AAS Meeting #194 - Chicago, Illinois, May/June 1999
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All findings are embargoed until time of presentation at the meeting.
Session 56. New Views of the Solar Interior
Solar, Display, Tuesday, June 1, 1999,
10:00am-7:00pm, Southeast Exhibit Hall
- 56.01 Solar Cycle Changes in GONG Data 1995-1998
- R. Komm, R. Howe, F. Hill (NSO)
- 56.02 Solar Internal Rotation as Measured by the SOHO SOI/MDI Full-Disk Program
- E.J. Rhodes,Jr. (USC AND JPL), J. Reiter (Tech. Univ. Munich), A.G. Kosovichev, J. Schou, P.H. Scherrer (Stanford U.)
- 56.03 How much do helioseismological inferences depend upon the assumed reference model?
- S. Basu (Inst. for Advanced Study), M.H. Pinsonneault (Ohio State U.), J.N. Bahcall (Inst. for Advanced Study)
- 56.04 A New Technique for Inversion of Helioseismic Data
- R.M. Larsen, A.G. Kosovichev, J. Schou (Stanford)
- 56.05 Three-dimensional simulations of solar oscillations: line profiles and asymmetries
- D.G. Georgobiani (Michigan State U.), R. Nigam, A.G. Kosovichev (Stanford U.), R.F. Stein (Michigan State U.), A. Nordlund (Teoretisk Astrofysik Center)
- 56.06 Subsurface Observations of Sunspots and Solar Supergranulation
- T.L. Duvall Jr. (Laboratory for Astronomy and Solar Physics, NASA/GSFC), A.G. Kosovichev, P.H. Scherrer (Hansen Experimental Physics Lab., Stanford Univ.)
- 56.07 Interaction of P-Modes with Sunspots
- T.J. Bogdan (HAO/NCAR), G.K. Barnes, P.S. Cally, A.D. Crouch (Monash University)
- 56.08 Comparison Between Near-Surface Flow Fields Deduced from Correlation Tracking and Time-Distance Helioseismology Methods
- M.L. DeRosa, J. Toomre (JILA and Department of Astrophysical and Planetary Sciences, University of Colorado), T.L. Duvall Jr. (NASA / GSFC)
- 56.09 Interpretation of Solar Activity Features Using Joint Instability of Differential Rotation and Toroidal Magnetic Fields
- P. A. Gilman, M. Dikpati (HAO/NCAR*)
- 56.10 Phase-Sensitive Holography of Acoustic Moats
- D.C. Braun (SPRC, HAO), C. Lindsey (SPRC)
- 56.11 Daily Variations and Average Structure of Solar Shear Flows Deduced from Helioseismic Dense-Pack Samplings of Ring Diagrams
- D.A. Haber, B.W. Hindman, J. Toomre (JILA, Univ. of Colorado), R.S. Bogart, J. Schou (CSSA, Stanford Univ.), F. Hill (National Solar Obs.)
- 56.12 Zonal Flows from the MDI Medium-l Data
- J. Schou (Stanford)
- 56.13 A Proposed Laboratory Experiment on Dynamo Action in a Liquid Metal Torus
- H. Ji, M. Yamada (Princeton Plasma Physics Lab., Princeton U.)
- 56.14 An Investigation into High Conductivity Dynamo Action Driven by Rotating Convection
- E. Kim (HAO, NCAR), D.W. Hughes (Dept. of Applied Maths. Univ. of Leeds), A.M. Soward (Dept. of Maths. Univ. of Exeter)
- 56.15 Axisymmetric Magnetoconvection in a Twisted Field: the effect of Compressibility
- R. Cameron (Caltech)
- 56.16 Nonlinear Compressible Dynamos
- E. E. DeLuca (Smithsonian Astrophysical Observatory), N. E. Hurlburt (Lockheed Martin)
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