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| 20221011 - Latest Filament data |
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Available data for 20221011: »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 819 1791 (N61W18 L= 18) 518 43 0 ( 791/1766- 844/1811) 78.7 W15-W21 N58-N63
2 1224 1782 (N43W47 L= 47) 855 144 1 (1148/1753-1295/1803) -48.8 W43-W50 N39-N47
3 1564 1748 (N28W73 L= 73) 761 79 1 (1520/1734-1607/1765) -18.4 W68-W80 N26-N30
4 616 1659 (N58E11 L=348) 1272 225 3 ( 514/1594- 700/1717) 0.0 E24-W00 N55-N61
5 1365 1611 (N28W42 L= 41) 770 180 0 (1286/1591-1460/1631) -32.5 W37-W48 N24-N31
6 1574 1556 (N19W54 L= 53) 571 102 1 (1539/1528-1616/1580) -59.0 W50-W57 N15-N20
7 430 1543 (N55E35 L=324) 478 59 1 ( 407/1502- 455/1572) 53.1 E38-E31 N52-N57
8 1472 1423 (N15W39 L= 38) 813 293 0 (1333/1366-1588/1465) -45.0 W31-W44 N08-N21
9 860 1352 (N29E01 L=359) 213 77 1 ( 833/1331- 896/1378) -63.4 E01-W01 N26-N31
10 433 1174 (N29E35 L=325) 339 112 0 ( 378/1151- 482/1197) 0.0 E39-E30 N28-N30
11 611 1055 (N18E23 L=336) 206 31 1 ( 593/1037- 636/1074) -18.4 E24-E21 N16-N19
12 1629 711 (S30W30 L= 29) 680 159 0 (1558/ 687-1681/ 762) -5.7 W24-W34 S31-S27
13 1086 601 (S19E08 L=351) 426 153 0 (1071/ 533-1105/ 676) 66.0 E10-E04 S24-S15
14 897 439 (S24E25 L=334) 763 284 0 ( 804/ 358- 945/ 558) 26.6 E34-E17 S28-S17
15 1469 443 (S43W13 L= 12) 2004 343 4 (1326/ 373-1604/ 538) 2.3 W00-W26 S45-S39
16 1053 402 (S31E17 L=342) 367 104 0 (1020/ 353-1085/ 439) 26.6 E21-E13 S34-S29
17 641 300 (S27E51 L=308) 952 141 2 ( 579/ 266- 700/ 344) -63.4 E53-E48 S31-S22
18 1101 255 (S45E23 L=336) 1510 221 1 (1034/ 214-1192/ 320) -82.4 E26-E15 S51-S36
19 524 293 (S25E64 L=295) 914 78 2 ( 486/ 270- 558/ 313) -31.0 E68-E58 S27-S23
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Download FITS filament maps as tar archive
» All Filament Data of 20221011 ...
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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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