|
|
|
|
| 20250731 - Filament data for 10 UTC |
|
Available data for 20250731: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1453 1729 (N45W54 L=219) 433 55 1 (1431/1697-1475/1747) 53.1 W50-W58 N42-N46
2 566 1683 (N55E39 L=126) 350 37 1 ( 544/1659- 580/1706) -68.2 E42-E36 N52-N57
3 1271 1527 (N34W25 L=190) 226 34 2 (1252/1505-1292/1548) -90.0 W23-W26 N32-N35
4 1757 1349 (N15W59 L=224) 385 79 0 (1730/1316-1779/1386) -68.2 W57-W60 N12-N17
5 448 1347 (N31E39 L=126) 984 231 1 ( 363/1319- 552/1370) -3.4 E47-E30 N28-N32
6 180 1039 (N12E64 L=101) 1720 250 4 ( 148/ 947- 220/1120) 74.7 E69-E59 N06-N17
7 747 986 (N06E17 L=148) 392 131 1 ( 714/ 928- 772/1050) -82.9 E18-E16 N02-N10
8 1814 865 (S15W55 L=221) 377 72 0 (1792/ 830-1835/ 899) 36.9 W53-W58 S16-S12
9 1297 833 (S09W15 L=180) 192 76 1 (1283/ 798-1312/ 873) 76.0 W13-W15 S10-S06
10 537 735 (S08E35 L=131) 251 77 1 ( 503/ 704- 567/ 760) 31.0 E37-E31 S09-S06
11 1692 626 (S28W45 L=211) 1222 241 4 (1613/ 561-1760/ 714) 28.3 W38-W51 S33-S23
12 1107 583 (S23W00 L=166) 856 160 3 (1052/ 516-1154/ 647) 66.0 E03-W04 S27-S18
13 571 593 (S17E35 L=130) 595 114 2 ( 537/ 544- 600/ 629) -80.5 E37-E33 S20-S14
14 1362 488 (S33W18 L=183) 1708 336 3 (1251/ 388-1428/ 625) 50.9 W09-W22 S39-S23
15 1170 420 (S35W03 L=168) 1254 220 4 (1102/ 358-1250/ 504) -53.1 W00-W09 S41-S28
16 665 445 (S28E33 L=132) 553 72 1 ( 631/ 424- 706/ 478) -31.0 E35-E29 S29-S25
17 495 391 (S31E51 L=114) 448 68 0 ( 466/ 366- 520/ 422) 18.4 E55-E46 S33-S28
18 1518 318 (S51W39 L=204) 649 72 1 (1481/ 304-1562/ 334) 0.0 W33-W45 S53-S49
19 1365 256 (S55W22 L=187) 1169 117 2 (1317/ 232-1423/ 284) -15.9 W16-W30 S57-S50
|
Download FITS filament maps as tar archive
» All Filament Data of 20250731 ...
|
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.
|
|
|
|