Search Publications

Time-Distance Inversion Methods and Results - (Invited Review)
DOI: 10.1023/A:1005251208431 Bibcode: 2000SoPh..192..159K

Kosovichev, A. G.; Scherrer, P. H.; Duvall, T. L. _Jr., Jr.

The current interpretations of the travel-time measurements in quiet and active regions on the Sun are discussed. These interpretations are based on various approximations to the 3-D wave equation such as the Fermat principle for acoustic rays and the Born approximation. The ray approximation and its modifications have provided the first view of t…

2000 Solar Physics
SOHO 259
A comparison of differential rotation measurements - (Invited Review)
DOI: 10.1023/A:1005226402796 Bibcode: 2000SoPh..191...47B

Beck, John G.

Observers have long measured solar rotation with different techniques and obtained different results. This paper compares differential rotation measurements from four techniques: Doppler shift, Doppler feature tracking, magnetic feature tracking, and p-mode splittings. The different rotation rates measured by the first three techniques are interpr…

2000 Solar Physics
SOHO 198
Basic Principles of Solar Acoustic Holography - (Invited Review)
DOI: 10.1023/A:1005227200911 Bibcode: 2000SoPh..192..261L

Braun, D. C.; Lindsey, C.

We summarize the basic principles of holographic seismic imaging of the solar interior, drawing on familiar principles in optics and parallels with standard optical holography. Computational seismic holography is accomplished by the phase-coherent wave-mechanical reconstruction of the p-mode acoustic field into the solar interior based on heliosei…

2000 Solar Physics
SOHO 171
Time-Distance Helioseismology with f Modes as a Method for Measurement of Near-Surface Flows
DOI: 10.1023/A:1005239503637 Bibcode: 2000SoPh..192..177D

Duvall, T. L., Jr.; Gizon, L.

Travel times measured for the f mode have been used to study flows near the solar surface in conjunction with simultaneous measurements of the magnetic field. Previous flow measurements of Doppler surface rotation, small magnetic feature rotation, supergranular pattern rotation, and surface meridional circulation have been confirmed. In addition, …

2000 Solar Physics
SOHO 137
Supra-arcade Downflows in Long-Duration Solar Flare Events
DOI: 10.1023/A:1005220604894 Bibcode: 2000SoPh..195..381M

McKenzie, D. E.

This report seeks to introduce the reader to a set of observations made during the decay phase of long-duration event (LDE) flares on the Sun. In a number of events, the soft X-ray images from Yohkoh SXT indicate a downward-directed flow field in the region immediately above the flare arcade. The prototypical event is the M5 flare of 20 January 19…

2000 Solar Physics
SOHO 134
The Photospheric Convection Spectrum
DOI: 10.1023/A:1005200809766 Bibcode: 2000SoPh..193..299H

Raymond, J.; Hathaway, D. H.; Bogart, R. S. +5 more

Spectra of the cellular photospheric flows are determined from observations acquired by the MDI instrument on the SOHO spacecraft. Spherical harmonic spectra are obtained from the full-disk observations. Fourier spectra are obtained from the high-resolution observations. The p-mode oscillation signal and instrumental artifacts are reduced by tempo…

2000 Solar Physics
SOHO 132
Simultaneous SOHO and Ground-Based Observations of a Large Eruptive Prominence and Coronal Mass Ejection
DOI: 10.1023/A:1005287524302 Bibcode: 2000SoPh..194..371P

Heinzel, P.; Plunkett, S. P.; Wu, S. T. +6 more

Coronal mass ejections (CMEs) are frequently associated with erupting prominences near the solar surface. A spectacular eruption of the southern polar crown prominence was observed on 2June 1998, accompanied by a CME that was well-observed by the LASCO coronagraphs on SOHO. The prominence was observed in its quiescent state and was followed throug…

2000 Solar Physics
SOHO 124
Solar shear flows deduced from helioseismic dense-pack samplings of ring diagrams
DOI: 10.1023/A:1005235610132 Bibcode: 2000SoPh..192..335H

Thompson, M. J.; Hill, F.; Toomre, J. +3 more

We report on large-scale horizontal flows in the solar convection zone and their variability in time and space using a local-helioseismology technique known as ring-diagram analysis. By performing this analysis on a dense mosaic of individual regions on the solar disk, i.e., a `Dense-Pack' sampling, and repeating the analysis periodically on sever…

2000 Solar Physics
SOHO 101
Travel Time Sensitivity Kernels
DOI: 10.1023/A:1005283526062 Bibcode: 2000SoPh..192..193B

Kosovichev, A. G.; Birch, A. C.

We derive, following the standard first Born approximation approach used in the geophysics literature, an expression for the travel time perturbation caused by a perturbation to sound speed. In our simple model we employ a point source at one point and calculate the time taken for a wave packet created at the source to move to a second point. In t…

2000 Solar Physics
SOHO 74
Phase-sensitive Holography of Solar Activity
DOI: 10.1023/A:1005239216840 Bibcode: 2000SoPh..192..307B

Braun, D. C.; Lindsey, C.

Phase-correlation statistics comparing acoustic radiation coming out of a particular point on the solar photosphere with acoustic radiation going into it show considerably reduced sound travel times through the subphotospheres of active regions. We have now applied techniques in phase-sensitive seismic holography to data from the Solar Oscillation…

2000 Solar Physics
SOHO 69