Search Publications

Three-dimensional global simulation of interplanetary coronal mass ejection propagation from the Sun to the heliosphere: Solar event of 12 May 1997
DOI: 10.1029/2006JA012211 Bibcode: 2007JGRA..112.9104W

Wu, S. T.; Dryer, M.; Fry, C. D. +2 more

A newly developed hybrid code, HAFv.2+3DMHD, that combines two simulation codes, Hakamada-Akasofu-Fry code version 2 (HAFv.2) and a fully three-dimensional (3-D), time-dependent MHD simulation code, is used to study the global interplanetary coronal mass ejection (ICME) from the 12 May 1997 solar event. The solar wind structure is first simulated …

2007 Journal of Geophysical Research (Space Physics)
SOHO 58
The outburst of the eruptive young star OO Serpentis between 1995 and 2006
DOI: 10.1051/0004-6361:20066108 Bibcode: 2007A&A...470..211K

Prusti, T.; Siebenmorgen, R.; Hony, S. +4 more

Aims:OO Serpentis is a deeply embedded pre-main sequence star in the Serpens NW star-forming region. The star went into outburst in 1995 and gradually faded afterwards. In many respects its eruption resembled the well-known FU Orionis-type (FUor) or EX Lupi-type (EXor) outbursts. Since very few such events have ever been documented at infrared wav…

2007 Astronomy and Astrophysics
ISO 58
Atmospheric composition, chemistry, and clouds
DOI: 10.1029/176GM06 Bibcode: 2007GMS...176...73M

Esposito, Larry W.; Yung, Yuk L.; Mills, Franklin P.

Venus' atmosphere has a rich chemistry involving interactions among sulfur, chlorine, nitrogen, hydrogen, and oxygen radicals. The chemical regimes in the atmosphere range from ion-neutral reactions in the ionosphere to photochemistry in the middle atmosphere to thermal equilibrium chemistry and surface-atmosphere reactions in the lower atmosphere…

2007 Geophysical Monograph Series
VenusExpress 58
Ptolemy an Instrument to Measure Stable Isotopic Ratios of Key Volatiles on a Cometary Nucleus
DOI: 10.1007/s11214-006-9001-5 Bibcode: 2007SSRv..128..363W

Andrews, D. J.; Leese, M. R.; Zarnecki, J. C. +17 more

A fundamental goal of cometary studies is to determine the exact relationship between these bodies and the Solar System - the question(s) can be summarised as follows: did comets originate during the same events that spawned the Sun and planets, are they more primitive bodies that record a pre-solar history, or are they interstellar materials coll…

2007 Space Science Reviews
Rosetta 58
Feedback in the Antennae Galaxies (NGC 4038/9). I. High-Resolution Infrared Spectroscopy of Winds from Super Star Clusters
DOI: 10.1086/520910 Bibcode: 2007ApJ...668..168G

Graham, James R.; Gilbert, Andrea M.

We present high-resolution (R~24,600) near-IR spectroscopy of the youngest super star clusters (SSCs) in the prototypical starburst merger, the Antennae galaxies. These SSCs are young (3-7 Myr old) and massive (105-107 Msolar for a Kroupa initial mass function), and their spectra are characterized by broad, extende…

2007 The Astrophysical Journal
eHST 58
Role of photoionization in the formation of complex organic molecules in Titan's upper atmosphere
DOI: 10.1029/2006GL028317 Bibcode: 2007GeoRL..34.2204I

Imanaka, Hiroshi; Smith, Mark A.

Recent observations by the Cassini Orbiter suggest that complex organic chemistry occurs in the upper atmosphere of Titan. To understand the role of EUV-VUV light in the complex organic chemistry of Titan's upper atmosphere, we investigate the formation of gaseous species from a N2/CH4 gas mixture as a function of irradiation…

2007 Geophysical Research Letters
Cassini 57
Measuring PAH Emission in Ultradeep Spitzer IRS Spectroscopy of High-Redshift IR-Luminous Galaxies
DOI: 10.1086/512802 Bibcode: 2007ApJ...659..941T

Frayer, D. T.; Scott, D.; Chary, R. +9 more

The study of the dominant population of high-redshift IR-luminous galaxies (1011-1012 Lsolar at 1<z<3), requires observation of sources at the ~0.1 mJy level in the mid-IR. We present the deepest spectra taken to date with the Infrared Spectrograph (IRS) on the Spitzer Space Telescope. We targeted two faint (…

2007 The Astrophysical Journal
eHST 57
Dust Environment Modelling of Comet 67P/Churyumov-Gerasimenko
DOI: 10.1007/s11214-006-9139-1 Bibcode: 2007SSRv..128...79A

Agarwal, Jessica; Grün, Eberhard; Müller, Michael

Dust is an important constituent of cometary emission; its analysis is one of the major objectives of ESA's Rosetta mission to comet 67P/Churyumov-Gerasimenko (C-G). Several instruments aboard Rosetta are dedicated to studying various aspects of dust in the cometary coma, all of which require a certain level of exposure to dust to achieve their go…

2007 Space Science Reviews
Rosetta 57
Local plasma processes and enhanced electron densities in the lower ionosphere in magnetic cusp regions on Mars
DOI: 10.1016/j.pss.2007.07.003 Bibcode: 2007P&SS...55.2164N

Gurnett, D. A.; Lundin, R.; Winningham, J. D. +11 more

Both the MARSIS ionospheric sounder and the charged particle instrument package ASPERA-3 are experiments on board the Mars Express spacecraft. Joint observations have shown that events of intense ionospheric electron density enhancements occur in the lower ionosphere of magnetic cusp regions, and that these enhancements are not associated with pre…

2007 Planetary and Space Science
MEx 57
The Titan 14N/ 15N and 12C/ 13C isotopic ratios in HCN from Cassini/CIRS
DOI: 10.1016/j.icarus.2007.06.001 Bibcode: 2007Icar..191..712V

Bézard, Bruno; Vinatier, Sandrine; Nixon, Conor A.

We report the detection of H 13CN and HC 15N in mid-infrared spectra recorded by the Composite Infrared Spectrometer (CIRS) aboard Cassini, along with the determination of the 12C/ 13C and 14N/ 15N isotopic ratios. We analyzed two sets of limb spectra recorded near 13-15° S (Tb flyb…

2007 Icarus
Cassini 57