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| 20150608 - Filament data for 09 UTC |
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Available data for 20150608: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1134 1691 (N46E04 L=118) 1481 315 4 (1082/1614-1183/1793) -76.0 E07-W01 N40-N56
2 615 1721 (N39E47 L= 75) 492 122 0 ( 591/1684- 636/1749) -29.7 E50-E43 N36-N40
3 545 1552 (N26E43 L= 79) 1525 275 3 ( 462/1473- 639/1669) 68.2 E48-E39 N19-N35
4 1480 1579 (N44W28 L=150) 721 158 1 (1422/1556-1540/1599) 20.0 W22-W33 N41-N46
5 434 1499 (N21E50 L= 72) 380 94 2 ( 404/1472- 460/1523) -18.4 E53-E47 N19-N22
6 561 1414 (N17E37 L= 85) 529 143 1 ( 499/1377- 605/1470) 50.2 E40-E34 N14-N20
7 1470 1423 (N32W25 L=148) 415 114 0 (1443/1375-1487/1462) -80.5 W23-W26 N28-N34
8 933 1300 (N15E10 L=113) 221 106 1 ( 879/1287- 986/1314) 8.1 E13-E06 N14-N17
9 692 1252 (N09E24 L= 98) 384 102 2 ( 669/1215- 721/1289) -45.0 E25-E21 N06-N11
10 1181 1218 (N14W07 L=129) 547 144 2 (1118/1181-1217/1270) 51.3 W03-W09 N11-N17
11 1213 1087 (N06W10 L=133) 899 342 3 (1074/ 967-1301/1179) -29.4 W01-W17 N00-N10
12 231 950 (S16E56 L= 66) 815 245 0 ( 189/ 861- 245/1061) 69.0 E60-E54 S21-S08
13 391 1004 (S10E41 L= 81) 418 104 2 ( 347/ 975- 422/1022) -15.9 E45-E38 S11-S08
14 1638 922 (N02W42 L=164) 595 161 2 (1619/ 869-1660/ 981) -63.4 W40-W44 N00-N06
15 817 893 (S11E11 L=112) 399 165 1 ( 725/ 875- 888/ 917) 16.7 E16-E06 S11-S08
16 1181 792 (S12W13 L=135) 723 173 3 (1139/ 722-1219/ 881) -66.0 W09-W16 S15-S06
17 1609 728 (S10W43 L=166) 507 118 0 (1582/ 661-1646/ 783) 82.9 W41-W45 S13-S05
18 1722 689 (S10W55 L=177) 356 57 1 (1704/ 658-1745/ 715) 63.4 W53-W56 S12-S08
19 681 564 (S34E17 L=105) 286 57 1 ( 655/ 547- 706/ 584) 36.9 E19-E15 S35-S32
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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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