We illustrate a semi-automated procedure to detect the field line resonance (FLR) frequencies and the derived equatorial plasma mass densities in the inner magnetosphere from ULF measurements recorded at the European quasi-Meridional Magnetometer Array (EMMA). FLR frequencies are detected using the standard technique based on cross-phase and amplitude ratio spectra from pairs of stations latitudinally separated. Equatorial plasma mass densities are then inferred by solving the toroidal MHD wave equation using the TS05 Tsyganenko magnetic field model and assuming a 1/r dependence of the mass density along the field line. We also present a statistical analysis of the results obtained from 165 non-consecutive days of observations at 8 station ...
Coupled fast mode resonances (cFMRs) in the outer magnetosphere, between the magnetopause and a turn...
Cross-phase-derived plasma mass density trends during the Hallowe'en 2003 geomagnetic storms are pre...
The cold, core plasma mass density in the Earth's magnetosphere may be deduced from the resonant beh...
We illustrate a semi-automated procedure to detect the field line resonance (FLR) frequencies and th...
We illustrate a semi-automated procedure to detect the field line resonance (FLR) frequencies and th...
We illustrate a semi-automated procedure to detect the field line resonance (FLR) frequencies and th...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/99015/1/jgra50274.pd
It is well known that the resonant frequency of geomagnetic field lines is determined by the magneti...
AbstractIn the austral summer of 2006–2007, the 48th Japanese Antarctic Research Expedition (JARE-48...
Measurements of the eigenfrequency of geomagnetic field lines can provide information on the plasma ...
International audienceBy applying the cross-phase method and the amplitude-ratio method to magnetic ...
International audienceBy applying the cross-phase method and the amplitude-ratio method to magnetic ...
This data set contains a list of simultaneous observations of electron number density and plasma ma...
This data set contains a list of simultaneous observations of electron number density and plasma ma...
International audienceMonitoring the plasmasphere is an important task to achieve in the Space Weath...
Coupled fast mode resonances (cFMRs) in the outer magnetosphere, between the magnetopause and a turn...
Cross-phase-derived plasma mass density trends during the Hallowe'en 2003 geomagnetic storms are pre...
The cold, core plasma mass density in the Earth's magnetosphere may be deduced from the resonant beh...
We illustrate a semi-automated procedure to detect the field line resonance (FLR) frequencies and th...
We illustrate a semi-automated procedure to detect the field line resonance (FLR) frequencies and th...
We illustrate a semi-automated procedure to detect the field line resonance (FLR) frequencies and th...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/99015/1/jgra50274.pd
It is well known that the resonant frequency of geomagnetic field lines is determined by the magneti...
AbstractIn the austral summer of 2006–2007, the 48th Japanese Antarctic Research Expedition (JARE-48...
Measurements of the eigenfrequency of geomagnetic field lines can provide information on the plasma ...
International audienceBy applying the cross-phase method and the amplitude-ratio method to magnetic ...
International audienceBy applying the cross-phase method and the amplitude-ratio method to magnetic ...
This data set contains a list of simultaneous observations of electron number density and plasma ma...
This data set contains a list of simultaneous observations of electron number density and plasma ma...
International audienceMonitoring the plasmasphere is an important task to achieve in the Space Weath...
Coupled fast mode resonances (cFMRs) in the outer magnetosphere, between the magnetopause and a turn...
Cross-phase-derived plasma mass density trends during the Hallowe'en 2003 geomagnetic storms are pre...
The cold, core plasma mass density in the Earth's magnetosphere may be deduced from the resonant beh...