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Jozsef Kota
Researcher/Scientist IV
Lunar and Planetary Laboratory
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Overview
Research
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Collaboration
(2)
Joe Giacalone
Mutual work: 37 Proposalsīš8 Grantsīš1 Supervisor
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Walter Harris
Mutual work: 1 Proposal
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Grants
(11)
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Publications
(27)
Recent
Magnetic Trapping of Galactic Cosmic Rays in the Outer Heliosheath and Their Preferential Entry into the Heliosphere
2024
cosmic rays,
heliosphere,
galactic
On the Energy Dependence of Galactic Cosmic Ray Anisotropies in the Very Local Interstellar Medium
2022
cosmic rays,
galactic,
interstellar medium,
energy dependence,
anisotropies
No Stagnation Region before the Heliopause at Voyager 1? Inferences from New Voyager 2 Results
2021
heliopause,
voyager mission,
interstellar medium,
space exploration,
solar wind
Hybrid Simulations of Interstellar PickuProtons Accelerated at the Solar-wind Termination Shock at Multiple Locations
2021
interstellar pickups,
solar-wind termination shock,
hybrid simulations,
proton acceleration,
multiple locations
Transient Cosmic-ray Events beyond the Heliopause: Interpreting Voyager-1 Observations
2017
cosmic-ray events,
voyager-1 observations,
heliopause,
transient events,
interpreting observations
The Role of Particle Drifts in the Heliosphere
2016
solar wind,
plasma physics,
space weather,
interstellar medium,
cosmic rays
Erratum: Erratum to: The spatial density gradient of galactic cosmic rays and its solar cycle variation observed with the Global Muon Detector Network
2016
cosmic rays,
solar cycle,
density gradient,
galactic,
muon detector
{Particle Acceleration at Low Coronal Compression Regions and Shocks}
2015
particle acceleration,
coronal compression,
shocks,
low coronal,
acceleration regions
{Broken Power-law Distributions from Low Coronal Compression Regions or Shocks}
2015
astrophysics,
solar physics,
plasma physics,
statistical analysis,
geophysics
{Effects of Large-Scale Simple Velocity Shear on a Fluctuating Interplanetary Magnetic Field}
2015
fluctuating magnetic field,
interplanetary,
velocity shear,
large-scale effects,
research
