 L=248) 706 90 1 (1604/ 482-1664/ 578) -71.6 W53-W58 S16-S10
16 574 468 (S53E16 L=176) 404 120 0 ( 543/ 428- 620/ 519) -24.0 E19-E10 S54-S49
17 1649 434 (S18W65 L=257) 527 68 0 (1627/ 398-1672/ 456) -63.4 W61-W67 S20-S16
18 1029 288 (S49W32 L=223) 1915 357 5 ( 870/ 219-1150/ 382) 0.0 W13-W47 S50-S45
|
Download FITS filament maps as tar archive
» All Filament Data of 20250411 ...
|
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.
|
|
|
|