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| 20240804 - Filament data for 16 UTC |
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Available data for 20240804: »06 UTC »08 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 1628 1654 (N34W68 L=315) 928 80 3 (1589/1630-1676/1675) -3.6 W61-W78 N32-N34
2 385 1552 (N48E55 L=192) 2158 293 4 ( 339/1433- 425/1657) -23.0 E87-E43 N38-N55
3 780 1569 (N44E11 L=236) 271 54 0 ( 752/1548- 810/1590) -38.7 E13-E08 N42-N46
4 1028 1414 (N30W06 L=253) 274 92 1 ( 976/1400-1071/1429) -26.6 W02-W09 N28-N31
5 610 1404 (N35E25 L=222) 1499 405 3 ( 432/1366- 785/1428) -9.8 E40-E11 N30-N37
6 1293 1279 (N17W21 L=267) 525 101 3 (1256/1220-1324/1320) 71.6 W18-W22 N13-N19
7 1640 1263 (N11W45 L=292) 644 195 0 (1546/1217-1715/1288) -30.3 W38-W50 N06-N13
8 172 998 (N12E66 L=181) 2746 291 7 ( 89/ 907- 235/1113) 77.0 E89-E57 N06-N19
9 1913 1006 (S11W70 L=317) 1825 122 3 (1889/ 944-1943/1071) -63.4 W65-W77 S14-S06
10 655 702 (S09E28 L=219) 1834 482 5 ( 558/ 584- 795/ 848) 28.8 E36-E16 S16-S01
11 217 656 (S10E70 L=177) 2602 272 3 ( 156/ 548- 283/ 759) -69.0 E78-E63 S17-S03
12 1755 717 (S25W50 L=297) 442 79 1 (1731/ 679-1778/ 755) -50.2 W46-W53 S28-S22
13 519 673 (S10E38 L=209) 263 61 2 ( 492/ 654- 542/ 699) -33.7 E39-E36 S11-S07
14 348 650 (S10E53 L=194) 368 58 1 ( 323/ 632- 377/ 670) -36.9 E56-E50 S11-S08
15 1656 643 (S28W40 L=287) 389 82 1 (1613/ 627-1690/ 670) 0.0 W36-W43 S29-S26
16 363 480 (S22E61 L=186) 2179 281 4 ( 327/ 368- 392/ 607) 50.2 E75-E54 S31-S12
17 710 517 (S22E28 L=218) 905 189 5 ( 649/ 469- 760/ 570) 26.6 E34-E24 S24-S18
18 1714 474 (S44W55 L=302) 995 73 4 (1675/ 446-1743/ 508) -11.3 W48-W63 S46-S40
19 994 165 (S57E25 L=222) 546 41 1 ( 969/ 143-1020/ 194) 33.7 E30-E21 S60-S53
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Download FITS filament maps as tar archive
» All Filament Data of 20240804 ...
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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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