Andreu

Adrover

University of the Balearic Islands

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Matheus

Aguiar-Kriginsky Silva

Universitat de les Illes Balears

Magnetic field determination of chromospheric spicules using the Weak Field Approximation

Alejandro

Alvarez Laguna

Ecole Polytechnique

Consistent transport properties in multicomponent two-temperature magnetized plasmas:

Patrick

Antolin

University of St Andrews

Thermal instability-induced fundamental magnetic strands in coronal loops

Istvan

Ballai

University of Sheffield

Waves in partially ionised non-equlibrium plasma

José Luis

Ballester

Universitat illes Balears

Nonlinear evolution of Alfvén waves in a partially ionized plasma

Javier

Ballesteros

IRyA-UNAM

Formation and evolution of molecular clouds and stars

Adel

Boul'harrak Abed

University of the Balearic Islands

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Marc

Carbonell

University of the Balearic Islands

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Khatuna

Chargazia

Iv. Javakhishvili Tbilisi State University

Self-organization of the low frequency internal gravity wavy perturbations into the nonlinear vortex structures in the ionosphere plasma at interaction with local nonuniform winds

Manolo

Collados

Instituto de Astrofísica de Canarias

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antonino

del popolo

catania university

Neutron stars struture due to dark matter trapping

Turlough

Downes

Dublin City University

Energy dissipation in multi-fluid turbulence in weakly ionised plasmas

Mario

Flock

Max-Planck Institute for Astronomy

Gone with the wind: News from magnetic driven wind models of protoplanetary disks.

Holly

Gilbert

NASA/Goddard Space Flight Center

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Andrew

Hillier

University of Exeter

Attempting to identify ion-neutral drift through Dopplershifts in prominence spectral lines

Andrew

Hillier

University of Exeter

Multi-scale, nonliear dynamics of the magnetic Kelvin-Helmholtz in a partially ionised plasma

Peter

Hunana

Instituto de Astrofısica de Canarias (IAC), La Laguna, Tenerife, Spain

Fluid modeling of astrophysical plasmas - matching the fluid and collisionless kinetic descriptions

Laila Zafar

Kahlon

FC College (A Chartered University), Lahore

Zonal Flow and Magnetic Field Generation by Electromagnetic Planetary Waves in the E Ionospheric Region

Elena

Khomenko

Instituto de Astrofisica de Canarias

Generation and dissipation of Alfven waves in partially ionized solar atmosphere

Agnes

Kis-Toth

Eötvös University, Budapest, Hungary

Cosmological ionized bubbles

Vasily

Kozhevnikov

Intitute of High Current Electronics

The apokamp discharge: Experiment, theory and numerical simulations

Linh

Le Phuong

Northumbria University

A 2D two-fluid MHD code to model partially-ionised plasma: calibration and a future benchmark

James

Leake

NASA Goddard Space Flight Center

Numerical advancements in the study of solar partially ionised plasmas

Jorrit

Leenaarts

Institute for Solar Physics - Stockholm University

Non-equilibrium ionization and ion-neutral interactions in the solar chromosphere

Sergo

Lomineishvili

Astronomical Institute, Slovak Academy of Sciences

A study of Kelvin-Helmholtz instability in solar partially ionised magnetised jets

David

Martínez Gómez

Instituto de Astrofísica de Canarias

Nonlinear waves and heating in multi-fluid partially ionized solar plasmas

Juan

Martinez-Sykora

BAERI/LMSAL

Ebysus: Multi-fluid & multi-species numerical code

Mikhail

Modestov

Instituto de Astrofísica de Canarias

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Fernando

Moreno-Insertis

Instituto de Astrofísica de Canarias

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Kris

Murawski

Univesity of M. Curie-Sklodowska

Realistic numerical simulations of ion and neutral waves in a quiet region of the solar atmosphere

Giulia

Murtas

University of Exeter

Study of coalescence instability in chromospheric partially ionised plasmas

Daniel

Nóbrega-Siverio

Rosseland Centre for Solar Physics, University of Oslo

Nonequilibrium ionization and ambipolar diffusion in magnetic flux emergence processes

Ramon

Oliver

University of the Balearic Islands

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Marco

Padovani

INAF-Osservatorio Astrofisico di Arcetri - Italy

Cosmic rays: the ubiquitous probe for the interstellar medium

Robert

Pfaff

NASA/Goddard Space Flight Center

The Earth’s Ionosphere -- A Fascinating and “Accessible” Partially Ionized Plasma

Robert

Pfaff

NASA/Goddard Space Flight Center

The Earth’s Ionosphere -- A Fascinating and “Accessible” Partially Ionized Plasma

Isabell

Piantschitsch

Institute of Physics, University of Graz

A comparison between single-fluid and two-fluid numerical simulations of dynamics in the solar atmosphere

Beatrice

Popescu Braileanu

IAC

Simulations of the Rayleigh Taylor instability in the two fluid approximation

Dr.Pramod

Purohit

National Institute of Technical Teacher’s Training and Research, Bhopal- 462002 M.P., India

Variability of Geomagnetic Field with Interplanetary Magnetic Field at High Latitudes

Anish

Roshi

Arecibo Observatory and University of Central Florida

Exploring Partially Ionized Plasma in the Galactic Interstellar Medium using Carbon Recombination Lines

Michael

Ruderman

The University of Sheffield

Rayleigh-Taylor instabilities with sheared magnetic fields in partially ionised plasmas

Takahito

Sakaue

Kyoto University

Partially ionization effect in the chromosphere of cool main-sequence stars

Shilpa

Sarkar

Aryabhatta Research Institute of Observational Sciences, Nainital, India

Two-temperature advective transonic accretion flows around black holes

Ildar

Shaikhislamov

Institute of Laser Physics SB RAS

Partially ionized plasma of hot exoplanets: a medium for detection of properties of upper atmospheres and stellar winds

Ben

Snow

University of Exeter

Shock substructure in partially-ionised plasma.

Roberto

Soler

Universitat de les Illes Balears

Energy transport by torsional Alfven waves through the partially ionized chromosphere

Rosie

Sumpter

University of Leeds

Sputtering and grain-grain collisions in weakly-ionised plasmas using grain-size distribution functions

Jaume

Terradas

Universitat de les Illes Balears

Prominence threads and oscillations under the presence of partial ionizacion, thermal conduction, radiation and heating

Jeff

Thayer

University of Colorado

Earth’s Interaction Region: Plasma-Neutral Interactions in the Strongly Neutral Plasma of Earth’s High Latitude Upper Atmosphere

Eberhard

Wiehr

Inst. Astrophys. Uni-Goettingen

Velocity and line-width excess of emission lines from ions over such from nuetrals

Teimuraz

Zaqarashvili

Ilia State University, Tbilisi, Georgia

Rapid heating of type II spicules in PIP of the solar atmosphere

Lingling

Zhao

CSPAR, UAH

Interstellar pickup ions transport in the turbulent solar wind