Limitations on the parameters of the solar wind in modelling lunar electromagnetic induction

Details Limitations on the parameters of the solar wind in modelling lunar electromagnetic induction Limitations on the parameters of the solar wind in modelling lunar electromagnetic induction

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978geoj...52..433h&link_type=abstract

Geophysical Journal, vol. 52, no. 3, Mar. 1978, p. 433-439.

Physics

Solar Wind, Solar Wind Velocites, Models, Magnetic Fields, Moon, Conductivity

Scientific paper

A striking feature of the data on the response of the moon to periodic fluctuations in the solar wind is the large amplitude (3.65) of the transfer function at 24 mHz followed by a rolloff to a considerably lower value (3.18) at 40 mHz. By using some results of Parker (1972), it is shown that for certain parameter pairs of the solar wind speed (v) and the angle (theta) between the solar wind velocity and the magnetic field propagation direction, no lunar conductivity profiles exist that satisfy the data pair (3.65, 3.18) at the frequencies of 24 and 40 mHz, respectively. This enables some constraints to be imposed on the range of the parameter pair (v, theta).

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