|
|
|
|
| 20250830 - Filament data for 07 UTC |
|
Available data for 20250830: »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 1645 1654 (N27W70 L=200) 567 68 1 (1616/1634-1680/1670) -38.7 W66-W74 N24-N28
2 864 1564 (N43W02 L=133) 230 40 2 ( 837/1540- 889/1583) -14.0 W00-W04 N41-N44
3 1051 1538 (N37W15 L=145) 277 69 1 (1021/1513-1089/1562) 0.0 W12-W18 N35-N38
4 817 1480 (N39E03 L=127) 588 170 0 ( 798/1419- 858/1558) 78.7 E05-W00 N34-N44
5 1518 1372 (N15W40 L=170) 306 86 1 (1494/1331-1537/1405) 78.7 W38-W41 N12-N17
6 827 1210 (N22E08 L=122) 987 334 0 ( 761/1085- 931/1338) -74.5 E11-E04 N12-N30
7 149 901 (N13E70 L= 60) 1061 114 2 ( 118/ 856- 176/ 931) -90.0 E76-E65 N10-N15
8 1050 897 (S01E01 L=129) 211 40 2 (1018/ 877-1076/ 917) 0.0 E02-W00 S01-N00
9 921 839 (S01E10 L=120) 239 86 1 ( 873/ 820- 961/ 860) 0.0 E12-E07 S02-N00
10 1636 740 (S24W34 L=164) 1387 283 2 (1554/ 616-1700/ 848) 42.7 W26-W39 S30-S18
11 495 711 (S02E40 L= 91) 328 87 0 ( 484/ 668- 508/ 758) 59.0 E41-E37 S04-N01
12 1162 663 (S17W01 L=131) 559 74 3 (1127/ 626-1199/ 692) 26.6 E01-W03 S19-S14
13 841 562 (S17E21 L=109) 239 123 0 ( 824/ 513- 869/ 609) 74.1 E22-E18 S20-S13
14 906 519 (S21E19 L=112) 376 70 0 ( 883/ 487- 924/ 557) 63.4 E20-E16 S22-S18
15 1045 507 (S24E10 L=120) 289 111 0 (1008/ 468-1070/ 553) 45.0 E13-E07 S26-S21
16 716 514 (S17E31 L=100) 254 83 1 ( 680/ 492- 761/ 534) -36.9 E32-E28 S19-S15
17 943 311 (S36E25 L=106) 5051 817 13 ( 669/ 167-1230/ 507) 13.0 E65-W01 S44-S28
18 384 428 (S18E64 L= 67) 632 83 0 ( 344/ 406- 419/ 453) 12.1 E71-E57 S19-S16
19 1581 359 (S54W32 L=163) 704 64 1 (1556/ 340-1613/ 387) -32.5 W27-W38 S56-S49
|
Download FITS filament maps as tar archive
» All Filament Data of 20250830 ...
|
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.
|
|
|
|