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| 20260101 - Filament data for 08 UTC |
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Available data for 20260101: »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 1540 1656 (N38W43 L=338) 4268 629 6 (1237/1558-1771/1735) -10.0 W18-W69 N31-N43
2 576 1622 (N36E34 L=260) 855 157 2 ( 526/1549- 613/1680) -42.3 E41-E29 N30-N40
3 824 1496 (N26E13 L=282) 262 91 1 ( 800/1468- 850/1532) -63.4 E14-E10 N24-N28
4 1828 1265 (N12W58 L=353) 467 0 0 (1802/1247-1853/1284) 18.4 W55-W61 N10-N13
5 784 1170 (N06E14 L=280) 209 89 0 ( 770/1129- 798/1225) 90.0 E15-E13 N03-N09
6 1903 1145 (N05W66 L= 0) 799 81 4 (1873/1115-1937/1183) 33.7 W61-W71 N03-N07
7 994 1125 (N03E02 L=293) 384 161 0 ( 924/1098-1070/1163) 15.9 E05-W02 N01-N05
8 920 972 (S06E06 L=288) 552 230 3 ( 852/ 897-1011/1018) 31.0 E10-W00 S10-S03
9 323 864 (S11E48 L=247) 689 152 0 ( 305/ 792- 340/ 941) 83.7 E49-E46 S15-S06
10 959 921 (S09E04 L=290) 255 84 0 ( 917/ 902- 999/ 940) 11.3 E06-E01 S10-S07
11 528 772 (S17E33 L=262) 802 238 0 ( 512/ 660- 554/ 887) 70.3 E35-E29 S24-S10
12 921 845 (S14E06 L=288) 215 21 0 ( 901/ 822- 941/ 868) -45.0 E07-E05 S14-S12
13 998 841 (S14E02 L=293) 292 61 1 ( 971/ 811-1023/ 868) -45.0 E03-W00 S15-S12
14 668 831 (S14E22 L=272) 365 87 2 ( 628/ 802- 700/ 860) -11.3 E25-E20 S15-S12
15 639 750 (S19E25 L=269) 431 158 1 ( 600/ 708- 696/ 820) -60.3 E27-E21 S21-S14
16 1758 755 (S19W53 L=347) 454 81 0 (1723/ 729-1793/ 791) -20.6 W48-W56 S20-S16
17 1764 656 (S25W56 L=351) 524 73 1 (1719/ 640-1807/ 677) -5.2 W51-W62 S25-S23
18 489 512 (S34E42 L=252) 805 281 0 ( 431/ 420- 565/ 627) -75.1 E46-E38 S40-S25
19 904 313 (S50E12 L=282) 288 29 0 ( 884/ 292- 925/ 338) -63.4 E13-E10 S51-S47
20 809 161 (S65E34 L=260) 3643 266 6 ( 704/ 126- 917/ 213) 0.0 E55-E15 S70-S58
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Data will be available after one hour of observations. |
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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