Search Publications

Electron acoustic solitons in the presence of an electron beam and superthermal electrons
DOI: 10.5194/npg-18-627-2011 Bibcode: 2011NPGeo..18..627D

Lakhina, G. S.; Singh, S. V.; Bharuthram, R. +1 more

Arbitrary amplitude electron acoustic solitons are studied in an unmagnetized plasma having cold electrons and ions, superthermal hot electrons and an electron beam. Using the Sagdeev pseudo potential method, theoretical analysis is carried out by assuming superthermal hot electrons having kappa distribution. The results show that inclusion of an …

2011 Nonlinear Processes in Geophysics
Cluster 43
Evolution of the equatorial oscillation in Saturn's stratosphere between 2005 and 2010 from Cassini/CIRS limb data analysis
DOI: 10.1029/2011GL047192 Bibcode: 2011GeoRL..38.9201G

Flasar, F. M.; Bézard, B.; Fouchet, T. +2 more

We present an analysis of thermal infrared spectra acquired in limb viewing geometry by Cassini/CIRS in February 2010. We retrieve vertical profiles of Saturn's stratospheric temperature from 20 hPa to 10-2 hPa, at 9 latitudes between 20°N and 20°S. Using the gradient thermal wind equation, we derive a map of the zonal wind field. Both …

2011 Geophysical Research Letters
Cassini 43
The expansion proper motions of the planetary nebula NGC 6302 from Hubble Space Telescope imaging
DOI: 10.1111/j.1365-2966.2011.19087.x Bibcode: 2011MNRAS.416..715S

Walsh, J. R.; Zijlstra, A. A.; Szyszka, C.

Planetary nebulae expand on time-scales of 103- 104 yr. For nearby objects, their expansion can be detected within years to decades. The pattern of expansion probes the internal velocity field and provides clues to the nebula ejection mechanism. In the case of non-symmetric nebulae, and bipolar nebulae in particular, it can a…

2011 Monthly Notices of the Royal Astronomical Society
eHST 43
Compositional interpretation of PFS/MEx and TES/MGS thermal infrared spectra of Phobos
DOI: 10.1016/j.pss.2011.01.019 Bibcode: 2011P&SS...59.1308G

Duxbury, T.; Geminale, A.; Formisano, V. +4 more

The origin of the Martian satellites presents a puzzle of long standing. Addressing the composition of Phobos will help constrain theories of its formation. Visible and near-infrared spectra of Phobos lack deep absorption features, making the compositional interpretation a tricky task. PFS/MEx and TES/MGS observations in the thermal infrared show …

2011 Planetary and Space Science
MEx 43
Detection of Supergranulation Alignment in Polar Regions of the Sun by Helioseismology
DOI: 10.1088/2041-8205/726/2/L17 Bibcode: 2011ApJ...726L..17N

Zhao, Junwei; Kosovichev, Alexander G.; Sekii, Takashi +1 more

We report on a new phenomenon of "alignment" of supergranulation cells in the polar regions of the Sun. Recent high-resolution data sets obtained by the Solar Optical Telescope on board the Hinode satellite enabled us to investigate supergranular structures in high-latitude regions of the Sun. We have carried out a local helioseismology time-dista…

2011 The Astrophysical Journal
Hinode 43
Water Production by Comet 103P/Hartley 2 Observed with the SWAN Instrument on the SOHO Spacecraft
DOI: 10.1088/2041-8205/734/1/L6 Bibcode: 2011ApJ...734L...6C

Bertaux, J. -L.; Combi, M. R.; Quémerais, E. +2 more

Global water production rates were determined from the Lyα emission of hydrogen around comet 103P/Hartley 2, observed with the SWAN (Solar Wind Anisotropies) all-sky camera on the SOHO spacecraft from 2010 September 14 through December 12. This time period included the November 4 flyby by the EPOXI spacecraft. Water production was three times lowe…

2011 The Astrophysical Journal
SOHO 43
First detection of hydrogen isocyanide (HNC) in Titan's atmosphere
DOI: 10.1051/0004-6361/201118189 Bibcode: 2011A&A...536L..12M

Lara, L. M.; Hartogh, P.; Lellouch, E. +7 more

We report on the first identification of hydrogen isocyanide (HNC) in Titan's atmosphere, from observations using the HIFI instrument on the Herschel Space Observatory. An emission line from the HNC J = 6 → 5 rotational transition at 543.897 GHz was measured in Titan on June 14 and December 31, 2010. Radiative transfer modeling indicates that the …

2011 Astronomy and Astrophysics
Cassini Herschel 43
Monitoring a high-amplitude δ Scuti star for 152 days: discovery of 12 additional modes and modulation effects in the light curve of CoRoT 101155310
DOI: 10.1051/0004-6361/201016045 Bibcode: 2011A&A...528A.147P

Auvergne, M.; Baudin, F.; Poretti, E. +12 more


Aims: The detection of small-amplitude nonradial modes in high-amplitude δ Sct (HADS) variables has been very elusive until at least five of them were detected in the light curve of V974 Oph obtained from ground-based observations. The combination of radial and nonradial modes has a high asteroseismic potential, thanks to the strong constrain…

2011 Astronomy and Astrophysics
CoRoT 43
Study of the many fluorescent lines and the absorption variability in GX 301-2 with XMM-Newton
DOI: 10.1051/0004-6361/201117665 Bibcode: 2011A&A...535A...9F

Wilms, J.; Ferrigno, C.; Pottschmidt, K. +7 more

We present an in-depth study of the high mass X-ray binary (HMXB) GX 301-2 during its pre-periastron flare using data from the XMM-Newton satellite. The energy spectrum shows a power law continuum absorbed by a large equivalent hydrogen column on the order of 1024 cm-2 and a prominent Fe Kα fluorescent emission line. Besides …

2011 Astronomy and Astrophysics
XMM-Newton 43
Electron dynamics in two-dimensional asymmetric anti-parallel reconnection
DOI: 10.1063/1.3646316 Bibcode: 2011PhPl...18j2901E

Pritchett, P. L.; Egedal, J.; Daughton, W. +1 more

Kinetic simulations and spacecraft observations have documented strong anisotropy in the electron distribution function during magnetic reconnection. The level and role of electron pressure anisotropy is investigated for asymmetric geometries applicable to reconnection in the day-side magnetopause. A previously derived analytic model for the press…

2011 Physics of Plasmas
Cluster 43