A filter method is presented which allows a qualitative and quantitative id
entification of wave modes observed with plasma experiments on satellites.
Hitherto existing mode filters are based on the MHD theory and thus they ar
e restricted to low frequencies well below the ion cyclotron frequency. The
present method is generalized to cover wave modes up to the characteristic
ion frequencies. The spectral density matrix determined by the observation
s is decomposed using the eigenvectors of the linearized Hall-MHD equations
. As the wave modes are dispersive ill this formalism, a precise determinat
ion of the k-vectors requires the use of multi-point measurements. Therefor
e the method is particularly relevant to multi-satellite missions. The meth
od is tested using simulated plasma data. The Hall-MHD filter is able to id
entify the modes excited in the model plasma and to assign the correct ener
getic contributions. By comparison with the former method it is shown that
the simple MHD filter leads to large errors if the frequency is not well be
low the ion cyclotron frequency. Further the range of validity of the linea
r theory is examined rising the simulated wave amplitudes.