Presentations

The 2007 SHINE Workshop Presentations from Whistler

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Agency Talks
Paul Bellaire SHINE and the NSF's Solar Terrestrial Research (STR) Program    
Student Tutorials
Andrew Jordan A Quick Journey Through the Heliosphere    
Carla Jacobs Modelling of the solar corona and the solar wind  
Christina Prested Voyager 1's Dec. 2004 Termination Shock Crossing and Energetic Neutral Atoms    
Eileen Chollet Energetic Particles: Populations, Transport and Acceleration  
Gemma Attrill CMEs & ICMEs Observations and Theories    
Student Research Talks
Errol Summerlin Applying Field Line Wandering (FLW) to a Monte-Carlo Simulation    
Eve Stenson Flows and interactions in laboratory coronal loops    
Christina O. Lee Comparison of the 3D MHD Solar Wind Model Results with ACE Data    
Lan Jian Radial Evolution of Major Solar Wind Structures    
Laurel Rachmeler CME initiation without reconnection    
Nicholeen Viall, Larry Kekpo, and Harlan Spence Inherent Length Scales and Apparent Frequencies of Periodic Solar Wind Number Density Structures    
WG 1: The Magnetic and Energetic Connection Between the Solar Photosphere and Corona
Leaders: Bill Abbett and K. D. Leka
Post-Session Summary
Bill Abbett The Magnetic and Energetic Connection Between the Solar Photosphere and Corona    
Talks
Alex Pevtsov Understanding the Connection Between the Solar Interior and Corona: Progress and Challenges    
Alex Pevtsov Knots and Bolts of Solar Helicity    
Marc DeRosa Preliminary Results from Nonlinear Field Extrapolations using Hinode Boundary Data    
Marc Cheung Magnetic Flux Emergence In Granular Convection    
Manolis Georgoulis Magnetic Helicity and Energetics in Solar Active Regions: Can we calculate them - why do we need them?    
WG 2: Active Region Flux
Leaders: Holly Gilbert and Nick Arge
Post-Session Summary
Holly Gilbert Active Region Flux   
Talks
Jack Harvey What is the Evidence for Open Field Lines from Active Regions?    
Roberto Lionello, Jon A. Linker, Zoran Mikic, Pete Riley MHD Evolution of Bipolar Active Regions through Differential Rotation  
Marcia Neugebauer The Quasi-Stationary Solar Wind from Active Region Sources    
WG 3: Filament Dynamics
Leaders: Holly Gilbert and Nick Arge
Post-Session Summary
Holly Gilbert Filament Dynamics    
Talks
Berhnard Kliem Numerical Modeling of Filament Eruptions  
T. A. Kucera and E. Landi Multi-wavelength Observations of Low Level Heating in an Erupting Prominence    
Rui Liu, H. R. Gilbert, D. Alexander, and Y. Su A Partial Filament Eruption Driven by Kink Instability    
WG 4: The Heliospheric Plasma Sheet
Leaders: Ian Richardson and Angelos Vourlidas
Talks
Nancy Crooker The Heliospheric Plasma Sheet: Definition, Dynamics, Solar Connections    
WG 5: Magnetic Data Inputs to Global Models
Leaders: Ilia Roussev, Nick Arge, and K. D. Leka
Post-Session Summary
Ilia Roussev WG2 Session: Magnetic Data Input into Global Models    
Talks
George Fisher The Use of Vector Magnetogram Data in MHD Models of the Solar Atmosphere and Prospects for an Assimilative Model    
G.J.D. Petrie GONG Magnetograms and Coronal Field Modeling    
K.D. Leka Promises and Reality of Analysis using Vector Magnetic Field Data  
Peter MacNeice GONG Magnetograms Impact on CCMC Modeling    
Marc DeRosa Pros and Cons of Various Magnetic Field Extrapolation Techniques    
WG 6: Origin of Structure in the Solar Wind
Leaders: Joe Borovsky and Nick Arge
Post-Session Summary
Joe Borovsky Session 10: Origin of Structure in the Solar Wind    
Talks
Nick Arge Using the WSA Model to Connect the Solar Wind Observed Near Earth with its Sources Back at Sun    
L. A. Fisk Comments on Reconnection at the Sun    
L. K. Jian What Mirror Mode Waves in the Solar Wind Are Telling Us about the Corona Heating Region    
Gang Li Flux tubes in solar wind from Ulysses observations    
Harlan Spence and Justin C. Kasper Time-Dependence (structuring) of the Alpha-to-Proton Ratio (AHe) in the Solar Wind at 1 AU: Initial results, Implications, and Speculations    
Nicholeen Viall Inherent Length Scales and Apparent Frequencies of Periodic Solar Wind Number Density Structures  
WG 7: Is the Ubiquitous Suprathermal Seed Population Generated in the Corona or Interplanetary Medium?
