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| 20231002 - Filament data for 11 UTC |
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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 1004 1752 (N51W29 L= 10) 301 45 1 ( 980/1729-1030/1767) -11.3 W26-W32 N49-N52
2 1532 1599 (N23W54 L= 35) 1004 190 2 (1501/1495-1553/1665) 29.7 W45-W60 N17-N26
3 1300 1505 (N25W32 L= 13) 455 134 0 (1242/1469-1351/1529) -60.3 W29-W34 N21-N28
4 1197 1396 (N22W21 L= 2) 662 222 2 (1097/1343-1273/1433) -45.0 W15-W24 N17-N26
5 240 1403 (N49E63 L=278) 483 59 0 ( 215/1379- 271/1418) 11.3 E67-E56 N47-N50
6 970 1207 (N18W02 L=343) 891 361 2 ( 886/1074-1095/1328) -78.7 E02-W05 N07-N27
7 404 1257 (N36E37 L=304) 1101 190 3 ( 328/1208- 494/1307) -29.4 E45-E29 N31-N40
8 572 1132 (N24E25 L=316) 313 74 0 ( 541/1100- 605/1161) -59.0 E26-E22 N21-N26
9 171 1023 (N26E65 L=275) 743 69 3 ( 154/ 983- 186/1061) 63.4 E68-E62 N23-N27
10 196 931 (N20E63 L=278) 2468 210 7 ( 135/ 853- 244/1036) 51.3 E72-E55 N15-N25
11 1741 938 (S19W43 L= 24) 878 176 2 (1721/ 857-1758/1033) 68.2 W40-W46 S23-S13
12 1459 884 (S13W21 L= 2) 951 298 0 (1399/ 769-1517/1026) 38.2 W14-W28 S18-S06
13 697 913 (N09E22 L=319) 566 172 0 ( 637/ 854- 762/ 978) -66.0 E23-E18 N04-N13
14 408 886 (N13E42 L=299) 295 73 0 ( 373/ 859- 430/ 905) -31.0 E45-E40 N11-N14
15 1209 627 (S21E00 L=341) 299 117 0 (1175/ 608-1260/ 659) -45.0 E01-W03 S22-S18
16 1458 609 (S30W15 L=356) 587 111 1 (1424/ 557-1496/ 644) 29.7 W11-W18 S32-S27
17 974 449 (S26E20 L=321) 434 171 0 ( 927/ 392-1035/ 512) 22.6 E25-E13 S28-S23
18 954 262 (S39E32 L=309) 690 126 0 ( 925/ 204- 977/ 325) 54.0 E37-E28 S44-S33
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Download FITS filament maps as tar archive
» All Filament Data of 20231002 ...
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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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