|
|
|
|
| 20251229 - Filament data for 10 UTC |
|---|
|
Available data for 20251229: »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
1 804 1693 (N41E15 L=318) 283 50 2 ( 771/1675- 835/1710) 11.3 E17-E12 N40-N42
2 957 1687 (N40E03 L=330) 309 78 1 ( 913/1672- 995/1700) 9.5 E06-W00 N39-N41
3 1278 1589 (N32W20 L=353) 2023 517 4 (1032/1529-1508/1691) -17.9 W02-W36 N27-N40
4 395 1493 (N29E46 L=287) 469 70 3 ( 355/1472- 435/1520) 0.0 E49-E41 N27-N30
5 404 1427 (N24E43 L=290) 405 26 0 ( 383/1401- 427/1449) 45.0 E44-E40 N22-N25
6 1558 1227 (N09W34 L= 7) 1061 163 3 (1495/1171-1620/1284) 36.9 W29-W38 N05-N11
7 397 1252 (N13E41 L=292) 266 77 0 ( 366/1233- 429/1267) 11.3 E43-E38 N12-N13
8 396 1093 (N03E40 L=293) 507 102 1 ( 354/1058- 430/1132) 38.7 E43-E37 N01-N05
9 150 1107 (N06E64 L=269) 427 57 1 ( 121/1084- 188/1126) 6.3 E68-E59 N04-N06
10 1869 940 (S08W61 L= 34) 786 89 1 (1843/ 892-1893/ 977) -59.0 W57-W64 S11-S06
11 1857 825 (S15W61 L= 34) 2317 427 8 (1734/ 725-1956/ 960) 30.3 W50-W75 S21-S06
12 1600 897 (S11W37 L= 10) 514 164 1 (1531/ 858-1679/ 922) 20.0 W31-W42 S13-S09
13 397 819 (S13E42 L=291) 598 133 2 ( 361/ 776- 441/ 882) -60.3 E44-E39 S15-S08
14 267 703 (S19E57 L=276) 1003 146 7 ( 219/ 647- 307/ 780) -71.6 E60-E52 S22-S13
15 202 677 (S20E66 L=267) 1437 134 3 ( 167/ 620- 241/ 727) 81.9 E71-E61 S23-S16
16 386 707 (S19E45 L=288) 249 33 1 ( 365/ 686- 403/ 724) -45.0 E46-E43 S20-S18
17 431 674 (S22E42 L=291) 305 77 0 ( 410/ 630- 449/ 707) 39.8 E45-E39 S24-S19
18 1288 667 (S25W16 L=349) 330 98 0 (1237/ 655-1340/ 685) 0.0 W12-W19 S25-S23
19 495 653 (S23E38 L=295) 277 56 2 ( 474/ 619- 510/ 684) 53.1 E39-E35 S25-S21
|
|
Data will be available after one hour of observations. |
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.
|
|
|
|
