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| 20240816 - Filament data for 12 UTC |
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Available data for 20240816: »06 UTC »07 UTC »08 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC »16 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1756 1492 (N17W69 L=159) 1078 117 3 (1711/1460-1807/1524) -33.7 W63-W75 N14-N20
2 1548 1438 (N20W45 L=135) 572 86 2 (1520/1391-1572/1472) 33.7 W42-W48 N17-N22
3 1726 1420 (N15W60 L=150) 812 88 1 (1687/1380-1761/1459) -45.0 W56-W64 N11-N16
4 624 1402 (N37E22 L= 69) 231 86 0 ( 605/1362- 647/1441) 45.0 E23-E19 N34-N39
5 1088 1170 (N14W06 L= 97) 218 103 1 (1048/1141-1130/1209) -59.0 W04-W08 N11-N17
6 155 1143 (N25E70 L= 20) 1218 133 2 ( 123/1087- 189/1203) -26.6 E78-E63 N21-N28
7 1596 941 (S09W34 L=125) 238 89 0 (1583/ 897-1610/ 988) -90.0 W33-W35 S12-S06
8 1221 886 (S05W09 L= 99) 491 210 1 (1164/ 836-1286/ 979) -60.9 W06-W12 S08-N01
9 1837 890 (S19W57 L=147) 901 115 1 (1805/ 847-1886/ 928) 5.2 W52-W63 S21-S16
10 1513 895 (S10W28 L=118) 268 68 0 (1491/ 868-1537/ 926) -68.2 W26-W29 S12-S07
11 350 838 (N05E48 L= 42) 412 110 0 ( 311/ 803- 397/ 874) 18.4 E52-E43 N03-N06
12 1285 775 (S13W11 L=102) 409 97 3 (1244/ 740-1321/ 806) 36.9 W08-W13 S14-S11
13 325 597 (S10E59 L= 31) 1676 194 3 ( 282/ 527- 389/ 673) -68.2 E62-E55 S14-S04
14 714 548 (S17E29 L= 61) 362 94 1 ( 695/ 496- 731/ 596) 71.6 E30-E27 S20-S14
15 293 538 (S13E67 L= 23) 970 49 0 ( 272/ 500- 311/ 572) 59.0 E70-E63 S16-S11
16 1441 530 (S33W19 L=109) 711 117 0 (1382/ 510-1494/ 566) 0.0 W14-W23 S34-S30
17 485 462 (S20E50 L= 40) 515 97 0 ( 459/ 413- 510/ 514) 37.9 E54-E45 S23-S16
18 1007 455 (S29E12 L= 78) 460 92 0 ( 988/ 408-1029/ 505) 56.3 E14-E10 S32-S25
19 594 328 (S31E50 L= 41) 1145 177 1 ( 517/ 300- 681/ 349) -3.4 E57-E40 S33-S29
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Download FITS filament maps as tar archive
» All Filament Data of 20240816 ...
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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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