|
|
|
|
| 20240830 - Filament data for 06 UTC |
|
Available data for 20240830: »06 UTC »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 1165 1573 (N36W25 L=294) 1450 360 3 ( 993/1519-1308/1600) -11.8 W11-W35 N32-N39
2 1494 1579 (N27W49 L=317) 814 170 0 (1413/1560-1575/1596) -22.6 W43-W56 N23-N29
3 1614 1507 (N19W54 L=323) 513 92 1 (1578/1469-1650/1538) -78.7 W51-W56 N16-N21
4 1350 1267 (N13W25 L=294) 715 269 0 (1235/1200-1454/1315) -45.0 W18-W30 N07-N18
5 997 1189 (N17W02 L=270) 397 93 2 ( 965/1142-1033/1226) 59.0 W00-W04 N14-N19
6 1841 1119 (S08W59 L=327) 635 109 3 (1819/1069-1874/1171) -69.4 W56-W62 S12-S04
7 478 1061 (N20E34 L=234) 380 101 0 ( 442/1025- 526/1094) -50.2 E36-E31 N16-N22
8 1865 860 (S25W59 L=327) 2761 424 11 (1777/ 728-1920/1030) 41.2 W47-W69 S31-S15
9 483 876 (N09E37 L=232) 308 116 1 ( 455/ 819- 515/ 922) -66.8 E38-E35 N04-N11
10 584 736 (S01E33 L=235) 993 317 1 ( 522/ 625- 705/ 806) 17.4 E40-E24 S06-N03
11 469 599 (S08E46 L=223) 1529 390 6 ( 363/ 470- 561/ 687) -66.4 E52-E41 S17-N00
12 410 565 (S09E52 L=216) 874 124 1 ( 372/ 521- 446/ 610) -90.0 E54-E49 S11-S05
13 279 523 (S11E71 L=197) 988 76 4 ( 247/ 491- 309/ 553) -45.0 E76-E66 S12-S08
14 478 475 (S16E51 L=217) 1608 209 5 ( 441/ 387- 521/ 544) 37.6 E60-E45 S21-S11
15 1395 402 (S42W11 L=279) 1139 239 2 (1316/ 333-1480/ 483) 25.0 W03-W18 S46-S37
16 851 424 (S26E26 L=242) 493 178 2 ( 783/ 397- 920/ 462) 0.0 E31-E21 S28-S23
17 548 408 (S21E49 L=219) 481 64 2 ( 517/ 370- 569/ 438) -90.0 E51-E45 S24-S19
18 819 268 (S37E38 L=231) 334 55 1 ( 791/ 251- 851/ 280) 0.0 E40-E34 S38-S35
|
Download FITS filament maps as tar archive
» All Filament Data of 20240830 ...
|
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.
|
|
|
|