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| 20150328 - Filament data for 11 UTC |
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Available data for 20150328: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1113 1813 (N46E24 L=329) 375 102 0 (1080/1781-1141/1843) -24.0 E28-E19 N43-N47
2 960 1687 (N30E25 L=328) 350 119 1 ( 905/1657-1019/1700) 14.0 E28-E20 N28-N31
3 1482 1621 (N44W12 L= 5) 815 118 2 (1439/1578-1522/1648) -38.7 W08-W16 N41-N47
4 1554 1602 (N46W19 L= 12) 449 113 1 (1534/1554-1581/1635) 82.9 W17-W21 N41-N49
5 1713 1383 (N36W36 L= 28) 3981 481 8 (1585/1203-1788/1536) -38.7 W23-W43 N25-N44
6 400 1486 (N04E54 L=299) 487 137 1 ( 363/1447- 428/1507) -14.0 E58-E50 N01-N05
7 1057 1258 (N07E05 L=348) 233 85 0 (1042/1217-1078/1301) -53.1 E05-E02 N04-N09
8 180 1259 (S13E67 L=286) 743 141 1 ( 145/1222- 208/1294) -76.0 E72-E63 S14-S10
9 1557 1160 (N16W27 L= 20) 494 125 0 (1510/1097-1586/1224) -32.0 W22-W30 N13-N18
10 1809 1095 (N21W48 L= 41) 418 75 0 (1780/1072-1836/1121) 0.0 W45-W51 N20-N22
11 1475 1007 (N05W26 L= 19) 789 176 3 (1413/ 957-1551/1076) -10.3 W20-W31 N03-N07
12 1875 976 (N17W58 L= 51) 865 116 1 (1856/ 925-1892/1030) -39.8 W55-W61 N14-N20
13 1720 935 (N09W45 L= 38) 1245 272 2 (1625/ 904-1806/ 958) 25.0 W38-W53 N04-N11
14 1730 754 (N00W52 L= 45) 976 160 1 (1664/ 693-1782/ 828) 63.4 W49-W55 S05-N05
15 1235 775 (S14W19 L= 12) 317 129 0 (1171/ 761-1303/ 794) 20.6 W15-W23 S16-S12
16 741 743 (S30E09 L=344) 234 54 0 ( 712/ 721- 765/ 769) 63.4 E10-E07 S32-S27
17 1084 685 (S24W14 L= 6) 644 132 1 (1010/ 657-1136/ 720) 23.2 W08-W16 S25-S20
18 1533 589 (S15W45 L= 37) 552 140 0 (1461/ 543-1594/ 629) 56.3 W41-W47 S19-S10
19 1219 575 (S26W26 L= 19) 492 111 1 (1178/ 529-1262/ 623) -12.5 W21-W30 S27-S23
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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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