Zank, G.P.
Zank, Gary P.
Gary P. Zank
Zank, Gary P. 1961-
VIAF ID: 44560500 (Personal)
Permalink: http://viaf.org/viaf/44560500
Preferred Forms
- 100 0 _ ‡a Gary P. Zank
- 200 _ | ‡a Zank ‡b Gary P.
- 100 1 _ ‡a Zank, G. P.
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- 100 1 _ ‡a Zank, G. P.
- 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-
4xx's: Alternate Name Forms (7)
5xx's: Related Names (2)
Works
Title | Sources |
---|---|
6th Annual International Astrophysics Conference | |
ASTRONUM-2012 | |
Cosmic Rays in Supernova Remnants and the Galaxy | |
Coupling of the interstellar and interplanetary magnetic fields at the heliospheric interface: The effect of neutral hydrogen atoms | |
Diffusive shock acceleration and large SEP events | |
Does Turbulence Turn off at the Alfvén Critical Surface? | |
The Effects of a κ‐Distribution in the Heliosheath on the Global Heliosphere and ENA Flux at 1 AU | |
The Effects of Global Heliospheric Asymmetries on Energetic Neutral Atom Sky Maps | |
An energetic-particle-mediated termination shock observed by Voyager 2 | |
Energy cascades in a partially ionized astrophysical plasma | |
Global MHD Modeling of CMEs and Related Shocks from Complex Active Regions | |
Heliopause stability revisited: dispersion analysis and numerical simulations | |
The heliosphere in the local interstellar medium : into the unknown | |
Heliospheric Response to Different Possible Interstellar Environments | |
Heliospheric structure: the bow wave and the hydrogen wall | |
The injection problem for anomalous cosmic rays | |
Interaction between the solar wind and interstellar gas: A comparison between Monte Carlo and fluid approaches | |
The interaction of turbulence with shock waves | |
Interstellar Boundary Explorer (IBEX) | |
Interstellar Mapping and Acceleration Probe (IMAP): A New NASA Mission | |
Investigating Geocoronal Absorption for Wavelength Calibration of Sounding Rockets | |
Linear and nonlinear modes in nonrelativistic electron-positron plasmas | |
LISA-PF radiation monitor performance during the evolution of SEP events for the monitoring of test-mass charging | |
Modeling energetic neutral atoms and the IBEX spectrum | |
Modeling Particle Acceleration at Interplanetary Shocks | |
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 | |
Observation of a Magnetic Switchback in the Solar Corona | |
Particle acceleration and transport at an oblique CME-driven shock | |
Particle acceleration in cosmic plasmas : Newark, De., 1991 | |
Physics of the outer heliosphere | |
Physics of the Solar Wind–Local Interstellar Medium Interaction: Role of Magnetic Fields | |
The Pickup Ion-mediated Solar Wind | |
A preliminary analysis of dynamic and realistic heliosphere using interplanetary scintillation and photospheric magnetic data | |
Radial dependence of peak proton and iron ion fluxes in solar energetic particle events: application of the PATH code | |
Recent IBEX Observations and the Evolving Interstellar Interaction | |
A role of magnetosonic pulses on variations of Voyager-1 MeV electron intensity in the heliosheath | |
Shock geometry and spectral breaks in large SEP events | |
Sketches of Physics : The Celebration Collection | |
Small-scale magnetic islands in the solar wind and their role in particle acceleration. I. Dynamics of magnetic islands near the heliospheric current sheet | |
Solar wind 13 : Proceedings of the Thirteenth International Solar Wind Conference : 17-22 June 2012 Big Island, Hawaii | |
STABILITY OF A PICKUP ION RING-BEAM POPULATION IN THE OUTER HELIOSHEATH: IMPLICATIONS FOR THEIBEXRIBBON | |
Strength of the Termination Shock Inferred from the Globally Distributed Energetic Neutral Atom Flux from IBEX | |
The Structure of Comets’ Induced Magnetotails: Remote and in situ Observations | |
Structure of mass-loading shocks: 2. Comparison of theory and observation at comet Halley | |
Termination Shock Asymmetries as Seen by theVoyagerSpacecraft: The Role of the Interstellar Magnetic Field and Neutral Hydrogen | |
Theory and Transport of Nearly Incompressible Magnetohydrodynamic Turbulence. IV. Solar Coronal Turbulence | |
Trajectories and distribution of interstellar dust grains in the heliosphere | |
The transport of low-frequency turbulence in astrophysical flows. I. Governing equations | |
Transport processes in space physics and astrophysics | |
Turbulent Transport in a Three-dimensional Solar Wind | |
Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event | |
Using the path code for modeling gradual SEP events in the inner heliosphere | |
What controls the maximum particle energy in large SEP events | |
The Wind‐ISM Interaction of α Tauri |