Zank, G.P.
Zank, Gary P.
Gary P. Zank South African astrophysicist
Zank, Gary P. 1961-
VIAF ID: 44560500 (Personal)
Permalink: http://viaf.org/viaf/44560500
Preferred Forms
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100 0 _ ‡a Gary P. Zank ‡c South African astrophysicist
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200 _ | ‡a Zank ‡b Gary P.
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100 1 _ ‡a Zank, G. P.
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100 1 _ ‡a Zank, G. P.
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100 1 _ ‡a Zank, G. P.
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100 1 _ ‡a Zank, Gary P.
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100 1 _ ‡a Zank, Gary P. ‡d 1961-
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100 1 _ ‡a Zank, Gary P. ‡d 1961-
4xx's: Alternate Name Forms (5)
5xx's: Related Names (2)
Works
Title | Sources |
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6th Annual International Astrophysics Conference |
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ASTRONUM-2012 |
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Cosmic Rays in Supernova Remnants and the Galaxy |
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Coupling of the interstellar and interplanetary magnetic fields at the heliospheric interface: The effect of neutral hydrogen atoms |
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Diffusive shock acceleration and large SEP events |
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Does Turbulence Turn off at the Alfvén Critical Surface? |
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The Effects of a κ‐Distribution in the Heliosheath on the Global Heliosphere and ENA Flux at 1 AU |
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The Effects of Global Heliospheric Asymmetries on Energetic Neutral Atom Sky Maps |
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An energetic-particle-mediated termination shock observed by Voyager 2 |
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Energy cascades in a partially ionized astrophysical plasma |
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Global MHD Modeling of CMEs and Related Shocks from Complex Active Regions |
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Heliopause stability revisited: dispersion analysis and numerical simulations |
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The heliosphere in the local interstellar medium : into the unknown |
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Heliospheric Response to Different Possible Interstellar Environments |
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Heliospheric structure: the bow wave and the hydrogen wall |
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The injection problem for anomalous cosmic rays |
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Interaction between the solar wind and interstellar gas: A comparison between Monte Carlo and fluid approaches |
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The interaction of turbulence with shock waves |
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Interstellar Boundary Explorer (IBEX) |
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Interstellar Mapping and Acceleration Probe (IMAP): A New NASA Mission |
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Linear and nonlinear modes in nonrelativistic electron-positron plasmas |
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LISA-PF radiation monitor performance during the evolution of SEP events for the monitoring of test-mass charging |
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Modeling energetic neutral atoms and the IBEX spectrum |
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Numerical modeling of space plasma flows : ASTRONUM-2007 : proceedings of the 2nd International Conference held at Hotel Concorde Montparnasse, Paris, France, 10-15 June 2007 |
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Particle Acceleration at Interplanetary Shocks |
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Particle acceleration in cosmic plasmas : Newark, De., 1991 |
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Physics of the outer heliosphere |
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Physics of the Solar Wind–Local Interstellar Medium Interaction: Role of Magnetic Fields |
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The Pickup Ion-mediated Solar Wind |
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A preliminary analysis of dynamic and realistic heliosphere using interplanetary scintillation and photospheric magnetic data |
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Radial dependence of peak proton and iron ion fluxes in solar energetic particle events: application of the PATH code |
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Recent IBEX Observations and the Evolving Interstellar Interaction |
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A ROLE OF MAGNETOSONIC PULSES ON VARIATIONS OFVOYAGER-1MeV ELECTRON INTENSITY IN THE HELIOSHEATH |
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Shock geometry and spectral breaks in large SEP events |
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Sketches of Physics : The Celebration Collection |
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Small-scale magnetic islands in the solar wind and their role in particle acceleration. I. Dynamics of magnetic islands near the heliospheric current sheet |
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Solar wind 13 : Proceedings of the Thirteenth International Solar Wind Conference : 17-22 June 2012 Big Island, Hawaii |
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Stability of a pickup ion ring-beam population in the outer heliosheath: implications for the IBEX ribbon |
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Strength of the Termination Shock Inferred from the Globally Distributed Energetic Neutral Atom Flux from IBEX |
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The Structure of Comets’ Induced Magnetotails: Remote and in situ Observations |
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Structure of mass-loading shocks: 2. Comparison of theory and observation at comet Halley |
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Termination Shock Asymmetries as Seen by theVoyagerSpacecraft: The Role of the Interstellar Magnetic Field and Neutral Hydrogen |
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Theory and Transport of Nearly Incompressible Magnetohydrodynamic Turbulence. IV. Solar Coronal Turbulence |
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Trajectories and distribution of interstellar dust grains in the heliosphere |
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The transport of low-frequency turbulence in astrophysical flows. I. Governing equations |
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Transport Processes in Space Physics and Astrophysics : Problems and Solutions |
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Turbulent Transport in a Three-dimensional Solar Wind |
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Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event |
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Using the path code for modeling gradual SEP events in the inner heliosphere |
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What controls the maximum particle energy in large SEP events |
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The Wind‐ISM Interaction of α Tauri |
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