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| 20221003 - Filament data for 11 UTC |
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Available data for 20221003: »06 UTC »07 UTC »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 1356 1832 (N42W66 L=171) 519 36 0 (1341/1804-1371/1858) 24.0 W61-W71 N39-N43
2 337 1559 (N59E55 L= 50) 540 62 1 ( 301/1545- 375/1572) -8.1 E67-E46 N57-N61
3 1505 1535 (N20W47 L=153) 495 73 2 (1479/1494-1529/1567) 68.2 W45-W49 N17-N22
4 1567 1497 (N16W50 L=155) 370 74 1 (1544/1457-1592/1529) 78.7 W48-W51 N13-N18
5 618 1477 (N44E15 L= 90) 243 83 0 ( 603/1439- 637/1516) 53.1 E16-E12 N42-N46
6 275 1295 (N41E52 L= 53) 629 135 0 ( 264/1227- 285/1358) -83.7 E54-E50 N36-N45
7 722 1284 (N29E11 L= 94) 259 104 0 ( 675/1254- 765/1314) -51.3 E13-E08 N26-N32
8 486 1121 (N25E31 L= 74) 658 155 0 ( 427/1076- 556/1166) -45.0 E35-E26 N21-N29
9 247 1051 (N26E55 L= 51) 1291 152 4 ( 187/1006- 303/1113) 18.4 E62-E48 N23-N29
10 586 1030 (N18E26 L= 79) 233 39 2 ( 562/1004- 610/1050) 33.7 E27-E24 N16-N18
11 1651 981 (S14W37 L=142) 844 191 0 (1563/ 937-1728/1027) -4.1 W29-W43 S15-S12
12 282 993 (N22E51 L= 54) 344 54 0 ( 264/ 967- 303/1023) 45.0 E53-E48 N20-N23
13 1869 994 (S21W58 L=163) 662 38 1 (1847/ 964-1890/1019) 21.8 W55-W61 S22-S19
14 619 960 (N13E25 L= 80) 241 94 1 ( 596/ 919- 647/1005) -78.7 E26-E24 N10-N15
15 273 911 (N17E54 L= 51) 1251 235 4 ( 214/ 806- 333/ 980) -57.5 E60-E48 N10-N22
16 1394 636 (S26W11 L=117) 915 268 0 (1322/ 528-1442/ 754) 42.5 W04-W16 S31-S19
17 1140 539 (S24E07 L= 98) 1480 570 0 ( 971/ 359-1322/ 714) 22.1 E24-W08 S32-S18
18 1769 627 (S41W45 L=150) 1194 136 1 (1713/ 594-1828/ 672) 0.0 W37-W54 S42-S39
19 502 342 (S21E60 L= 45) 827 54 0 ( 473/ 314- 530/ 373) 20.0 E66-E55 S23-S19
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Download FITS filament maps as tar archive
» All Filament Data of 20221003 ...
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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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