SHINE 2012 Abstracts
Choose a session to view associated abstracts.
Sessions |
|
|---|---|
| Advances in Understanding the Solar Wind through Spectroscopic Observations | |
| Assessing the Contribution of Heliospheric Imaging, IPS and other remote sensing observations in Improving Space Weather Prediction | |
| Causes of the wide longitudinal signatures of Solar Energetic Particle (SEP) events | |
| Community wide validation study of models of the corona and inner heliosphere | |
| Data driven MHD modeling of CME events | |
| Dynamics of the Heliosheath and Signatures of the Heliopause - Expectations and Observations | |
| Fast reconnection in large, high-Lundquist number coronal plasmas mediated by plasmoids: Implications for reconnecting current sheets and supra-arcade downflows | |
| Interaction of CMEs with Coronal and Heliospheric Structures | |
| Multi-Wavelength/Multi-Viewpoint Coronal Observations from SDO, Hinode, STEREO and SOHO | |
| Observation Tests That Differentiate Between the Various Solar Wind Models | |
| Origin of CIR-associated suprathermal and energetic particles at 1 AU | |
| Other | |
| Sympathetic and Homologous Eruptions in the Solar Corona | |
| The compressible nature of solar wind turbulence in the inertial range and dissipation range: What, How, and Why? | |
| The need for high accuracy, high time resolution plasma and electromagnetic field measurements in the solar wind | |
| The Turbulent Solar Wind and Dissipation | |
| What do prominence and cavity activation tell us about the magnetic structure and triggering of the CME? |