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Transmission Electron Microscopy of CONCORDIA UltraCarbonaceous Antarctic MicroMeteorites (UCAMMs): Mineralogical properties
DOI: 10.1016/j.gca.2011.10.025 Bibcode: 2012GeCoA..76...68D

Engrand, C.; Rouzaud, J. -N.; Duprat, J. +2 more

We performed mineralogical and petrographic studies of three UltraCarbonaceous Antarctic Micrometeorites (UCAMMs) by analytical transmission electron microscopy (TEM). The UCAMMs were identified in the CONCORDIA micrometeorite collection (2002 and 2006) recovered from central Antarctic snow, and are of probable cometary origin. UCAMMs are dominate…

2012 Geochimica et Cosmochimica Acta
Rosetta 78
Global maps of anhydrous minerals at the surface of Mars from OMEGA/MEx
DOI: 10.1029/2012JE004117 Bibcode: 2012JGRE..117.0J14O

Bibring, J. -P.; Gondet, B.; Langevin, Y. +7 more

We here reassess the global distribution of several key mineral species using the entire OMEGA/Mars Express VIS-NIR imaging spectrometer data set, acquired from orbit insertion in January 2004 to August 2010. Thirty-two pixels per degree global maps of ferric oxides, pyroxenes and olivines have been derived. A significant filtering process was app…

2012 Journal of Geophysical Research (Planets)
MEx 78
On the effects of clouds and hazes in the atmospheres of hot Jupiters: semi-analytical temperature-pressure profiles
DOI: 10.1111/j.1365-2966.2011.19943.x Bibcode: 2012MNRAS.420...20H

Sing, David K.; Heng, Kevin; Pont, Frédéric +1 more

Motivated by the work of Guillot, we present a semi-analytical formalism for calculating the temperature-pressure profiles in hot Jovian atmospheres which includes the effects of clouds/hazes and collision-induced absorption. Using the dual-band approximation, we assume that stellar irradiation and thermal emission from the hot Jupiter occur at di…

2012 Monthly Notices of the Royal Astronomical Society
eHST 78
LoCuSS: A Dynamical Analysis of X-Ray Active Galactic Nuclei in Local Clusters
DOI: 10.1088/0004-637X/754/2/97 Bibcode: 2012ApJ...754...97H

Finoguenov, A.; Smith, G. P.; Okabe, N. +7 more

We present a study of the distribution of X-ray active galactic nuclei (AGNs) in a representative sample of 26 massive clusters at 0.15 < z < 0.30, combining Chandra observations sensitive to X-ray point sources of luminosity LX ~ 1042 erg s-1 at the cluster redshift with extensive and highly complete spectro…

2012 The Astrophysical Journal
eHST 78
The location of reconnection at the magnetopause: Testing the maximum magnetic shear model with THEMIS observations
DOI: 10.1029/2011JA016959 Bibcode: 2012JGRA..117.1201T

Fuselier, S. A.; Phan, T. D.; Trattner, K. J. +1 more

Reconnection at the Earth's magnetopause is the mechanism by which magnetic fields in different regions change topology to create open magnetic field lines that allow energy and momentum to flow into the magnetosphere. One of the long-standing open questions about magnetic reconnection is the location of the reconnection line. There are two reconn…

2012 Journal of Geophysical Research (Space Physics)
Cluster 78
A unique volcanic field in Tharsis, Mars: Pyroclastic cones as evidence for explosive eruptions
DOI: 10.1016/j.icarus.2011.11.030 Bibcode: 2012Icar..218...88B

Hauber, E.; Brož, P.

Based on theoretical grounds, explosive basaltic volcanism should be common on Mars, yet the available morphological evidence is sparse. We test this hypothesis by investigating a unique unnamed volcanic field north of the shield volcanoes Biblis Patera and Ulysses Patera on Mars, where we observe several small conical edifices and associated lava…

2012 Icarus
MEx Ulysses 77
Three-dimensional Evolution of Solar Wind during Solar Cycles 22-24
DOI: 10.1088/0004-637X/751/2/128 Bibcode: 2012ApJ...751..128M

Manoharan, P. K.

This paper presents an analysis of three-dimensional evolution of solar wind density turbulence and speed at various levels of solar activity between solar cycles 22 and 24. The solar wind data used in this study have been obtained from the interplanetary scintillation (IPS) measurements made at the Ooty Radio Telescope, operating at 327 MHz. Resu…

2012 The Astrophysical Journal
SOHO Ulysses 77
Validation of the 3D AMR SIP-CESE Solar Wind Model for Four Carrington Rotations
DOI: 10.1007/s11207-012-9969-9 Bibcode: 2012SoPh..279..207F

Wu, S. T.; Feng, Xueshang; Xiang, Changqing +5 more

We carry out the adaptive mesh refinement (AMR) implementation of our solar-interplanetary space-time conservation element and solution element (CESE) magnetohydrodynamic model (SIP-CESE MHD model) using a six-component grid system (Feng, Zhou, and Wu, Astrophys. J.655, 1110, 2007; Feng et al., Astrophys. J.723, 300, 2010). By transforming the gov…

2012 Solar Physics
SOHO 77
Spitzer Observations of Young Red Quasars
DOI: 10.1088/0004-637X/757/2/125 Bibcode: 2012ApJ...757..125U

Lacy, Mark; Schulz, Bernhard; Urrutia, Tanya +3 more

We present mid-infrared spectra and photometry of 13 redshift 0.4 < z < 1 dust reddened quasars obtained with Spitzer IRS and MIPS. We compare properties derived from their infrared spectral energy distributions (intrinsic active galactic nucleus (AGN) luminosity and far-infrared luminosity from star formation) to the host luminosities and m…

2012 The Astrophysical Journal
eHST 77
Kinematic Signatures of Bulges Correlate with Bulge Morphologies and Sérsic Index
DOI: 10.1088/0004-637X/754/1/67 Bibcode: 2012ApJ...754...67F

Bender, Ralf; Drory, Niv; Fisher, David B. +3 more

We use the Marcario Low Resolution Spectrograph at the Hobby-Eberly Telescope to study the kinematics of pseudobulges and classical bulges in the nearby universe. We present major axis rotational velocities, velocity dispersions, and h 3 and h 4 moments derived from high-resolution (σinst ≈ 39 km s-1) sp…

2012 The Astrophysical Journal
eHST 77