Session 1. Chromosphere, Corona, Flares
Display, Friday, 7:00am-6:00pm, Ballroom B, Chair: Charles Kankelborg
- 1.74
Obtaining the 3D Structure of Coronal Magnetic Loops
from Stereo Observations
-
J. M. Davila (NASA-GSFC)
- 1.75
Preflare Event and Flare: Successive Stages of a
Single Physical Process in a System
of Intercommunicating Current Sheets
- A. I. Verneta (ZAO Comp. and Astron. Inst. MSU, Russia)
- 1.76
The relation of CaII K line features to magnetic
field intensity
- A. Nindos, H.
Zirin (Caltech, Solar Astronomy)
- 1.77
High Spectral Resolution Detectors for Solar Flare
X-Ray Studies
- U. D. Desai, L.
E. Orwig (NASA GSFC)
- 1.78
Nonlinear Magnetohydrodynamic Detonation of Solar
Flares
- O. A. Hurricane
(UCLA-Dept.
of Physics), B. H. Fong (Princeton Plasma Physics Lab), S. C. Cowley (UCLA-Dept. of Physics)
- 1.79
Non-LTE Radiative-hydrodynamic Models of Solar
Flares
- W. P. Abbett, S. L.
Hawley (Michigan State University)
- 1.80
Global Sun Study: line broadening in the extended
corona
- S. Giordano (University
of Torino, Italy), E. Antonucci (Astronomical Observatory of Torino, Italy), C. Benna (University of
Torino, Italy), J. K. Kohl (Harvard-Smithsonian Center for Astrophysics), G. Noci (University of
Firenze, Italy)
- 1.81
Evidence of untwisting magnetic fields in the Coronal
Mass Ejections of June 7,
1996
- E. Antonucci (Astronomical Observatory of Torino, Italy), S. Giordano (University of
Torino, Italy), G. Noci (University of Firenze, Italy), J. K. Kohl (Harvard-Smithsonian Center for
Astrophysics), D. Spadaro (Astronomical Observatory of Catania, Italy), C. Benna (University of Torino,
Italy)
- 1.82
Differential Emission Measures - Can we do more
??
- S. W. McIntosh, J. C. Brown
(Dept of Physics and Astronomy, University of Glasgow, Scotland, UK), P. G. Judge (High Altitude
Observatory, NCAR, Boulder, CO)
- 1.83
Studying the temporal behavior of the Evershed flow
from SOHO/MDI
- A. B.
Burnette, A. G. Kosovichev (Stanford University)
Session 2. Everything Else
Display, Friday, 7:00am-6:00pm, Ballroom C, Chair: Richard Canfield
- 2.76
P-Modes, Acoustic Emission and Surface Magnetic
Fields
- R. Jain (UMIST/JILA), D.
Haber (JILA)
- 2.77
Test for Constancy of the Solar Neutrino Flux as
Measured by the Homestake Neutrino
Experiment
- G. Walther, P. A. Sturrock, M. S. Wheatland (Stanford University)
- 2.78
Search for Periodicities in the Homestake Solar
Neutrino Data
- P. A. Sturrock, G.
Walther, M. S. Wheatland (Stanford University)
- 2.79
Evolution of the Granular Shear Flow
- A.
Nesis, R. Hammer, M. Kiefer, H.
Schleicher (Kiepenheuer-Institut Freiburg)
- 2.80
Preliminary Results Towards a Synoptic Velocity Map
of the Solar Subsurface
- I.
G. Hernandez, J. Patron (Instituto de Astrofisica de Canarias), R. S. Bogart (Stanford University), D. A.
Haber (Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder), F. Hill
(National Solar Observatory), The SOI Team (Stanford University)
- 2.81
On the direction of the rotation axis of the
Sun
- L. Gizon (Stanford), T.
Appourchaux (ESTEC)
- 2.82
Asymptotic Latitudinal Inversion of Frequency
Splitting Data
- A. C. Birch, A. G.
Kosovichev (Stanford University)
- 2.83
Persistent Convective Structures on the
Sun
- J. G. Beck (HEPL, Stanford
University), R. K. Ulrich (Dept. Physics and Astronomy, UCLA), F. Hill (NSO, NOAO), R. Bogart (HEPL,
Stanford University), L. Bertello (Dept. Physics and Astronomy, UCLA)