Search Publications

Venusian middle-atmospheric dynamics in the presence of a strong planetary-scale 5.5-day wave
DOI: 10.1016/j.icarus.2011.06.017 Bibcode: 2012Icar..217..702Y

Yamamoto, Masaru; Takahashi, Masaaki

The middle atmospheric dynamics on Venus are investigated using a middle atmosphere general circulation model. The magnitude of the superrotation is sensitive to the amplitude of the planetary-scale waves. In particular, the critical level absorptions of the forced planetary-scale waves might contribute to the maintenance of the superrotation near…

2012 Icarus
VenusExpress 16
Ground-based and spacecraft observations of lightning activity on Saturn
DOI: 10.1016/j.pss.2011.07.021 Bibcode: 2012P&SS...61...53Z

Schneider, J.; Cecconi, B.; Fischer, G. +21 more

In late 2007, Saturn electrostatic discharges (SED) were simultaneously observed at the radio telescope UTR-2 and with the Cassini spacecraft. Observations at UTR-2 were performed with a multichannel receiver in the frequency range 12-33 MHz, and those performed on Cassini-with a swept frequency receiver that is part of the RPWS (Radio and Plasma …

2012 Planetary and Space Science
Cassini 16
White-Light Observations and Polarimetric Analysis of the Solar Corona During the Eclipse of 1 August 2008
DOI: 10.1007/s11207-011-9910-7 Bibcode: 2012SoPh..277..267S

Skomorovsky, V. I.; Trifonov, V. D.; Mashnich, G. P. +4 more

In order to study the solar corona during eclipses, a new telescope was constructed. Three coronal images were obtained simultaneously through a single objective of the telescope as the coronal radiation passed through three polarizers (whose transmission directions were turned 0°, 60°, and 120° in the chosen direction); one image was obtained wit…

2012 Solar Physics
SOHO 16
Coronal Mass Ejections and the Index of Effective Solar Multipole
DOI: 10.1007/s11207-012-0096-4 Bibcode: 2012SoPh..281..779O

Obridko, V. N.; Yurchyshyn, V. B.; Ivanov, E. V. +2 more

The paper considers the relationship between the cyclic variations in the velocity of coronal mass ejections (CME) and the large-scale magnetic field structure (LSMF) in cycles 21 - 23. To characterize a typical size of the LSMF structure, we have used the index of the effective solar multipole (ESMI). The cyclic behavior of the CME occurrence rat…

2012 Solar Physics
SOHO 16
Discovery of multiple shells around the planetary nebula IC 418
DOI: 10.1111/j.1365-2966.2012.21165.x Bibcode: 2012MNRAS.423.3753R

Guerrero, M. A.; Ramos-Larios, G.; Bravo-Alfaro, H. +3 more

We have analysed optical, near- and mid-IR images of the bright planetary nebula (PN) IC 418. These images probe unambiguously for the first time a number of low surface brightness structures and shells around the bright main nebula, including radial filaments or rays, a system of three concentric rings and two detached haloes with sizes ∼150 arcs…

2012 Monthly Notices of the Royal Astronomical Society
eHST 16
Scalings, Cascade and Intermittency in Solar Wind Turbulence
DOI: 10.1007/s11214-012-9907-z Bibcode: 2012SSRv..172..343C

Carbone, Vincenzo

Investigating in situ fluctuations in the interplanetary space, offers us a unique challenge to study scaling properties in a turbulent medium which cover a wide range of scales. This includes not only the inertial range, where turbulence can be described within a fluid-like approach, but also the high-frequency region, where a kinetic approach is…

2012 Space Science Reviews
Cluster 16
Nonaxisymmetric Anisotropy of Solar Wind Turbulence as a Direct Test for Models of Magnetohydrodynamic Turbulence
DOI: 10.1103/PhysRevLett.108.085001 Bibcode: 2012PhRvL.108h5001T

Chapman, S. C.; Turner, A. J.; Gogoberidze, G.

Single point spacecraft observations of the turbulent solar wind flow exhibit a characteristic nonaxisymmetric anisotropy that depends sensitively on the perpendicular power spectral exponent. We use this nonaxisymmetric anisotropy as a function of wave vector direction to test models of MHD turbulence. Using Ulysses magnetic field observations in…

2012 Physical Review Letters
Ulysses 16
Hubble Space Telescope FUV Spectra of the Post-common-envelope Hyades Binary V471 Tauri
DOI: 10.1088/0004-637X/751/1/66 Bibcode: 2012ApJ...751...66S

Bond, Howard E.; Sion, Edward M.; Godon, Patrick +4 more

We have carried out an analysis of the Hubble Space Telescope (HST)/STIS archival spectra of the magnetic white dwarf (WD) in the Hyades eclipsing-spectroscopic, post-common-envelope binary V471 Tauri, time resolved on the orbit and on the X-ray rotational phase of the magnetic WD. An HST/STIS spectrum obtained during primary eclipse reveals a hos…

2012 The Astrophysical Journal
eHST 16
Empirical Estimates of Martian Surface Pressure in Support of the Landing of Mars Science Laboratory
DOI: 10.1007/s11214-012-9876-2 Bibcode: 2012SSRv..170..837W

Withers, Paul

The aim of this work is to develop an empirical expression for diurnal mean martian surface pressure in support of the landing of Mars Science Laboratory. We evaluate the consistency of surface pressure measurements from four landers, Viking Lander 1, Viking Lander 2, Mars Pathfinder, and Phoenix, and one radio occultation experiment, Mars Global …

2012 Space Science Reviews
MEx 16
Observations of oxygen ions in the dayside magnetosheath associated with southward IMF
DOI: 10.1029/2012JA017754 Bibcode: 2012JGRA..117.7218S

Nilsson, H.; Slapak, R.; Eriksson, A. +1 more

We present a case study of high energy oxygen ions (O+) observed in the dayside terrestrial magnetosheath, in the southern hemisphere. It is shown that the presence of O+ is strongly correlated to the IMF direction: O+ is observed only for Bz < 0. Three satellites observe O+ immediately at …

2012 Journal of Geophysical Research (Space Physics)
Cluster 16