|
|
|
|
| 20241230 - Filament data for 11 UTC |
|
Available data for 20241230: »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 1391 1562 (N30W28 L=124) 2186 572 3 (1174/1470-1661/1680) -20.9 W13-W47 N23-N39
2 462 1513 (N30E40 L= 57) 872 131 3 ( 413/1449- 503/1568) -38.7 E46-E35 N25-N33
3 1216 1449 (N22W13 L=110) 545 159 2 (1181/1383-1239/1511) 76.0 W11-W14 N18-N26
4 1097 1463 (N24W06 L=103) 320 111 0 (1047/1442-1145/1480) 0.0 W02-W08 N22-N24
5 1863 1303 (N13W64 L=161) 677 71 4 (1831/1266-1896/1335) -45.0 W60-W68 N10-N15
6 1324 1232 (N09W19 L=115) 276 99 0 (1308/1180-1341/1291) 74.1 W17-W20 N05-N12
7 195 758 (S15E64 L= 33) 4013 569 10 ( 110/ 502- 253/1029) 77.3 E76-E59 S30-N01
8 765 962 (S06E16 L= 81) 273 63 3 ( 734/ 929- 793/ 993) 26.6 E17-E13 S07-S03
9 1869 861 (S13W62 L=159) 3967 349 9 (1777/ 729-1941/ 988) 58.0 W54-W74 S21-S05
10 817 923 (S08E13 L= 84) 425 83 2 ( 790/ 882- 846/ 959) -53.1 E14-E10 S10-S06
11 326 844 (S11E48 L= 49) 890 128 2 ( 274/ 810- 387/ 887) 15.3 E52-E41 S12-S08
12 512 687 (S21E36 L= 61) 1901 510 4 ( 348/ 627- 643/ 819) 0.0 E48-E25 S25-S13
13 1896 767 (S19W69 L=166) 692 79 1 (1881/ 727-1908/ 809) 90.0 W67-W72 S21-S16
14 1564 615 (S29W38 L=134) 289 79 1 (1552/ 582-1583/ 665) -68.2 W36-W40 S30-S25
15 1231 555 (S32W13 L=110) 212 88 0 (1189/ 544-1276/ 570) -9.5 W10-W16 S32-S31
16 895 412 (S41E12 L= 84) 875 256 1 ( 793/ 354-1002/ 486) 24.0 E21-E03 S45-S36
17 1268 208 (S61W26 L=123) 621 45 1 (1240/ 187-1298/ 236) -6.3 W22-W31 S63-S57
18 1190 201 (S61W16 L=113) 649 63 1 (1161/ 169-1222/ 228) -40.6 W11-W20 S65-S58
|
Download FITS filament maps as tar archive
» All Filament Data of 20241230 ...
|
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.
|
|
|
|