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| 20251210 - Filament data for 12 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 1517 1740 (N39W55 L=277) 1920 175 2 (1430/1701-1598/1768) -21.8 W45-W63 N35-N41
2 1304 1719 (N40W33 L=255) 442 58 1 (1276/1694-1338/1749) -78.7 W31-W35 N37-N42
3 445 1662 (N49E45 L=177) 528 60 1 ( 425/1629- 465/1688) -78.7 E48-E41 N46-N51
4 1252 1503 (N26W21 L=243) 234 50 1 (1225/1484-1279/1524) -45.0 W19-W22 N24-N27
5 553 1309 (N22E27 L=195) 572 134 0 ( 480/1287- 613/1335) -5.7 E32-E22 N20-N24
6 1771 1274 (N06W54 L=276) 387 97 0 (1748/1226-1792/1325) -80.5 W52-W55 N02-N08
7 1689 1271 (N07W46 L=269) 266 77 1 (1647/1253-1732/1286) 0.0 W43-W50 N05-N07
8 1819 1233 (N03W58 L=280) 426 79 1 (1799/1192-1850/1257) 26.6 W55-W61 N00-N04
9 315 1116 (N13E46 L=176) 481 96 0 ( 288/1067- 342/1161) -56.3 E48-E43 N10-N16
10 1890 975 (S13W63 L=285) 4507 280 11 (1828/ 838-1951/1087) -56.3 W55-W72 S21-S06
11 1794 958 (S13W52 L=274) 1906 376 3 (1731/ 817-1847/1059) -86.2 W45-W57 S21-S06
12 1660 839 (S19W40 L=262) 1182 225 2 (1637/ 732-1682/ 950) 85.6 W37-W41 S25-S11
13 1725 903 (S15W45 L=267) 425 71 2 (1707/ 857-1747/ 937) 78.7 W43-W47 S18-S13
14 1123 897 (S09W04 L=226) 189 55 0 (1097/ 873-1146/ 925) 33.7 W02-W05 S10-S07
15 671 759 (S12E25 L=197) 246 84 2 ( 637/ 731- 694/ 779) 11.3 E27-E22 S13-S10
16 1353 654 (S26W17 L=239) 792 235 0 (1277/ 576-1409/ 756) 48.0 W11-W20 S30-S20
17 1140 657 (S23W03 L=225) 348 117 0 (1108/ 605-1171/ 706) 50.2 W00-W05 S26-S20
18 840 651 (S20E16 L=206) 267 94 0 ( 828/ 603- 855/ 698) 71.6 E17-E14 S23-S17
19 608 470 (S29E37 L=185) 479 150 2 ( 543/ 451- 682/ 490) -21.8 E41-E31 S30-S26
20 867 316 (S44E24 L=198) 307 70 1 ( 827/ 294- 903/ 338) 0.0 E27-E20 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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