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| 20251210 - Filament data for 10 UTC |
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Available data for 20251210: »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 1509 1736 (N38W54 L=277) 2039 189 4 (1420/1686-1589/1769) -30.3 W45-W62 N33-N41
2 1285 1719 (N40W32 L=255) 416 58 1 (1251/1691-1313/1744) -36.9 W29-W33 N38-N42
3 436 1659 (N49E46 L=178) 545 59 1 ( 415/1624- 458/1685) -78.7 E49-E42 N46-N51
4 1657 1516 (N22W52 L=276) 334 61 0 (1626/1498-1692/1533) -9.5 W49-W55 N20-N22
5 532 1305 (N22E28 L=195) 568 151 0 ( 458/1283- 594/1330) -10.3 E34-E23 N20-N24
6 1768 1254 (N05W53 L=276) 304 50 0 (1754/1219-1779/1283) -76.0 W52-W54 N02-N06
7 1667 1267 (N06W45 L=268) 301 93 1 (1620/1245-1719/1282) 0.0 W40-W49 N05-N07
8 1810 1232 (N03W57 L=280) 374 68 1 (1790/1199-1841/1253) 18.4 W54-W60 N01-N04
9 301 1115 (N13E47 L=176) 430 117 1 ( 274/1066- 330/1170) -54.5 E49-E44 N10-N17
10 1879 969 (S13W61 L=284) 3507 243 9 (1816/ 892-1945/1059) -54.0 W54-W71 S18-S07
11 1766 1006 (S10W49 L=272) 797 185 2 (1717/ 958-1820/1055) -16.7 W44-W54 S12-S06
12 1645 837 (S18W38 L=262) 1013 192 3 (1614/ 745-1663/ 935) -90.0 W36-W39 S24-S12
13 1712 895 (S16W44 L=267) 377 85 2 (1690/ 850-1731/ 932) 78.7 W42-W45 S18-S13
14 1783 859 (S19W51 L=274) 288 66 0 (1771/ 824-1793/ 896) 90.0 W49-W51 S20-S16
15 1265 837 (S14W12 L=235) 211 93 0 (1225/ 803-1290/ 870) 36.9 W09-W13 S15-S12
16 1123 653 (S24W02 L=225) 318 121 0 (1091/ 602-1152/ 706) 63.4 E01-W03 S26-S20
17 1323 619 (S28W14 L=238) 580 171 1 (1267/ 563-1368/ 694) 53.1 W10-W17 S31-S23
18 426 525 (S23E50 L=173) 319 62 2 ( 408/ 496- 444/ 555) 63.4 E52-E47 S24-S20
19 856 313 (S44E26 L=198) 333 92 1 ( 812/ 296- 897/ 333) 0.0 E29-E21 S44-S42
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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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