|
|
|
|
| 20240609 - Filament data for 11 UTC |
|
Available data for 20240609: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 384 1600 (N27E65 L=205) 1518 99 5 ( 344/1558- 424/1648) -60.3 E71-E59 N23-N30
2 747 1552 (N30E29 L=242) 1255 231 1 ( 705/1453- 815/1643) 90.0 E31-E26 N22-N37
3 1667 1527 (N43W49 L=320) 839 114 0 (1621/1483-1692/1557) -15.9 W44-W53 N39-N45
4 427 1394 (N15E47 L=223) 438 125 0 ( 413/1342- 446/1458) -60.3 E49-E44 N11-N18
5 1047 1365 (N22E03 L=267) 523 223 0 (1001/1267-1072/1430) -55.0 E07-W00 N15-N25
6 180 1090 (S07E65 L=205) 789 173 1 ( 154/1036- 203/1130) 56.3 E69-E61 S10-S04
7 1785 1099 (N15W54 L=324) 353 57 0 (1759/1076-1808/1116) -11.3 W51-W56 N14-N16
8 235 1050 (S09E58 L=213) 1160 127 4 ( 197/ 998- 258/1105) 81.9 E62-E55 S12-S05
9 328 1005 (S10E47 L=223) 414 60 0 ( 299/ 984- 353/1029) 0.0 E50-E45 S11-S08
10 366 965 (S12E44 L=227) 433 123 1 ( 322/ 934- 398/1023) 45.0 E47-E41 S14-S08
11 255 943 (S15E55 L=215) 470 63 0 ( 231/ 911- 280/ 971) -21.8 E57-E51 S16-S13
12 203 749 (S29E66 L=205) 1315 103 2 ( 157/ 714- 249/ 778) 12.3 E80-E57 S31-S26
13 1018 640 (S23W05 L=275) 320 58 0 ( 997/ 612-1044/ 680) -36.9 W03-W07 S25-S20
14 1793 615 (S14W69 L=339) 1545 85 0 (1762/ 570-1828/ 653) -63.4 W63-W75 S17-S11
15 921 584 (S29E00 L=270) 217 73 0 ( 883/ 572- 958/ 598) 0.0 E02-W02 S29-S27
16 1320 479 (S30W30 L=301) 1526 377 1 (1154/ 440-1494/ 527) 23.5 W19-W42 S35-S24
17 1187 249 (S50W34 L=304) 481 69 1 (1145/ 235-1224/ 269) 14.0 W29-W37 S51-S48
18 1378 230 (S48W57 L=328) 730 52 1 (1350/ 206-1403/ 260) -8.1 W50-W65 S50-S45
|
Download FITS filament maps as tar archive
» All Filament Data of 20240609 ...
|
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.
|
|
|
|