|
|
|
|
| 20251025 - Filament data for 09 UTC |
|
Available data for 20251025: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1387 1776 (N37W56 L=166) 786 123 2 (1317/1749-1445/1806) -13.0 W49-W63 N34-N38
2 1066 1614 (N37W22 L=132) 360 58 1 (1037/1585-1087/1644) 31.0 W19-W24 N35-N38
3 1045 1380 (N24W11 L=121) 317 75 1 (1008/1357-1087/1397) -36.9 W09-W13 N22-N25
4 1839 1337 (S01W65 L=175) 1276 106 3 (1791/1301-1892/1370) -18.4 W59-W73 S03-N01
5 1288 1153 (N05W18 L=128) 196 96 0 (1242/1128-1327/1179) 0.0 W14-W20 N04-N05
6 501 1130 (N23E29 L= 81) 1477 320 4 ( 336/1092- 639/1177) -24.4 E42-E20 N19-N29
7 1068 1129 (N10W05 L=115) 191 110 0 (1017/1118-1123/1141) -18.4 W02-W08 N08-N11
8 1504 867 (S16W24 L=134) 1467 437 3 (1348/ 731-1613/ 994) 22.8 W11-W31 S19-S09
9 781 902 (N04E16 L= 94) 460 177 0 ( 715/ 878- 836/ 946) -8.1 E19-E12 N02-N07
10 153 856 (N14E68 L= 42) 1241 119 3 ( 93/ 832- 214/ 890) -11.9 E79-E60 N12-N16
11 353 869 (N12E46 L= 64) 418 85 1 ( 322/ 843- 391/ 890) 0.0 E49-E42 N10-N13
12 1146 878 (S06W03 L=113) 191 86 0 (1103/ 857-1190/ 890) -31.0 W00-W05 S08-S04
13 372 819 (N08E45 L= 65) 253 0 0 ( 354/ 783- 394/ 852) 36.9 E47-E43 N06-N10
14 1724 704 (S33W39 L=149) 1760 305 3 (1652/ 608-1817/ 844) 30.5 W31-W49 S38-S27
15 318 644 (S00E56 L= 54) 1821 324 2 ( 227/ 526- 409/ 791) 20.0 E77-E43 S06-N06
16 1491 677 (S27W19 L=129) 261 77 0 (1466/ 638-1514/ 714) 31.0 W16-W21 S28-S25
17 632 636 (S07E33 L= 77) 431 123 0 ( 592/ 589- 682/ 677) 14.0 E36-E28 S09-S05
18 951 220 (S43E35 L= 76) 1392 354 3 ( 806/ 169-1083/ 318) 5.4 E50-E18 S46-S39
|
Download FITS filament maps as tar archive
» All Filament Data of 20251025 ...
|
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.
|
|
|
|