A magnetic disturbance index for Mercury's magnetic field derived from MESSENGER Magnetometer data

被引:43
作者
Anderson, Brian J. [1 ]
Johnson, Catherine L. [2 ,3 ]
Korth, Haje [1 ]
机构
[1] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[2] Univ British Columbia, Dept Earth & Ocean Sci, Vancouver, BC V5Z 1M9, Canada
[3] Planetary Sci Inst, Tucson, AZ USA
来源
GEOCHEMISTRY GEOPHYSICS GEOSYSTEMS | 2013年 / 14卷 / 09期
基金
加拿大自然科学与工程研究理事会;
关键词
Mercury; magnetic field; magnetosphere; disturbance index; PLANET MERCURY; 1ST FLYBY; MAGNETOSPHERE; MISSION; DYNAMO; MAGNETOPAUSE; SATURN; CORE;
D O I
10.1002/ggge.20242
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
We present a magnetic disturbance measure for Mercury derived from MESSENGER Magnetometer data. Magnetic field fluctuations were computed in three period bands: 0.1-2 s, 2-20 s, and 20-300 s. From these, we determined log average magnetic variability versus latitude and local time in Mercury's magnetosphere. The quietest regions are the southern tail lobe and the nightside poleward of 30 degrees magnetic latitude, and the most disturbed regions are near magnetopause boundaries and the magnetospheric cusp. We used ratios at each location between the mean disturbance and that observed on each pass to compute normalized measures of magnetic disturbance for each orbit. Composite disturbance indices incorporate disturbance levels in all three bands. Percentile ranking of the composite indices provides a quantitative basis for selecting data from quiet to disturbed conditions.
引用
收藏
页码:3875 / 3886
页数:12
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