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| 20150421 - Latest Filament data |
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Available data for 20150421: »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 1008 1849 (N47E35 L= 0) 483 66 1 ( 976/1829-1039/1870) 45.0 E36-E31 N44-N49
2 1079 1692 (N37E19 L= 16) 2022 459 8 (1011/1565-1163/1823) -40.4 E29-E08 N29-N46
3 371 1671 (N17E71 L=324) 2724 235 5 ( 321/1628- 409/1717) 60.3 E75-E67 N13-N21
4 509 1596 (N15E51 L=344) 1318 413 0 ( 467/1450- 567/1712) -39.8 E58-E39 N07-N22
5 346 1528 (N07E62 L=333) 2230 302 4 ( 266/1446- 399/1631) 77.9 E67-E56 N00-N14
6 1725 1456 (N44W39 L= 74) 397 43 0 (1701/1437-1752/1473) 0.0 W35-W41 N42-N44
7 1570 1237 (N23W27 L= 62) 683 278 1 (1511/1120-1633/1375) -42.7 W20-W33 N17-N29
8 1018 1251 (N07E06 L= 29) 383 112 1 ( 989/1198-1042/1308) 90.0 E07-E05 N03-N11
9 361 1207 (S11E47 L=348) 293 61 0 ( 337/1175- 386/1236) 63.4 E47-E45 S13-S09
10 1303 1033 (N03W15 L= 50) 605 190 2 (1209/1004-1379/1070) 21.8 W09-W19 N00-N05
11 1763 938 (N12W49 L= 84) 1934 352 3 (1690/ 804-1848/1058) -40.6 W41-W57 N05-N17
12 1834 877 (N11W58 L= 93) 992 159 3 (1814/ 799-1859/ 948) -56.3 W55-W62 N06-N15
13 1084 859 (S13W08 L= 43) 269 100 0 (1046/ 807-1133/ 899) 74.1 W06-W09 S16-S09
14 773 885 (S19E11 L= 24) 242 108 0 ( 719/ 872- 831/ 898) 15.9 E14-E07 S20-S18
15 1713 862 (N06W47 L= 82) 327 44 1 (1693/ 833-1736/ 894) 68.2 W46-W49 N03-N08
16 1826 757 (N04W63 L= 98) 420 104 0 (1804/ 738-1852/ 780) 8.1 W59-W66 N03-N06
17 872 741 (S25E01 L= 34) 644 194 0 ( 774/ 715- 966/ 778) 35.0 E07-W03 S27-S20
18 1045 590 (S29W15 L= 49) 359 62 2 (1007/ 568-1081/ 612) 11.3 W12-W17 S30-S27
19 821 529 (S40W03 L= 38) 464 109 0 ( 766/ 516- 878/ 548) 29.7 E01-W06 S41-S37
20 1308 224 (S42W54 L= 89) 608 79 0 (1270/ 208-1342/ 242) 53.1 W50-W56 S43-S39
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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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