|
|
|
|
| 20260526 - Filament data for 06 UTC |
|
Available data for 20260526: »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
1 474 1620 (N24E55 L=128) 448 66 2 ( 442/1601- 509/1646) -7.1 E59-E51 N22-N25
2 1337 1584 (N40W09 L=193) 341 47 0 (1309/1567-1363/1603) 0.0 W07-W11 N39-N42
3 1367 1528 (N37W13 L=196) 352 55 2 (1333/1509-1401/1548) 21.8 W10-W15 N35-N38
4 550 1380 (N10E37 L=146) 547 166 0 ( 528/1310- 571/1457) -60.9 E41-E34 N05-N14
5 353 1341 (N04E51 L=132) 787 109 1 ( 332/1285- 370/1389) -45.0 E55-E48 N01-N07
6 1696 1306 (N30W42 L=225) 325 83 0 (1675/1259-1709/1341) -68.2 W39-W43 N26-N31
7 746 1278 (N08E22 L=162) 203 70 1 ( 716/1248- 784/1303) -11.3 E23-E18 N06-N09
8 288 1047 (S14E50 L=133) 988 244 1 ( 254/ 951- 330/1122) 74.7 E53-E47 S19-S08
9 1716 1057 (N14W45 L=228) 307 90 0 (1699/1000-1728/1090) -68.2 W43-W46 N11-N16
10 297 916 (S22E48 L=135) 779 231 3 ( 229/ 869- 353/ 975) 33.7 E55-E43 S25-S17
11 1277 941 (S01W16 L=200) 275 49 1 (1249/ 923-1306/ 958) 33.7 W14-W17 S02-N00
12 1345 831 (S06W23 L=206) 474 84 2 (1308/ 785-1371/ 864) 90.0 W20-W24 S08-S03
13 1442 755 (S09W31 L=214) 349 132 0 (1384/ 721-1496/ 793) 50.2 W28-W33 S11-S05
14 1566 624 (S14W44 L=227) 458 125 1 (1524/ 593-1605/ 645) 26.6 W41-W48 S16-S12
15 635 468 (S45E17 L=167) 269 61 0 ( 606/ 445- 660/ 494) -11.3 E19-E14 S46-S43
16 810 434 (S43E01 L=182) 769 124 1 ( 736/ 417- 881/ 455) 15.3 E07-W04 S45-S40
17 1491 374 (S31W53 L=236) 4897 416 15 (1302/ 305-1650/ 449) 2.7 W33-W75 S34-S25
18 1081 419 (S37W19 L=202) 279 66 0 (1050/ 395-1118/ 447) -9.5 W16-W22 S38-S35
|
Download FITS filament maps as tar archive
» All Filament Data of 20260526 ...
|
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.
|
|
|
|