|
|
|
|
| 20250831 - Filament data for 08 UTC |
|
Available data for 20250831: »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 972 1518 (N38W09 L=126) 1345 323 1 ( 937/1363-1015/1644) 48.6 W02-W17 N28-N45
2 1195 1608 (N38W29 L=145) 368 57 0 (1171/1579-1227/1626) 0.0 W26-W31 N35-N38
3 1420 1584 (N30W43 L=160) 675 127 1 (1372/1559-1488/1606) -5.2 W38-W49 N28-N31
4 1034 1289 (N22W06 L=123) 685 114 2 ( 984/1243-1088/1339) -56.3 W03-W08 N18-N25
5 160 1128 (N27E68 L= 49) 1956 187 3 ( 127/1048- 194/1188) 48.8 E75-E62 N22-N31
6 865 992 (N08E10 L=107) 451 198 3 ( 781/ 956- 946/1017) -5.7 E15-E05 N07-N09
7 263 908 (N13E55 L= 62) 680 196 2 ( 221/ 828- 290/ 964) 53.1 E59-E51 N08-N16
8 1783 817 (S24W48 L=164) 2295 327 2 (1696/ 676-1843/ 960) 41.2 W38-W55 S30-S16
9 214 857 (N11E62 L= 55) 411 92 0 ( 196/ 817- 240/ 901) -59.0 E63-E59 N08-N13
10 1357 819 (S12W15 L=132) 361 120 2 (1321/ 785-1395/ 877) 26.6 W12-W18 S13-S09
11 683 777 (S01E25 L= 91) 325 121 0 ( 670/ 720- 694/ 840) 63.4 E26-E23 S03-N03
12 1420 723 (S19W17 L=134) 1155 412 4 (1306/ 649-1567/ 763) -3.2 W09-W28 S23-S14
13 873 676 (S10E16 L=100) 221 85 0 ( 861/ 644- 891/ 727) 80.5 E17-E15 S12-S06
14 1040 628 (S16E08 L=109) 330 156 0 (1018/ 574-1077/ 688) 82.9 E09-E04 S20-S12
15 1219 665 (S18W04 L=120) 323 56 0 (1182/ 642-1250/ 684) -36.9 W01-W05 S19-S16
16 487 449 (S18E51 L= 66) 1338 231 0 ( 383/ 407- 559/ 516) 8.1 E62-E41 S20-S14
17 1068 333 (S38E15 L=102) 4387 695 4 ( 796/ 207-1310/ 467) 9.7 E42-W05 S42-S33
18 1564 352 (S54W30 L=146) 456 51 0 (1537/ 333-1599/ 370) 0.0 W25-W34 S54-S52
|
Download FITS filament maps as tar archive
» All Filament Data of 20250831 ...
|
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.
|
|
|
|