|
|
|
|
| 20260408 - Filament data for 07 UTC |
|
Available data for 20260408: »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
1 949 1817 (N40E36 L= 61) 650 120 0 ( 898/1800-1012/1842) 10.3 E41-E30 N38-N41
2 634 1564 (N14E40 L= 57) 629 272 0 ( 568/1490- 728/1660) -17.5 E49-E30 N10-N18
3 731 1366 (N05E26 L= 71) 372 76 0 ( 699/1343- 775/1384) 36.9 E27-E23 N03-N06
4 295 1291 (S09E55 L= 42) 870 112 1 ( 253/1251- 340/1324) 39.8 E58-E50 S12-S07
5 1687 1278 (N29W34 L=132) 440 69 1 (1652/1253-1716/1302) 9.5 W31-W37 N26-N30
6 1705 1198 (N24W37 L=134) 738 95 1 (1678/1144-1721/1247) -80.5 W34-W39 N21-N27
7 451 1067 (S19E36 L= 61) 2115 599 1 ( 258/1007- 706/1226) 0.0 E56-E18 S22-S13
8 1661 1049 (N14W37 L=134) 313 50 1 (1634/1028-1694/1068) 36.9 W34-W39 N12-N15
9 1563 824 (S01W37 L=134) 867 193 1 (1535/ 730-1583/ 920) -52.1 W33-W40 S05-N04
10 1793 795 (N06W56 L=153) 469 67 1 (1769/ 766-1811/ 834) -45.0 W53-W58 N03-N07
11 1843 791 (N07W62 L=159) 778 80 1 (1820/ 749-1866/ 821) -63.4 W58-W65 N05-N09
12 1195 783 (S14W16 L=114) 436 174 0 (1115/ 767-1267/ 804) 32.0 W11-W20 S15-S10
13 417 717 (S40E33 L= 64) 332 51 0 ( 396/ 688- 439/ 746) -56.3 E35-E31 S42-S38
14 1727 594 (S07W60 L=157) 673 102 0 (1681/ 565-1766/ 632) 56.3 W56-W63 S09-S03
15 525 441 (S57E20 L= 77) 958 138 1 ( 454/ 416- 590/ 467) 10.0 E29-E12 S60-S54
16 697 425 (S52E02 L= 95) 419 48 1 ( 664/ 405- 725/ 457) 36.9 E04-W01 S53-S49
17 1395 379 (S29W48 L=146) 528 78 2 (1356/ 360-1434/ 404) 26.6 W44-W52 S30-S27
18 1264 365 (S35W41 L=138) 293 51 1 (1233/ 344-1295/ 391) 0.0 W37-W44 S35-S33
|
Download FITS filament maps as tar archive
» All Filament Data of 20260408 ...
|
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.
|
|
|
|