Search Publications

Are All Coronal Mass Ejections Hollow Flux Ropes?
DOI: 10.1086/510191 Bibcode: 2007ApJ...657..559K

Krall, J.

A quantitative specification of a three-dimensional flux rope is examined statistically for comparison to previously published statistical measures of coronal mass ejections (CMEs) as observed by the Solar Maximum Mission (SMM) spacecraft. The three-dimensional geometry that has been previously shown to reproduce statistical measures (average angu…

2007 The Astrophysical Journal
SOHO 35
The Posteruptive Evolution of a Coronal Dimming
DOI: 10.1086/512665 Bibcode: 2007ApJ...660.1653M

McIntosh, Scott W.; Davey, Alisdair R.; Leamon, Robert J. +1 more

We discuss the posteruptive evolution of a ``coronal dimming'' based on observations of the EUV corona from the Solar and Heliospheric Observatory and the Transition Region and Coronal Explorer (TRACE). This discussion highlights the roles played by magnetoconvection-driven magnetic reconnection and the global magnetic environment of the plasma in…

2007 The Astrophysical Journal
SOHO 35
Seismic Study of the Chemical Composition of the Solar Convection Zone
DOI: 10.1086/520916 Bibcode: 2007ApJ...668..603L

Basu, Sarbani; Antia, H. M.; Lin, Chia-Hsien

Recent downward revision of solar heavy-element abundances using a three-dimensional atmospheric model has introduced serious discrepancies between standard solar models and helioseismic inferences about solar structure. In this paper we investigate the possibility of determining the heavy-element abundances using helioseismic inversion techniques…

2007 The Astrophysical Journal
SOHO 35
Contamination by Surface Effects of Time-Distance Helioseismic Inversions for Sound Speed beneath Sunspots
DOI: 10.1086/515436 Bibcode: 2007ApJ...661..558C

Rajaguru, S. P.; Couvidat, S.

Using Doppler velocity data from the SOI/MDI instrument on board the SOHO spacecraft, we do time-distance helioseismic inversions for sound-speed perturbations beneath 16 sunspots observed in high-resolution mode. We clearly detect ringlike regions of enhanced sound speed beneath most sunspot penumbrae, extending from near the surface to depths of…

2007 The Astrophysical Journal
SOHO 35
Direct Measurement of the Radius and Density of the Transiting Exoplanet HD 189733b with the CHARA Array
DOI: 10.1086/519002 Bibcode: 2007ApJ...661L.195B

Swain, Mark; van Belle, Gerard T.; McAlister, Harold A. +5 more

We have measured the angular diameter of the transiting extrasolar planet host star HD 189733 using the CHARA optical/IR interferometric array. Combining our new angular diameter of 0.377+/-0.024 mas with the Hipparcos parallax leads to a linear radius for the host star of 0.779+/-0.052 Rsolar and a radius for the planet of 1.19+/-0.08 …

2007 The Astrophysical Journal
Hipparcos 35
Validation of Helioseismology through Forward Modeling: Realization Noise Subtraction and Kernels
DOI: 10.1086/519070 Bibcode: 2007ApJ...664.1234H

Hanasoge, S. M.; Duvall, T. L., Jr.; Couvidat, S.

Through a series of numerical simulations of the near-surface acoustic wavefield of the Sun, we show the utility of the forward approach in local helioseismology. We demonstrate and apply a method to subtract a large fraction of the realization noise from the simulated data. The ability to attain high signal-to-noise ratios from brief forward calc…

2007 The Astrophysical Journal
SOHO 35
Halo Coronal Mass Ejections and Configuration of the Ambient Magnetic Fields
DOI: 10.1086/511385 Bibcode: 2007ApJ...654L.171L

Liu, Y.

In this study, we seek a correlation between the speed of active region-related halo coronal mass ejections (CMEs) and the configuration of the ambient magnetic fields. Having studied 99 halo CMEs in the period from 2000 to 2004, we find that CMEs under the heliospheric current sheet are significantly slower than CMEs situated under unidirectional…

2007 The Astrophysical Journal
SOHO 35
A Changing Solar Shape
DOI: 10.1086/518212 Bibcode: 2007ApJ...660L.161E

Bush, R. I.; Emilio, M.; Kuhn, J. +1 more

The Sun's shape is sensitive to the influence of gravity, rotation, and local turbulence and magnetic fields in its outer atmosphere. A careful measurement of this shape has long been sought to better understand the solar structure and its change during the 11 yr solar cycle. Numerous disparate measurements of the solar oblateness or the fractiona…

2007 The Astrophysical Journal
SOHO 35
A Photometrically Detected Forming Cluster of Galaxies at Redshift 1.6 in the GOODS Field
DOI: 10.1086/521595 Bibcode: 2007ApJ...671.1497C

Fiore, F.; Castellano, M.; Pentericci, L. +9 more

We report the discovery of a localized overdensity at z~1.6 in the GOODS-South field, presumably a poor cluster in the process of formation. The three-dimensional galaxy density has been estimated on the basis of well-calibrated photometric redshifts from the multiband photometric GOODS-MUSIC catalog using the (2+1)-dimensional technique. The dens…

2007 The Astrophysical Journal
eHST 35
Hubble Space Telescope and Optical Observations of Three Pulsating Accreting White Dwarfs in Cataclysmic Variables
DOI: 10.1086/511854 Bibcode: 2007ApJ...658.1188S

Szkody, Paula; Sion, Edward M.; Solheim, Jan-Erik +8 more

Ultraviolet observations using the Solar Blind Channel on the Hubble Space Telescope provide light curves and low-resolution spectra of three pulsating white dwarfs in the cataclysmic variables SDSS J013132.39-090122.3, SDSS J161033.64-010223.3, and SDSS J220553.98+115553.7. The UV light curves show enhanced pulsation amplitudes over those from si…

2007 The Astrophysical Journal
eHST 34