|
|
|
|
| 20231002 - Filament data for 12 UTC |
|
Available data for 20231002: »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 1007 1754 (N51W30 L= 10) 300 37 1 ( 983/1731-1033/1769) -11.3 W26-W32 N49-N52
2 1533 1644 (N25W58 L= 38) 765 73 1 (1496/1613-1558/1673) -78.7 W55-W61 N22-N27
3 1538 1533 (N19W50 L= 30) 347 70 1 (1519/1498-1555/1568) 26.6 W47-W53 N17-N20
4 1301 1510 (N25W32 L= 13) 401 111 0 (1245/1489-1354/1533) -39.8 W29-W35 N22-N28
5 1202 1401 (N22W22 L= 2) 650 225 0 (1103/1351-1283/1437) -48.4 W16-W24 N17-N26
6 244 1405 (N49E62 L=278) 512 58 0 ( 218/1379- 274/1422) 6.3 E67-E56 N47-N50
7 972 1216 (N19W02 L=342) 936 361 1 ( 884/1084-1096/1335) -75.3 W00-W05 N08-N27
8 410 1259 (N36E36 L=304) 1174 198 2 ( 338/1208- 501/1312) -29.4 E44-E28 N31-N40
9 579 1135 (N24E24 L=316) 336 77 0 ( 548/1106- 619/1162) -45.0 E26-E21 N21-N26
10 174 1021 (N25E65 L=275) 667 66 1 ( 156/ 989- 191/1060) -63.4 E67-E62 N23-N27
11 204 930 (N20E62 L=279) 2790 212 8 ( 137/ 853- 251/1039) 51.3 E71-E55 N14-N25
12 1466 886 (S13W22 L= 2) 952 302 0 (1405/ 770-1523/1028) 42.7 W15-W28 S18-S06
13 1746 936 (S20W44 L= 24) 906 172 2 (1725/ 850-1762/1025) 63.4 W41-W46 S24-S14
14 707 914 (N08E21 L=319) 613 169 0 ( 643/ 858- 771/ 979) -66.0 E23-E18 N04-N13
15 412 888 (N13E42 L=298) 293 66 1 ( 376/ 865- 443/ 908) -31.0 E44-E39 N11-N14
16 1206 635 (S20E00 L=340) 295 99 1 (1182/ 611-1252/ 671) -63.4 E01-W02 S22-S17
17 1466 615 (S30W16 L=356) 551 104 1 (1440/ 569-1506/ 648) 33.7 W13-W19 S32-S27
18 981 454 (S26E19 L=321) 449 171 0 ( 933/ 395-1043/ 516) 20.0 E24-E13 S28-S23
19 958 267 (S38E31 L=309) 726 124 0 ( 930/ 208- 982/ 326) 51.3 E36-E27 S43-S33
|
Download FITS filament maps as tar archive
» All Filament Data of 20231002 ...
|
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.
|
|
|
|