|
|
|
|
| 20230920 - Filament data for 08 UTC |
|
Available data for 20230920: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 524 1732 (N71E34 L=107) 738 54 2 ( 495/1701- 550/1757) -26.6 E46-E26 N66-N75
2 1084 1638 (N41W25 L=166) 293 58 1 (1051/1618-1109/1660) 0.0 W22-W28 N39-N42
3 1475 1553 (N24W47 L=187) 588 168 1 (1439/1500-1524/1614) 69.4 W44-W50 N19-N27
4 1653 1481 (N14W56 L=197) 1091 129 5 (1617/1420-1693/1533) 66.8 W52-W61 N09-N16
5 1567 1489 (N17W50 L=190) 355 113 1 (1538/1459-1603/1532) 26.6 W46-W53 N15-N18
6 1258 1363 (N20W23 L=164) 679 309 0 (1100/1314-1365/1401) -37.6 W14-W28 N14-N25
7 233 1278 (N40E59 L= 82) 583 67 1 ( 204/1250- 264/1304) -20.0 E65-E54 N37-N42
8 701 1261 (N29E14 L=127) 276 116 0 ( 667/1234- 747/1304) -56.3 E15-E11 N26-N32
9 1883 1160 (S11W66 L=206) 934 83 3 (1855/1115-1912/1209) -90.0 W63-W70 S13-S07
10 582 1178 (N26E24 L=117) 340 78 1 ( 549/1153- 627/1208) -31.0 E26-E20 N24-N28
11 217 958 (N20E60 L= 81) 847 101 1 ( 173/ 921- 247/ 999) 24.0 E66-E56 N18-N22
12 358 866 (N13E47 L= 94) 697 119 3 ( 304/ 835- 424/ 897) -21.8 E51-E41 N10-N15
13 570 808 (N05E32 L=108) 316 113 0 ( 555/ 758- 603/ 855) 45.0 E34-E29 N02-N07
14 852 803 (S01E15 L=125) 273 48 0 ( 822/ 781- 879/ 824) -45.0 E16-E13 S02-N00
15 688 585 (S10E32 L=109) 307 83 2 ( 658/ 552- 724/ 611) 18.4 E34-E28 S11-S09
16 535 534 (S10E44 L= 96) 339 40 0 ( 515/ 510- 553/ 561) -90.0 E45-E42 S11-S08
17 1340 492 (S34W05 L=146) 621 81 2 (1306/ 460-1375/ 524) -36.9 W02-W07 S36-S30
18 375 461 (S12E64 L= 77) 1763 193 6 ( 315/ 388- 422/ 518) -78.7 E69-E58 S18-S08
|
Download FITS filament maps as tar archive
» All Filament Data of 20230920 ...
|
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.
|
|
|
|