Z
Zoran Mikic
Researcher at Science Applications International Corporation
Publications - 197
Citations - 11925
Zoran Mikic is an academic researcher from Science Applications International Corporation. The author has contributed to research in topics: Solar wind & Corona. The author has an hindex of 59, co-authored 197 publications receiving 10855 citations. Previous affiliations of Zoran Mikic include University of New Hampshire.
Papers
More filters
Journal ArticleDOI
Ion Charge States in a Time-Dependent Wave-Turbulence-Driven Model of the Solar Wind
Roberto Lionello,Cooper Downs,Jon A. Linker,Zoran Mikic,John C. Raymond,Chengcai Shen,Marco Velli +6 more
TL;DR: In this paper, the authors implemented non-equilibrium ionization calculations into a 1D wave-turbulence-driven (WTD) hydrodynamic solar wind model and compared modeled charge states with the Ulysses 1994-5 in situ measurements.
Proceedings ArticleDOI
Understanding the Solar Sources of In Situ Observations
TL;DR: In this paper, the authors apply a two-step mapping technique, incorporating a magnetohydrodynamic model of the solar corona, to bring in situ observations from Ulysses, WIND, and ACE back to the solar surface in an effort to determine some intrinsic properties of the quasi-steady solar wind.
Journal ArticleDOI
Global MHD Modeling of the Solar Corona and Inner Heliosphere for the Whole Heliosphere Interval
TL;DR: In this article, a global MHD solution for Carrington rotation (CR) 2068 was developed, which includes energy transport processes, such as coronal heating, conduction of heat parallel to the magnetic field, radiative losses, and the effects of Alfven waves.
Journal ArticleDOI
Energetic particle signatures of a corotating interaction region from a high latitude coronal hole: SOHO, wind and Ulysses observations
Arik Posner,Volker Bothmer,H. Kunow,J. T. Gosling,B. Heber,B. Heber,A. J. Lazarus,Jon A. Linker,Richard G. Marsden,Zoran Mikic,Reinhold Müller-Mellin,T. R. Sanderson,Adam Szabo,Barbara J. Thompson +13 more
TL;DR: In this paper, the authors used the solar wind speeds observed at both locations to estimate the corresponding solar source longitudes of the particle events, which were related to warps of the Sun's large high latitude northern coronal hole boundaries observed by SOHO's Extreme Ultraviolet Imaging Telescope (EIT).
Understanding the Solar Sources of In Situ Observations
TL;DR: In this article, the authors apply a two-step mapping technique, incorporating a magnetohydrodynamic model of the solar corona, to bring in situ observations h m Ulysses, WIND, and ACE back to the solar surface in an effort to determine some intrinsic properties of the quasi-steady solar wind.