tudies of the Earth's magnetic field reveal that its strength at its surface along its e s approximately 25 µT while its strength at its poles is 65 µT. ) Assuming the Earth's magnetic field can be modeled as a dipole, compute the stren nagnetic field at a radius of 3 Earth radii above the equatorial surface (corresponding t adii from its center). ) At this radius, compute the mirror ratio RM, the half-opening angle ao in degrees an robability P. Wiu di: fuonm th uth'
tudies of the Earth's magnetic field reveal that its strength at its surface along its e s approximately 25 µT while its strength at its poles is 65 µT. ) Assuming the Earth's magnetic field can be modeled as a dipole, compute the stren nagnetic field at a radius of 3 Earth radii above the equatorial surface (corresponding t adii from its center). ) At this radius, compute the mirror ratio RM, the half-opening angle ao in degrees an robability P. Wiu di: fuonm th uth'
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