PROM Workshop 2007
(Prominence Research: Observations and Models)

October 29-30, Space Sciences Laboratory,
University of California, Berk
eley
List of participants
K. S. (Bala) Balasubramaniam
NSO/Sacramento Peak Obs.
Association of an Erupting Filament  and
Neighbouring Flare
(to be presented by Sara Martin)
Paul Bellan
Caltech
Why Current-Carrying Magnetic Flux  Tubes
Gobble up Plasma and Become Thin as a
Result - Model and Supporting Lab Experiments
Tom Berger
Lockheed Solar and Astrophysics Lab
New Hinode Observations of Quiescent and
Active Region Prominences
Elena Benevolenskaya
Stanford
Small-scale magnetic fields at high latitude on
the Sun, their relation to the filaments and
prominences observed in H-alpha and He II
Oddbjorn Engvold
University of Oslo
The enigmatic threads -- what can be               
inferred from current observations?  
Terry G. Forbes                                   
University of New Hampshire        
The Role of Magnetic Reconnection in
Prominence Eruptions
Holly Gilbert
Rice University        
Observational Evidence for Cross-field
Diffusion of Neutral Filament Material
Judy Karpen
NRL        
Numerical Studies of Flux Cancellation
Therese Kucera
Goddard Space Flight Center
Talking point presentation:
Questions Concerning the Disconnection and
Eruption of Filaments and CMEs
Yan Li and B. J. Lynch
Berkeley SSL
The magnetic connectivity for quiescent
filaments over neighbouring neutral lines
Ben Lynch, Y. Li, and J.G. Luhmann        
Berkeley Space Science Laboratory
Sheared-Field Prominences and the Eruptive
Implications of Magnetic Topology
Paulett Liewer                              
Jet Propulsion Laboratory, STEREO team
Prominences in 3D:  Movies from
SECCHI/EUVI
Duncan Mackay and Anthony Yeates        
University of St. Andrews
Modelling the Large Scale Corona :
Reproducing the Hemispheric Pattern of           
Filaments
Sara Martin, Helio Research              
O. Panasenco, O. Engvold and Y. Lin
A Concept of Coronal Mass Ejections
and their Origin
Sara Martin
Helio Research
Illusive Illusions in the Dynamics of Filaments
Kasia Mikurda
Prairie View Solar Observatory
Texas A&M University
Observations of the Merge of two Quiescent
Filaments
Karin Muglach
Naval Research Observatory
The Formation of Three Filament Channels and
Filaments
Joten Okamoto
National Astronomical Observatory
Hinode Science Center
Mitaka, Tokyo,  Japan     
Direct evidence of the emergence of the
helical flux rope  under an active-region
prominence
Olya Panasenco
Helio Research
Newly Recognized Cases of the  Roll Effect in
Solar Prominences
George Parks
U of C, Berkeley
Energy dissipation in collisionless plasmas        
Alex Pevtsov
NSO/Sacramento Peak Obs.
Helicity in solar prominences
Ilan Roth
U of C, Berkeley
not presenting
Nandita Srivastava        
Udaipur Solar Observatory
India
1. STEREO EUVI data and relevance of
progress on ground-based dual beam Ha
Doppler Systems   
2. Techniques for 3d reconstruction of CME
leading edge
Pat Stoker
Southern California               
Amateur Astronomer
High Resolution Solar Observations using .
Commercial Filters and Small Aperture
Telescopes
Brian Welsch
U of C, Berkeley               
Magnetogram Evolution Near Neutral Lines
Jack Zirker
free-lance writer,
former director NSO/Sacramento Peak            
 
Magnetic Models: Where are we?
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