Cusp-latitude Pc3 spectra: band-limited and power-law components
Cusp-latitude Pc3 spectra: band-limited and power-law components
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尖点纬度 Pc3 谱:带限和幂律分量
DOI:
10.5194/angeo-20-1539-2002
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发表时间:
2002
影响因子:
1.9
通讯作者:
R. Morris
中科院分区:
文献类型:
--
作者:
P. Ponomarenko;B. J. Fraser;F. Menk;S. Ables;R. Morris
This work attempts to fill a gap in compara- tive studies of upstream-generated Pc3-4 waves and broad band ULF noise observed at cusp latitudes. We performed a statistical analysis of the spectral properties of three years of cusp-latitude ground magnetometer data, finding that the average daytime Pc3-4 spectra are characterized by two principal components: an upstream-related band-limited en- hancement ('signal') and a power-law background ('noise') with S(f) / f 4 . Based on this information we devel- oped an algorithm allowing for the deconvolution of these two components in the spectral domain. The frequency of the signal enhancement increases linearly with IMF mag- nitude as f (mHz) ' 4.4|BIMF|(nT), and its power maxi- mizes around IMF cone angles xB ' 20 and 160 and at 10:30-11:00 MLT. Both spectral components exhibit similar semiannual variations with equinoctial maxima. The back- groundnoise power grows with increasing southwardBz and remains nearly constant for northward Bz. Its diurnal varia- tion resembles that of Pc5 field-line resonance power, with a maximum near 09:00 MLT. Both the band-limited signal and broad band noise components show power-law growth with solar wind velocity / V 5.71 sw and / V 4.12 sw , respectively. Thus, the effective signal-to-noise ratio increases with in- creasing Vsw. The observations suggest that the noise gen- eration is associated with reconnection processes.