Search Publications

Background and pickup ion velocity distribution dynamics in Titan's plasma environment: 3D hybrid simulation and comparison with CAPS T9 observations
DOI: 10.1016/j.asr.2011.05.026 Bibcode: 2011AdSpR..48.1114L

Hartle, R. E.; Sittler, E. C.; Cooper, J. F. +2 more

In this report we discuss the ion velocity distribution dynamics from the 3D hybrid simulation. In our model the background, pickup, and ionospheric ions are considered as a particles, whereas the electrons are described as a fluid. Inhomogeneous photoionization, electron-impact ionization and charge exchange are included in our model. We also tak…

2011 Advances in Space Research
Cassini 9
Temporal changes in the frequencies and widths of the solar p-mode oscillations
DOI: 10.1088/1742-6596/271/1/012029 Bibcode: 2011JPhCS.271a2029R

Schou, J.; Rodriguez, J.; Scherrer, P. +7 more

We present a study of the temporal changes in the sensitivities of the frequencies and widths of the solar p-mode oscillations to corresponding changes in the levels of solar activity during Solar Cycle 23. From MDI and GONG++ full-disk Dopplergram three-day time series obtained between 1996 and 2008 we have computed a total of 221 sets of m-avera…

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 9
Comparisons of Supergranule Characteristics During the Solar Minima of Cycles 22/23 and 23/24
DOI: 10.1007/s11207-011-9718-5 Bibcode: 2011SoPh..270..125W

Williams, Peter E.; Pesnell, W. Dean

Supergranulation is a component of solar convection that manifests itself on the photosphere as a cellular network of around 35 Mm across, with a turnover lifetime of 1 - 2 days. It is strongly linked to the structure of the magnetic field. The horizontal, divergent flows within supergranule cells carry local field lines to the cell boundaries, wh…

2011 Solar Physics
SOHO 9
Accretion, jets and winds: High-energy emission from young stellar objects
DOI: 10.1002/asna.201111559 Bibcode: 2011AN....332..448G

Günther, H. M.

This article summarizes the processes of high-energy emission in young stellar objects. Stars of spectral type A and B are called Herbig Ae/Be (HAeBe) stars in this stage, all later spectral types are termed classical T Tauri stars (CTTS). Both types are studied by high-resolution X-ray and UV spectroscopy and modeling. Three mechanisms contribute…

2011 Astronomische Nachrichten
XMM-Newton 9
Water in star-forming regions with Herschel
DOI: 10.1002/asna.201111565 Bibcode: 2011AN....332..475K

van Dishoeck, E. F.; Kristensen, L. E.

The Herschel Space Observatory is well suited to address several important questions in star- and planet formation, as is evident from its first year of operation. This paper focuses on observations of water, a key molecule in the physics and chemistry of star-formation. In the WISH Key Program, a comprehensive set of water lines is being obtained…

2011 Astronomische Nachrichten
Herschel 9
The magnetic configuration of the high-latitude cusp and dayside magnetopause under strong magnetic shears
DOI: 10.1029/2011JA016501 Bibcode: 2011JGRA..116.9228S

Lucek, E.; Dunlop, M.; Liu, Z. X. +8 more

This paper investigates the structure of the magnetic field near the magnetopause (MP) by analyzing the multiple-point magnetic measurements from the Cluster mission. In this paper, the spatial distribution of the curvature radius of the MP surface at the noon-midnight meridian and for situations with moderate dynamical pressure of solar wind is i…

2011 Journal of Geophysical Research (Space Physics)
Cluster 9
Close to the Dredge: Precise X-Ray C and N Abundances in λ Andromeda and Its Precocious Red Giant Branch Mixing Problem
DOI: 10.1088/0004-6256/142/5/144 Bibcode: 2011AJ....142..144D

Ness, J. -U.; Drake, Jeremy J.; Eldridge, John J. +2 more

Chandra LETG+HRC-S and XMM-Newton RGS spectra of H-like C and N lines formed in the corona of the primary star of the RS CVn-type binary λ And, a mildly metal-poor G8 III-IV first ascent giant that completed dredge-up ~50 Myr ago, have been used to make a precise measurement of its surface C/N ratio. We obtain the formal result [C/N] = 0.03 ± 0.07…

2011 The Astronomical Journal
XMM-Newton 9
Landform hierarchy and evolution in Gorgonum and Atlantis basins, Mars
DOI: 10.1016/j.icarus.2010.08.006 Bibcode: 2011Icar..211..366C

Capitan, Radu Dan; Van De Wiel, Marco

This paper describes the evolution of landforms in Atlantis and Gorgonum basins, using a geomorphologic approach which interprets landform distribution and hierarchy. Rather than looking at the distribution of large-area (>10 6 km 2) geologic sequences, this study focuses on interpreting the local-scale (<10 3

2011 Icarus
MEx 9
The Internal Proper Motions of Stars in the Open Cluster M35
DOI: 10.1088/0004-6256/142/2/53 Bibcode: 2011AJ....142...53M

Harrison, Thomas E.; Benedict, G. Fritz; McArthur, Barbara E. +1 more

Relative proper motions, based on 108 orbits of Hubble Space Telescope Fine Guidance Sensor data extending from 1992 to 2006, are reported for 74 stars in the open cluster M35 (NGC 2168). A subset of 22 of these objects are then used to compute the cluster's internal proper motion dispersions in both right ascension and declination. We find that t…

2011 The Astronomical Journal
eHST 9
Titan impacts and escape
DOI: 10.1016/j.icarus.2010.09.013 Bibcode: 2011Icar..211..707K

Zahnle, Kevin J.; Korycansky, D. G.

We report on hydrodynamic calculations of impacts of large (multi-kilometer) objects on Saturn's moon Titan. We assess escape from Titan, and evaluate the hypothesis that escaping ejecta blackened the leading hemisphere of Iapetus and peppered the surface of Hyperion. We carried out two- and three-dimensional simulations of impactors ranging in si…

2011 Icarus
Cassini 9