Leaders: Matthew E. Hill and Dennis K. Haggerty
Post-Session Summary
Matthew Hill Working Group 17: Suprathermal Ions    
Talks
Richard A. Mewaldt Quiet-Time Spectra and Composition from Suprathermal to MeV Energies 1998-2007  
Matthew E. Hill, Douglas C. Hamilton, Craig Stutts, and Robert DeFabio Quiet & Active Time Composition of Suprathermal Ions Inside of 9 AU  
George Gloeckler and Len Fisk The Ubiquitous, Invariant, Quiet-time -5 Power Law Tails  
J. L. Kohl Progress Toward Measurements of Suprathermal Tails in Coronal Proton Velocity Distributions  
Nathan Schwadron and M. Desai, M. Hill, A. Posner On the Sources and Evolution of Suprathermal Ions  
Posters
J. R. Gruesbeck, S. T. Lepri, and T. H. Zurbuchen Analysis of Suprathermal Tails Over Varying Time Scales: Preliminary Results  
C. Prested, N. Schwadron, J. Passuite, B. Randol, B. Stuart, G. Siscoe, J. Herrikhuisen, N. Pogorelov, M. Opher, and B. Lavraud Observational Evidence of universal kappa distributions and the implications for the Interstellar Boundary Explorer  
David S. Smith and Joe Giacalone Hybrid Code Simulations of Pickup Ion Acceleration and Transport  
WG 8: Turbulence and Coronal Heating
Leaders: Ben Chandran and Joe Giacalone
Post-Session Summary
Ben Chandran Mechanisms for Heating the Corona and Launching the Solar Wind  
Talks
W. H. Matthaeus Coronal heating by low frequency wave- driven quasi-2D MHD turbulence cascade    
Randy Jokipii Do Shock Waves Heat the Solar Corona?  
Marco Velli Alfven Waves and MHD Turbulence in Coronal Heating and Solar Wind  
Greg Howes Particle Heating through the Dissipation of Magnetized Turbulence: Theory, Simulations, and Implications for Coronal Heating  
Vahe Petrosian Non-thermal Signatures in the Solar Corona: Heating and Acceleration by Turbulence    
Vahe Petrosian Turbulence Cascade and Damping beyond MHD and Inertial Range    
J. F. Drake On the filamentary structure of energetic electrons during flares    
Ben Chandran Turbulence and the Origin of Solar Wind  
WG 9: Shock geometry and particle injection at Shocks and upstream/downstream phenomena
Leaders: Gang Li and Matt Hill
Post-Session Summary
Gang Li Shock geometry & upstream and downstream phenomena    
Talks
WG 10: Interpreting Radio Measurements
Leaders: Justin Kasper and Holly Gilbert
Talks
WG 11: Is the open flux in the heliosphere conserved?
Leaders: Matt Owens and Dennis Haggerty
Post-Session Summary
Matt Owens The open flux of the Sun (PowerPoint)    
Matt Owens The open flux of the Sun (Document)    
Talks
Pete Riley Understanding the relationship between photospheric field observations and in-situ observations of the interplanetary magnetic field  
S. T. Lepri Comparison of Heliospheric Magnetic Flux from Observations and the SAIC MHD Model    
Nick Arge Comparing the Observed and Modeled Global Heliospheric Magnetic Flux    
Leif Svalgaard The Open Flux Has Been Constant Since ~1840  
Posters
WG 12: CME Dynamics: eruption, acceleration, energetics
Leaders: Angelos Vourlidas and Ilia Roussev
Post-Session Summary
Angelos Vourlidas CME Accelerations: So What? Who Cares?    
Talks
Jie Zhang CME Accelerations: What Observations Tell Us So Far?    
Noe Lugaz, Ilia Roussev, Huw Morgan, and Igor Sokolov CME Accelerations: What Observations Tell Us So Far?    
Geoff Reeves Acceleration vs Poynting flux    
Jiong Qiu Energy partition during the initial stages of the CME.    
C. St.Cyr CME accelerations in the low corona.    
Berhnard Kliem Models of erupting filaments and their acceleration profile.  
WG 13: The "Tell-Tale Topology" for CME Initiation
Leaders: K. D. Leka and Holly Gilbert
Post-Session Summary
K. D. Leka Tell-Tale Topology of CME initiation  
Talks
Ward Manchester Shear Flows Driven by the Lorentz Force During Flux Emergence: An Initiation Mechanism for CMEs and Flares    
David Alexander CME initiation: the Matrix Reloaded    
Holly Gilbert Kinking in observations    
Brian Welsch The Formation of Eruptive Structures in the Solar Corona    
Graham Barnes On The Relationship Between Coronal Magnetic Null Points and CMEs  
Ron Moore The Central Role of Tether-Cutting Reconnection in the Production of CMEs    
Alysha Reinard CME-associated dimming regions    
Laurel Rachmeler CME Initiation Without Reconnection    
B. J. Lynch, S. K. Antiochos, C. R. DeVore, J. G. Luhmann The Breakout Model for Coronal Mass Ejections and its "Generally Infallible Robustness?" in 3D    
WG 14: Shocks in the Corona
Leaders: Angelos Vourlidas and Ilia Roussev
Post-Session Summary
Angelos Vourlidas EUV Waves: So What? Who Cares?    
