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| 20230727 - Filament data for 07 UTC |
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Available data for 20230727: »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
1 927 1871 (N72W04 L=152) 569 50 1 ( 913/1840- 945/1899) 48.4 W00-W09 N67-N76
2 789 1846 (N71E23 L=125) 490 31 0 ( 771/1821- 810/1868) -80.5 E26-E18 N67-N73
3 1577 1561 (N33W52 L=200) 451 89 0 (1535/1544-1619/1576) -6.3 W47-W56 N31-N33
4 1112 1529 (N37W12 L=160) 368 85 1 (1067/1499-1151/1557) 23.2 W08-W15 N35-N38
5 1185 1514 (N35W17 L=165) 309 53 3 (1166/1485-1202/1544) -90.0 W15-W18 N32-N37
6 1546 1474 (N27W45 L=193) 783 177 1 (1509/1390-1579/1543) 79.7 W42-W46 N21-N32
7 1695 1479 (N25W60 L=208) 706 130 1 (1655/1423-1717/1531) 24.8 W52-W65 N22-N28
8 1779 1471 (N23W71 L=219) 764 96 1 (1744/1440-1821/1497) -21.8 W66-W77 N20-N24
9 793 1359 (N28E13 L=135) 501 185 2 ( 765/1278- 839/1433) -74.7 E14-E09 N22-N33
10 389 1282 (N25E45 L=103) 2624 438 2 ( 276/1156- 559/1340) 4.6 E55-E30 N17-N29
11 1253 1262 (N18W17 L=165) 383 133 1 (1218/1224-1302/1305) -45.0 W14-W20 N15-N20
12 384 1069 (N12E44 L=104) 556 110 1 ( 337/1026- 418/1107) -35.5 E47-E40 N09-N14
13 484 1001 (N08E36 L=112) 298 53 1 ( 462/ 973- 508/1032) 76.0 E37-E33 N05-N09
14 1747 857 (S13W50 L=198) 510 60 0 (1727/ 830-1770/ 885) 56.3 W47-W52 S14-S11
15 667 796 (S06E25 L=123) 216 111 0 ( 621/ 763- 707/ 812) -31.0 E27-E22 S08-S04
16 243 722 (S09E63 L= 85) 751 92 1 ( 227/ 681- 264/ 772) 56.3 E65-E59 S12-S06
17 434 407 (S32E58 L= 90) 573 126 0 ( 411/ 356- 466/ 467) 66.0 E60-E54 S36-S27
18 841 399 (S35E21 L=127) 429 112 1 ( 785/ 386- 896/ 414) -14.0 E24-E16 S35-S32
19 1235 249 (S54W11 L=159) 479 63 1 (1200/ 233-1267/ 270) -20.6 W06-W14 S55-S51
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Download FITS filament maps as tar archive
» All Filament Data of 20230727 ...
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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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