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Magnetic field investigation of the Venus plasma environment: Expected new results from Venus Express
DOI: 10.1016/j.pss.2006.04.018 Bibcode: 2006P&SS...54.1336Z

Barabash, S.; Russell, C. T.; Lammer, H. +24 more

The Venus Express mission is scheduled for launch in 2005. Among many other instruments, it carries a magnetometer to investigate the Venus plasma environment. Although Venus has no intrinsic magnetic moment, magnetic field measurements are essential in studying the solar wind interaction with Venus. Our current understanding of the solar wind int…

2006 Planetary and Space Science
VenusExpress 226
Venus Express science planning
DOI: 10.1016/j.pss.2006.04.017 Bibcode: 2006P&SS...54.1279T

Barabash, S.; Pätzold, M.; Zhang, T. L. +20 more

Venus Express is the first European mission to the planet Venus. Its payload consists of seven instruments and will investigate the atmosphere, the plasma environment, and the surface of Venus from orbit. Science planning is a complex process that takes into account requests from all experiments and the operational constraints. The planning of the…

2006 Planetary and Space Science
VenusExpress 134
Compact high-resolution spaceborne echelle grating spectrometer with acousto-optical tunable filter based order sorting for the infrared domain from 2.2 to 4.3 µm
DOI: 10.1364/AO.45.005191 Bibcode: 2006ApOpt..45.5191N

Korablev, Oleg; Neefs, Eddy; Berkenbosch, Sophie +12 more

A new compact spaceborne high-resolution spectrometer developed for the European Space Agency's Venus Express spacecraft is described. It operates in the IR wavelength range of 2.2 to 4.3 µm and measures absorption spectra of minor constituents in the Venusian atmosphere. It uses a novel echelle grating with a groove density of 4 lines/mm in…

2006 Applied Optics
VenusExpress 98
Loss of hydrogen and oxygen from the upper atmosphere of Venus
DOI: 10.1016/j.pss.2006.04.022 Bibcode: 2006P&SS...54.1445L

Barabash, S.; Gunell, H.; Lammer, H. +9 more

Atmospheric escape from the upper atmosphere of Venus is mainly influenced by the loss of hydrogen and oxygen caused by the interaction of solar radiation and particle flux with the unprotected planetary environment. Because one main aim of the ASPERA-4 particle/plasma and VEX-MAG magnetic field experiments on board of ESA's forthcoming Venus Expr…

2006 Planetary and Space Science
VenusExpress 95
Radio science investigations by VeRa onboard the Venus Express spacecraft
DOI: 10.1016/j.pss.2006.04.032 Bibcode: 2006P&SS...54.1315H

Pätzold, M.; Bird, M. K.; Imamura, T. +10 more

The Venus Express Radio Science Experiment (VeRa) uses radio signals at wavelengths of 3.6 and 13 cm ("X"- and "S"-band, respectively) to investigate the Venus surface, neutral atmosphere, ionosphere, and gravity field, as well as the interplanetary medium. An ultrastable oscillator (USO) provides a high quality onboard reference frequency source;…

2006 Planetary and Space Science
VenusExpress 80
Dynamics of the Venus upper atmosphere: Outstanding problems and new constraints expected from Venus Express
DOI: 10.1016/j.pss.2006.04.023 Bibcode: 2006P&SS...54.1371B

Drossart, P.; Bougher, S. W.; Rafkin, S.

A consistent picture of the dynamics of the Venus upper atmosphere from ∼90 to 200 km has begun to emerge [e.g., Bougher, S.W., Alexander, M.J., Mayr, H.G., 1997. Upper Atmosphere Dynamics: Global Circulation and Gravity Waves. Venus II, CH. 2.4. University of Arizona Press, Tucson, pp. 259-292; Lellouch, E., Clancy, T., Crisp, D., Kliore, A., Tit…

2006 Planetary and Space Science
VenusExpress 63
Venus-solar wind interaction: Asymmetries and the escape of O+ ions
DOI: 10.1016/j.pss.2006.04.030 Bibcode: 2006P&SS...54.1472K

Kallio, E.; Janhunen, P.; Jarvinen, R.

We study the interaction between Venus and the solar wind using a global three-dimensional self-consistent quasi-neutral hybrid (QNH) model. The model treats ions (H+,O+) as particles and electrons as a massless charge neutralizing fluid. In the analysed Parker spiral interplanetary magnetic field (IMF) case (IMF=[8.09,5.88,0…

2006 Planetary and Space Science
VenusExpress 57
Venus Express: Scientific goals, instrumentation, and scenario of the mission
DOI: 10.1134/S0010952506040071 Bibcode: 2006CosRe..44..334T

Barabash, S.; Zhang, T. L.; Bertaux, J. -L. +23 more

The first European mission to Venus (Venus Express) is described. It is based on a repeated use of the Mars Express design with minor modifications dictated in the main by more severe thermal environment at Venus. The main scientific task of the mission is global exploration of the Venusian atmosphere, circumplanetary plasma, and the planet surfac…

2006 Cosmic Research
VenusExpress 50
Venus O + pickup ions: Collected PVO results and expectations for Venus Express
DOI: 10.1016/j.pss.2005.10.009 Bibcode: 2006P&SS...54.1457L

Luhmann, J. G.; Russell, C. T.; Lyon, J. G. +1 more

Observations of oxygen pickup ions by the plasma analyzer on the Pioneer Venus Orbiter (PVO) Mission arguably launched broad interest in solar wind erosion of unmagnetized planet atmospheres, and its potential evolutionary effects. Oxygen pickup ions may play key roles in the removal of the oxygen excess left behind from the photodissociation of w…

2006 Planetary and Space Science
VenusExpress 43
Venus before Venus Express
DOI: 10.1016/j.pss.2006.04.031 Bibcode: 2006P&SS...54.1249T

Taylor, Fredric W.

An overview is given of current knowledge and mysteries about the planet Venus, with emphasis on those aspects that are intended to be studied with the Venus Express mission following orbit insertion at the planet in March 2006.

2006 Planetary and Space Science
VenusExpress 32