Talks
Marco Velli Deconstructing EIT Waves    
Jon Linker MHD modeling of Coronal Waves  
Elena Podladchikova What can we learn from the EIT wave observations?    
Gemma Attrill Coronal "Wave": Magnetic Footprint of a Large-Scale CME?    
WG 15: CME-ICME Connections
Leaders: Zoran Mikic
Post-Session Summary
Zoran Mikic Session 11: CME-ICME Connections  
Talks
Zoran Mikic CME-ICME Connections  
Manolis Georgoulis Nonlinear force-free calculation of magnetic energy and helicity in solar active regions - Method and Preliminary Results    
Rick DeVore Homologous Coronal Mass Ejections via Magnetic Breakout  
Craig DeForest Fluxon Modeling of Active Region Evolution  
Bernie Jackson Interplanetary Scintillation (IPS) Analysis of the 13-15 May 2005 Earth-Directed CME  
Curt A. de Koning, V.J. Pizzo, D.A. Biesecker CME Velocity Determined by Geometric Localization  
Gemma Attrill Dimming analysis 12/05/05    
WG 16: CME and SEP modeling of the April 21, 2002 SEP event
Leaders: Mihir Desai and Gang Li
Talks
WG 17: Community Modeling
Leaders: Jon Linker
Talks
Jon Linker Community Models: What Should The Future Be?    
Tamas Gombosi CSEM Experience with Community Modeling    
Stan Solomon Community Modeling in the Atmospheric Sciences    
Janet Luhmann Community Modeling: What Users Could Use    
J. Todd Hoeksema Useful Community Modeling Capabilities - One Perspective    
Posters
Phillip Traver, Pete Riley, Zoran Mikic, and Jon Linker Integrating Global MHD Models with STEREO Observations  
WG 18: Electron-rich and/or He3-rich impulsive events
Leaders: Dennis Haggerty and Gang Li
Post-Session Summary
Dennis Haggerty He3 and/or electron SHINE 2007 rich events    
Talks
Glenn Mason Recent Progress in Understanding 3He-rich SEP Events  
Vahe Petrosian Stochastic Acceleration in Solar Flares: Enrichments and Distributions  
Ilan Roth Solar Electrons - Clue to Coronal Magnetic Reconfiguration and Impulsive (Rare) Ion Energization (Some old inquiries and few new questions)  
L. Wang The timing between impulsive electrons and type III radio bursts and 3He-rich ions  
Posters
H. V. Cane, I. G. Richardson, and T. T. Von Rosenvinge The Solar Energetic Particle Event Zoo  
Dennis K. Haggerty and Edmond C. Roelof New Results for Interplanetary Type III Solar Radio Bursts Associated with Near-Relativistic Beam-Like Solar Electron Events  
Linghua Wang, Robert P. Lin, Sam Krucker, and Gang Li A Study of Pitch Angle Distributions for Solar Impulsive Electron Events  
Linghua Wang, Robert P. Lin, Sam Krucker, Gang Li, and Glenn Mason The timing between impulsive electrons and type III radio bursts and 3He-rich ions  
Linghua Wang, Robert P. Lin, Sam Krucker, and Glenn Mason A Statistical Study of Solar Energetic Electron Events over One Solar Cycle  
WG 19: Successfully modeling the May 12th, 1997 event from its eruption to its interplanetary propagation out past Earth: Are we there yet?
Leaders: Nick Arge
Talks
WG 20: Special Session on the 2005 January 20 Event
Leaders: Allan Tylka and John Raymond
Post-Session Summary
Allan Tylka Special Session on the 2005 January 20 Event    
Talks
Gerald Share, Ronald Murphy, David Smith, Gordon Hurford, Albert Shih, and Robert Lin RHESSI Observations of the 2005 January 20 Solar Flare  
Mewaldt, Cohen, Labrador, Leske, Mason, Haggerty, Looper, Mazur, Selesnick, Desai Solar Particle Energy Spectra and Composition in the January 20, 2005 Event  
B. Jackson 20 January 2005 Shock Observed by SMEI   
Victor Grechnev, V.Kurt, I.Chertok, A.Uralov, H.Nakajima, A.Altyntsev, A.Belov, B.Yushkov, S.Kuznetsov, L.Kashapova, N.Meshalkina, N.Prestage The Extreme Solar Event of 20 January 2005: Properties of the Flare and Origination of Energetic Particles    
Claire Foullon, C.J.Owen, S.Dasso, L.M.Green, I.Dandouras, H.A.Elliott, A.N.Fazakerley, Y.V.Bogdanova, N.U.Crooker Multi-spacecraft study of the 21 January 2005 ICME    
Cara Rakowski, M.Laming, S.Lepri Ion Charge States in Halo CMEs: 2003/10/29 and 2005/01/20