The Interplanetary Causes of Magnetic Storms, HILDCAAs and Viscous Interaction
A review of the Interplanetary causes of geomagnetic activity is presented.
Engineering topics
Publications and source records attributed to Tsurutani, B. T..
A review of the Interplanetary causes of geomagnetic activity is presented.
We examine possible interplanetary mechanisms for the Creation of the largest magnetic storms at the Earth.
This paper attempts to summarize the current understanding of the storm/substorm relationship by clearing up a considerabel amount of controversy and addressing the question of how solar wind energy is deposited into the constituent elements that are critical to magnetospheric and ionospheric processes.
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The process of magnetic reconnection plays an important role during the interaction of the solar wind with the Earth's magnetosphere which leads to the exchange of mass, momentum, and energy between these two highly conducting plasmas.
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We have examined the ISEE 3 distant tail data during three intense magnetic storms and have identified the tail response to high-speed solar wind streams, interplanetary magnetic clouds, and near-Earth storms.
We numerically simulate the effect of shear flow on the evolution of MHD waves in the solar corona which is modeled by a low-beta, resistive plasma slab. The hydromagnetic waves are generated in the coronal loop by applying a periodic driver which mimics foot point motion in the photosphere.
The Solar Probe Mission will be developed under the NASA Outer Planets Program using X-2000 system technology. The present design uses non-nuclear power systems, with the prime mission from 0.5 AU on the inbound pass, to a perihelion of 4Rs, to 0.5 AU on the outbound pass.
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