By James L. Horwitz, Nagendra Singh, James L. Burch
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Published by means of the yank Geophysical Union as a part of the Geophysical Monograph Series.
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Extra resources for Cross-Scale Coupling in Space Plasmas
AndB. , 8, 1253, 1981. FluidsB, 5, 2646, 1993. mechanismandthe relationshipof the mechanisms to each other.
Other contributionsby the micro-processes, suchasviscosity, resistivity, andthermal conduction, affect the large-scale plasma modesand transport properties. This leads to small-scale-size structures. Theprocess is iteratedanda balanceis reached. 5. •N•RGIZATIOI• Fig. 2. A possiblescenario. consistent with our modelpredictions. It is alsointeresting to notethatin a particlesimulation studyof plasma-wallsheath,Theilhaberand Birdsall [ 1989]reportedtheformationof a largescalesteadystate AND CONCLUSION Our particlesimulationsof the EIH instabilityshow that largereductionof the shearparameterare achieved within 20 lower hybrid times which is lessthan 2 ion gyroperiods[RomeroandGanguli, 1993].
C. Feldman, The whistler heat flux instability: Threshold conditions in the solar wind, J. , 99, 23,391, 1994d. Gary, S. , M. F. Thomsen,L. Yin, and D. Winske, Electromagnetic proton cyclotroninstability: interactions with magnetospheric protons,J. , submitted, 1995. -D. Phan,B. U. (•. Sonnerup, and G. Res. , 20, 2255, 1993. Kennel, C. , and H. E. Petschek,Limit on stably trapped particle fluxes, J. , 71, 1, 1966. , and D. A. Gurnett, Observationsof ion cyclotronwaveswithin the plasmaphereby Hawkeye 1, J.
Cross-Scale Coupling in Space Plasmas by James L. Horwitz, Nagendra Singh, James L. Burch