SHINE Survey 2018
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Please indicate your primary working group affiliation.
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Overall rating of the 2018 SHINE Workshop.
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Please rate the following meeting characteristics:
Poor
Below Average
Satisfactory
Good
Fantastic
Banquet
Web Site/ Meeting Updates/ Email Contact
Network Connectivity
Poster Session
Conference Facilities
Registration Process
Registration Packet Materials
Location
Agency Reports (NSF)
Free Afternoon
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Please provide information to support your responses. This will help us understand what worked and what did not.
Please rate the sessions.
Extremely Valuable
Very Useful
Useful
Not Enough Discussion
Did Not Attend
What's Next for Solar & Heliospheric Physics?
Observational Signatures of Star-Planet Interactions (SPI)
Instabilities and Their Role in Modifying Turbulence Dynamics
Signatures of Time-dependent Heating in Active Regions and the Slow Solar Wind
Modern observation and simulation of the physics of kinetic cascade leading to production of internal energy: MMS and beyond
Revealing the Physics of the Inner Heliosphere
Connecting Slow Solar Wind Theories to Current and Future Observations(Year II)
Global implications of kinetic-scale particle acceleration throughout the heliosphere
Using PSP to Probe Magnetic Reconnection at the Sun
How does the solar atmosphere connect to the inner heliosphere?
Understanding the Magnetic Configuration of CMEs
Advances and Challenges in Data-Constrained Modeling of Solar Eruptions
Galactic cosmic ray transport in the heliosphere
Suprathermal ions and electrons in interplanetary space: Properties and Roles
Predicting solar energetic particles: community campaign
Is Understanding Magnetic Field Connectivity Crucial for Understanding Solar Energetic Particle (SEP) Events?
The return of CMEs - What are we assuming, what do we know, and how can we move forward?
Role of turbulence in dynamics of SEPs
Coupled heliospheric and solar energetic particle models
Are SEP Spectral Breaks due to Acceleration near the Sun or Transport in Interplanetary Space?
Observations and interpretations of coronal shock waves
Advancing Solar Activity Forecasts Through Observations, Data Assimilation and Machine Learning
Really, What is Turbulent Dissipation?
Ion and Electron Distributions in the Solar Wind: Kinetic Physics
How do small-scale effects feedback on reconnection global dynamics, and vice versa?
Insights into CMEs and Their Substructure(s)
Testing the Standard Model of solar eruptive events: the X8 limb flare of 10 September 2017
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Which SHINE 2018 working group session did you attend that was the most beneficial and why? (e.g. overall topic, discussion, scene setters, organization, scientific focus)?
What new session topic(s) would you most like to see discussed next year?
Would you be willing to organize/lead a session on one of those topics?
You can contact Georgia de Nolfo at georgia.a.denolfo@nasa.gov for more informationabout session-proposal guidelines. These guidelines will also be distributed to SHINE participants via email later this Fall.)
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How did you find the balance between talks and discussion?
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SHINE has been growing in the past with ≥200 participants since 2018.  In your opinion, what should be done:
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Did you find there was adequate time for the poster sessions? Please answer Yes, No, or write a comment.
Please rate the following hotel facilities: (1 = Poor, 3 = Satisfactory, 5 = Excellent)
1
2
3
4
5
Bedrooms
Meals
Meeting facilites
Hotel Services / Staff
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Additional Comments:
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