|
|
|
|
| 20230921 - Filament data for 09 UTC |
|
Available data for 20230921: »06 UTC »07 UTC »08 UTC »09 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
1 570 1746 (N71E22 L=105) 1717 139 3 ( 496/1687- 629/1797) 4.6 E36-E10 N65-N76
2 1230 1629 (N36W35 L=162) 584 219 1 (1130/1598-1327/1668) -48.0 W29-W39 N30-N40
3 1578 1605 (N23W59 L=186) 728 140 2 (1537/1546-1612/1663) 63.4 W55-W61 N18-N26
4 1414 1453 (N20W37 L=164) 644 267 2 (1298/1399-1524/1484) -47.5 W30-W42 N13-N25
5 871 1349 (N29E00 L=127) 389 170 1 ( 816/1308- 951/1398) -60.9 E02-W03 N24-N33
6 331 1297 (N40E46 L= 81) 582 109 3 ( 295/1253- 356/1333) -50.2 E50-E42 N36-N42
7 779 1250 (N26E09 L=118) 655 231 0 ( 704/1216- 886/1314) -45.0 E12-E02 N21-N31
8 712 1024 (N15E18 L=109) 197 99 0 ( 688/ 974- 734/1065) 45.0 E20-E16 N12-N16
9 508 934 (N14E34 L= 93) 589 141 2 ( 445/ 913- 573/ 971) -26.6 E37-E29 N11-N17
10 346 906 (N15E47 L= 80) 340 86 1 ( 318/ 874- 370/ 943) 53.1 E50-E44 N13-N17
11 749 894 (N06E19 L=108) 272 83 1 ( 723/ 847- 774/ 922) 78.7 E20-E17 N03-N08
12 1291 800 (S12W09 L=137) 482 190 0 (1265/ 716-1331/ 886) 52.1 W06-W13 S17-S08
13 263 752 (N07E60 L= 67) 795 86 2 ( 230/ 726- 304/ 790) -20.6 E63-E55 N05-N09
14 878 655 (S10E18 L=109) 235 74 1 ( 842/ 622- 911/ 685) 36.9 E20-E15 S11-S08
15 1569 613 (S33W25 L=152) 422 59 1 (1540/ 576-1586/ 645) 76.0 W22-W26 S35-S30
16 710 590 (S10E30 L= 97) 290 91 0 ( 694/ 539- 724/ 629) 71.6 E31-E28 S13-S07
17 513 513 (S11E47 L= 80) 291 61 1 ( 491/ 486- 533/ 544) -90.0 E48-E45 S12-S08
18 480 450 (S14E53 L= 74) 868 162 2 ( 416/ 415- 551/ 475) -26.6 E60-E48 S17-S12
19 515 367 (S21E57 L= 71) 386 70 0 ( 481/ 348- 550/ 389) 11.3 E61-E51 S21-S19
|
Download FITS filament maps as tar archive
» All Filament Data of 20230921 ...
|
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.
|
|
|
|