COSPAR 2024, July 13-21, Busan, South Korea: Abstract Submission & Registration Open

Annonce transmise par Nicole Vilmer (LESIA)

COSPAR 2024 will be held on July 13-21, 2024 in South Korea in the seaside metropolis of Busan. The deadline for submitting an abstract is : February 9, 2004.

All the information can be found at https://www.cospar2024.org/ and at https://www.cospar-assembly.org/assembly.php

Here is a list of sessions with topics related to PNST:

D1.1: Acceleration and Transport of Energetic Particles in the Heliosphere, the Interstellar Medium, and Astrospheres
D1.2  Large Scale Structure of Heliosphere and its Physical Drivers
D1.3: Magneto-plasma Structures, Streams and Flows in the Heliosphere
D1.4: Suprathermal and Pickup Ions Throughout the Heliosphere
D1.5: Turbulence in the Heliosphere from the Solar Corona to the Very Local Interstellar Medium
D1.6: Understanding and Predicting Solar Energetic Particle Events Across the Heliosphere
D1.7: Science from Neutron Monitors, Muon Telescopes, and other Detectors of Atmospheric Showers from GeV Cosmic Rays
D2.1: Off-the-Sun-Earth-Line(OSEL) Missions
D2.2: Heliospheric Variability, its Solar Sources and Impacts on Solar System Objects
D2.3: Magnetic Reconnection in the Turbulent Plasmas – From the Sun through the Heliosphere to Stars and Galaxies
D2.4: STEREO's Journey around the Sun: An Era of Single and Multi-spacecraft Observations from 2007 to 2024
D2.5: Impact of the Inhomogeneous Solar Corona and Solar wind on CME Evolution
D3.1  Highlights of Magnetospheric Plasma Physics
D3.2   Cross-scale Coupling and Multi-point Observations in the Solar Wind and Magnetosphere
D3.3    Origin of Non-thermal Distributions in Space Plasmas and their Role in Wave Generation and Heating / Acceleration of Particles
D3.4    Particle Transport Acceleration and Loss in the Earth and Planetary Magnetospheres
D3.5    Role of Mesoscale Coupling as the Driver of System Level Storm and Substorm Dynamics in Geospace
D3.6    CubeSat and Small Satellite Technology Addressing Magnetospheric Challenges
D3.7    Machine Learning and Data Sciences
D3.8    Dayside Magnetosphere Interactions
D4.1    Dust Observations in Space and Laboratory Experiments
E2.1: Energetics and dynamics in the quiet solar atmosphere and beyond
E2.2: Energy and mass transport of small scales in the low solar atmosphere
E2.3: Plasma and Magnetic Field Coupling in Solar Prominences
E2.4: Application of Machine Learning Techniques in Solar and Heliospheric Physics
E2.5: Waves in the Solar Atmosphere, from the Photosphere to the Corona and Solar Wind
E2.6: Developments and Applications of the Solar Magnetic Field Modelling
E2.7: Waves and Flows in Solar Coronal Active Regions, from Heating to Coronal Seismology
E3.1: Off-the-Sun-Earth-Line(OSEL) Missions
E3.2: Heliospheric Variability, its Solar Sources and Impacts on Solar System Objects
E3.3: Magnetic Reconnection in the Turbulent Plasmas – From the Sun through the Heliosphere to Stars and Galaxies
E34: STEREO's Journey around the Sun: An Era of Single and Multi-spacecraft Observations from 2007 to 2024
E3.5: Impact of the Inhomogeneous Solar Corona and Solar wind on CME Evolution