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| 20241022 - Filament data for 12 UTC |
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Available data for 20241022: »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 1221 1528 (N27W27 L=313) 562 104 2 (1181/1497-1280/1548) -15.9 W24-W31 N25-N29
2 1606 1529 (N15W53 L=339) 933 123 1 (1540/1510-1676/1548) -17.1 W47-W60 N13-N18
3 249 1335 (N43E54 L=232) 649 96 1 ( 207/1303- 298/1360) 0.0 E60-E46 N41-N44
4 1286 1281 (N12W22 L=307) 1236 434 0 (1126/1179-1454/1339) -41.2 W12-W28 N01-N18
5 1748 1278 (S02W52 L=338) 778 132 0 (1686/1241-1792/1303) -18.4 W46-W56 S04-N00
6 1851 1178 (S10W59 L=345) 1396 217 3 (1824/1082-1902/1254) 41.6 W54-W68 S15-S06
7 799 1111 (N16E10 L=275) 499 170 1 ( 771/1037- 846/1184) -90.0 E11-E09 N10-N20
8 313 1003 (N21E47 L=239) 332 85 0 ( 288/ 976- 348/1042) -51.3 E48-E43 N18-N23
9 1702 779 (S28W37 L=322) 2355 517 0 (1565/ 555-1826/ 946) 30.7 W22-W50 S39-S21
10 698 892 (N06E22 L=264) 626 118 3 ( 642/ 865- 767/ 928) -29.7 E24-E17 N03-N08
11 271 886 (N15E53 L=233) 310 50 0 ( 247/ 870- 300/ 900) -18.4 E55-E49 N14-N16
12 1302 642 (S24W06 L=291) 1041 332 3 (1206/ 532-1406/ 758) 25.2 E03-W14 S27-S19
13 704 583 (S11E31 L=255) 1504 371 2 ( 634/ 515- 779/ 687) -90.0 E33-E25 S16-S04
14 389 446 (S13E61 L=224) 5050 450 16 ( 259/ 309- 522/ 560) -76.0 E73-E49 S23-S03
15 543 509 (S12E44 L=241) 369 76 0 ( 512/ 470- 572/ 536) -90.0 E46-E43 S14-S09
16 1429 396 (S45W08 L=294) 319 83 0 (1403/ 359-1450/ 439) 45.0 W05-W10 S47-S42
17 1005 315 (S36E25 L=261) 1019 131 2 ( 952/ 274-1065/ 359) 10.3 E29-E18 S39-S33
18 888 151 (S46E49 L=237) 559 50 0 ( 863/ 123- 909/ 181) 45.0 E54-E44 S49-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20241022 ...
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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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