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| 20230911 - Filament data for 06 UTC |
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Available data for 20230911: »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 1034 1747 (N51W29 L=290) 553 74 1 (1008/1712-1060/1780) 6.3 W25-W34 N48-N53
2 1448 1717 (N35W58 L=319) 397 41 0 (1425/1702-1476/1735) -56.3 W55-W60 N33-N36
3 918 1679 (N50W15 L=275) 365 48 0 ( 890/1658- 949/1697) -53.1 W12-W16 N48-N52
4 1688 1612 (N20W73 L=333) 1358 80 3 (1654/1584-1728/1643) -33.7 W68-W79 N18-N22
5 515 1357 (N39E28 L=233) 1452 290 4 ( 404/1280- 628/1392) -28.8 E39-E19 N31-N43
6 1038 1328 (N24W09 L=269) 1074 349 1 ( 905/1300-1208/1356) -20.2 W00-W19 N20-N27
7 1169 1233 (N15W14 L=274) 196 19 0 (1147/1218-1192/1252) -45.0 W12-W14 N14-N16
8 1761 1150 (S06W51 L=312) 1408 161 5 (1723/1072-1789/1228) 45.0 W46-W56 S09-S01
9 554 1076 (N20E28 L=233) 933 238 1 ( 467/ 998- 648/1137) -47.7 E34-E23 N14-N25
10 205 958 (N19E62 L=199) 2623 439 5 ( 98/ 811- 342/1096) -28.5 E85-E49 N08-N27
11 1659 620 (S35W34 L=295) 6658 815 13 (1458/ 384-1849/ 959) 33.4 W14-W56 S49-S18
12 1272 896 (S06W11 L=272) 286 64 0 (1251/ 860-1299/ 935) -90.0 W10-W12 S08-S03
13 1216 857 (S07W07 L=268) 272 103 0 (1170/ 846-1274/ 868) -26.6 W04-W10 S08-S05
14 1246 663 (S19W04 L=265) 646 268 1 (1180/ 564-1275/ 770) 48.0 E02-W07 S23-S12
15 1340 312 (S49W02 L=262) 391 61 1 (1321/ 287-1362/ 347) 59.0 W00-W03 S51-S45
16 1254 260 (S51E08 L=253) 674 79 1 (1219/ 233-1293/ 285) -38.7 E10-E04 S53-S47
17 929 237 (S42E34 L=227) 498 78 0 ( 892/ 219- 970/ 260) 0.0 E37-E29 S42-S40
18 1144 209 (S52E20 L=240) 536 76 1 (1111/ 186-1185/ 231) 0.0 E24-E15 S53-S50
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Download FITS filament maps as tar archive
» All Filament Data of 20230911 ...
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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.
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