Search Publications

Inferring Photospheric Velocity Fields Using a Combination of Minimum Energy Fit, Local Correlation Tracking, and Doppler Velocity
DOI: 10.1086/528363 Bibcode: 2008ApJ...677..751R

Longcope, D. W.; Ravindra, B.; Abbett, W. P.

The minimum energy fit (MEF), a velocity inversion technique, infers all components of the photospheric velocity that are consistent with the induction equation. From the set of consistent velocity fields, it selects the smallest overall flow speed by minimizing a kinetic energy functional. If partial velocity information is available from other m…

2008 The Astrophysical Journal
SOHO 26
Frequencies of wave packets of whistler-mode chorus inside its source region: a case study
DOI: 10.5194/angeo-26-1665-2008 Bibcode: 2008AnGeo..26.1665S

Gurnett, D. A.; Pickett, J. S.; Trakhtengerts, V. Y. +5 more

Whistler-mode chorus is a structured wave emission observed in the Earth's magnetosphere in a frequency range from a few hundreds of Hz to several kHz. We investigate wave packets of chorus using high-resolution measurements recorded by the WBD instrument on board the four Cluster spacecraft. A night-side chorus event observed during geomagnetical…

2008 Annales Geophysicae
Cluster 26
Asteroid 2867 Steins. III. Spitzer Space Telescope observations, size determination, and thermal properties
DOI: 10.1051/0004-6361:20078996 Bibcode: 2008A&A...487.1187L

Jorda, L.; Lamy, P. L.; Barucci, M. A. +6 more

Context: Asteroid 2867 Steins is the first target of the Rosetta space mission with a flyby scheduled in September 2008.
Aims: An early characterization is needed to optimize the flyby parameters and the science operations, and to maximize the scientific return.
Methods: We used the infrared spectrograph (IRS) of the Spitzer Space Telescop…

2008 Astronomy and Astrophysics
Rosetta 26
Spectroscopy and multiband photometry of the afterglow of intermediate duration γ-ray burst GRB 040924 and its host galaxy
DOI: 10.1051/0004-6361:20078050 Bibcode: 2008A&A...481..319W

Hornstrup, A.; Vreeswijk, P. M.; Wijers, R. A. M. J. +19 more

Aims: We present optical photometry and spectroscopy of the afterglow and host galaxy of gamma-ray burst GRB 040924. This GRB had a rather short duration of T90 ~2.4 s, and a well sampled optical afterglow light curve. We aim to use this dataset to find further evidence that this burst is consistent with a massive star core-collapse pro…

2008 Astronomy and Astrophysics
eHST 26
A Study of the ρ Ophiuchi Cloud: Mapping the Distribution and the Motions of Interstellar Gas
DOI: 10.1086/587132 Bibcode: 2008ApJ...679..512S

Welty, Daniel E.; Snow, Theodore P.; Destree, Joshua D.

Guest Investigator results from Hipparcos, combined with high-resolution optical spectra obtained with the Anglo-Australian Observatory, Kitt Peak National Observatory, and McDonald Observatory, are used to create a three-dimensional map of the stars and several interstellar gas components in the ρ Oph cloud complex. Many principal gas components …

2008 The Astrophysical Journal
Hipparcos eHST 26
A Comparison among Solar Diameter Measurements Carried Out from the Ground and outside Earth's Atmosphere
DOI: 10.1086/524680 Bibcode: 2008ApJ...676..651D

Thuillier, G.; Djafer, D.; Sofia, S.

The solar diameter has been measured since the 17th century, using different methods and instruments, and without a clear strategy of measurement, which could explain the lack of coherence between the results obtained. The present study confirms that the discrepancies between solar diameter measurements are mostly due to differences in instrumenta…

2008 The Astrophysical Journal
SOHO 26
UV and Radio Observations of the Coronal Shock Associated with the 2002 July 23 Coronal Mass Ejection Event
DOI: 10.1086/528839 Bibcode: 2008ApJ...677..683M

Mancuso, S.; Avetta, D.

We report on the analysis of a fast coronal mass ejection (CME)-driven shock observed on 2002 July 23 with the Ultraviolet Coronagraph Spectrometer (UVCS) on board the Solar and Heliospheric Observatory (SOHO). The CME was first detected in white light by the Large Angle and Spectrometric Coronagraph Experiment (LASCO), and shock-associated type I…

2008 The Astrophysical Journal
SOHO 26
The serendipituous discovery of a short-period eclipsing polar in 2XMMp
DOI: 10.1051/0004-6361:20079341 Bibcode: 2008A&A...485..787V

Watson, M. G.; Schwope, A.; Osborne, J. P. +3 more

We report the serendipituous discovery of the new eclipsing polar 2XMMp J131223.4+173659. Its striking X-ray light curve attracted immediate interest when we were visually inspecting the source products of the 2XMMp catalogue. This light curve revealed its likely nature as a magnetic cataclysmic variable of AM Herculis (or polar) type with an orbi…

2008 Astronomy and Astrophysics
XMM-Newton 26
NGC 602 Environment, Kinematics and Origins
DOI: 10.1086/592236 Bibcode: 2008PASP..120..972N

Sabbi, E.; Nota, A.; Gallagher, J. S. +3 more

The young star cluster NGC 602 and its associated HII region, N90, formed in a relatively isolated and diffuse environment in the Wing of the Small Magellanic Cloud. Its isolation from other regions of massive star formation and the relatively simple surrounding HI shell structure allows us to constrain the processes that may have led to its forma…

2008 Publications of the Astronomical Society of the Pacific
eHST 26
Validating Time-Distance Far-Side Imaging of Solar Active Regions through Numerical Simulations
DOI: 10.1086/592721 Bibcode: 2008ApJ...689.1373H

Zhao, Junwei; Kosovichev, Alexander G.; Hartlep, Thomas +1 more

Far-side imaging using time-distance helioseismology methods is assessed using numerically generated artificial data. The data are generated using direct numerical simulations of acoustic oscillations in a spherical solar model. Localized variations of the sound speed in the surface and subsurface layers are used to model the perturbations associa…

2008 The Astrophysical Journal
SOHO 26