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| 20230926 - Filament data for 09 UTC |
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Available data for 20230926: »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
1 877 1619 (N47W10 L= 71) 343 43 0 ( 857/1584- 894/1644) 59.0 W08-W12 N43-N48
2 958 1619 (N44W16 L= 77) 324 43 0 ( 934/1591- 979/1642) 63.4 W14-W18 N41-N45
3 1583 1448 (N14W48 L=110) 689 145 2 (1565/1379-1608/1527) 56.3 W45-W52 N09-N18
4 1463 1372 (N14W36 L= 98) 462 98 1 (1404/1338-1499/1395) -15.9 W32-W39 N11-N15
5 859 1280 (N26E03 L= 58) 195 87 0 ( 812/1269- 904/1292) -18.4 E06-W00 N24-N26
6 788 1197 (N23E09 L= 52) 308 64 1 ( 756/1163- 812/1220) -76.0 E11-E07 N20-N24
7 1758 1110 (S10W49 L=110) 414 108 0 (1720/1067-1793/1143) 6.3 W44-W53 S10-S08
8 1670 1042 (S10W40 L=101) 429 96 1 (1640/1004-1697/1092) -74.1 W37-W41 S13-S06
9 477 987 (N18E35 L= 26) 570 146 1 ( 433/ 943- 533/1038) 18.4 E38-E29 N15-N19
10 230 969 (N21E58 L= 3) 1066 219 1 ( 156/ 911- 299/1029) -19.4 E68-E51 N16-N25
11 793 934 (N08E15 L= 46) 253 83 1 ( 777/ 897- 814/ 980) 59.0 E17-E13 N05-N10
12 159 883 (N17E70 L=351) 562 78 1 ( 141/ 843- 176/ 921) -90.0 E72-E67 N14-N19
13 1703 766 (S28W38 L= 99) 574 164 0 (1667/ 715-1730/ 859) 53.1 W33-W41 S30-S22
14 1332 834 (S12W12 L= 74) 264 65 0 (1307/ 802-1354/ 853) 33.7 W10-W13 S13-S10
15 1609 783 (S24W30 L= 91) 670 171 1 (1562/ 714-1659/ 847) 29.1 W25-W34 S26-S21
16 1198 663 (S18W00 L= 61) 921 393 1 (1038/ 637-1379/ 697) -18.4 E09-W12 S22-S13
17 1715 595 (S41W39 L=100) 499 56 1 (1688/ 574-1737/ 626) 21.8 W35-W42 S42-S38
18 409 462 (S12E60 L= 1) 1238 234 1 ( 384/ 373- 432/ 568) 37.4 E69-E51 S18-S05
19 696 427 (S20E38 L= 23) 384 64 1 ( 678/ 394- 716/ 460) 68.2 E40-E35 S22-S17
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Download FITS filament maps as tar archive
» All Filament Data of 20230926 ...
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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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