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Polarization of Saturn's moon Iapetus. II. Comparison of the dark and the bright sides
DOI: 10.1051/0004-6361/201220177 Bibcode: 2013A&A...549A..61E

Muinonen, K.; Tozzi, G. P.; Boehnhardt, H. +3 more

Context. The surface properties of atmosphereless solar system objects can be constrained by investigating the nature of the polarized light scattered from their surfaces.
Aims: We provide new and precise measurements of the phase angle and the wavelength dependence of linear polarization on the leading side of Iapetus over the maximum phase …

2013 Astronomy and Astrophysics
Cassini 3
Magnetic interconnection of Saturn's polar regions: comparison of modelling results with Hubble Space Telescope UV auroral images
DOI: 10.5194/angeo-31-1447-2013 Bibcode: 2013AnGeo..31.1447B

Belenkaya, E. S.; Cowley, S. W. H.; Kalegaev, V. V. +2 more

We consider the magnetic interconnection of Saturn's northern and southern polar regions controlled by the interplanetary magnetic field (IMF), studying in particular the more complex and interesting case of southward IMF, when the Kronian magnetospheric magnetic field structure is the most twisted. The simpler case of northward IMF is also discus…

2013 Annales Geophysicae
eHST 3
Plasma processes at comet Churyumov-Gerasimenko: Expectations for Rosetta
DOI: 10.1017/S0022377813001116 Bibcode: 2013JPlPh..79.1067M

Mendis, D. A.; Horányi, M.; Horányi

The Rosetta-Philae mission to comet 67P/Churyumov-Gerasimenko in 2014 will provide a unique opportunity to observe the variable nature of the interaction of a comet with the solar radiation and the solar wind, as the comet approaches the Sun. In this short paper we will focus on the varying global structure of the cometary plasma environment. Spec…

2013 Journal of Plasma Physics
Rosetta 3
Martian atmospheric particulate spectral end-members recovery from PFS and IRIS data
DOI: 10.1016/j.icarus.2013.08.002 Bibcode: 2013Icar..226.1294D

Palomba, Ernesto; Zinzi, Angelo; Helbert, Jörn +2 more

We present an application of a multivariate analyses technique on data returned by the Planetary Fourier Spectrometer (PFS) instrument on board the ESA’s Mars Express (MEX) spacecraft in order to separate the atmospheric contribution from the observed radiation. We observe that Thermal/Far Infrared spectra returned from Mars, covering almost a who…

2013 Icarus
MEx 3
Photospheric Stratification of a Central Umbral Dot Using Stokes Profiles Recorded by Hinode: A Different Single-Case Study
DOI: 10.1007/s11207-013-0277-9 Bibcode: 2013SoPh..286..327H

Hamedivafa, H.

We aim to study the physical nature of a central umbral dot (UD) close to disk center by analyzing full-Stokes spectra of the two Fe I lines at 630 nm recorded by the spectropolarimeter on Hinode. Thermal and magnetic properties of the UD were directly inferred from Stokes profiles. Then, we applied the inversion code SIR to retrieve a single-comp…

2013 Solar Physics
Hinode 2
Probing the fast outflow in IRAS 15452 - 5459 with ATCA observations of OH, H2O and SiO masers
DOI: 10.1093/mnras/stt1039 Bibcode: 2013MNRAS.434..542C

Menten, K. M.; Cerrigone, L.; Wiesemeyer, H.

Maser lines of OH, H2O and SiO are commonly observed in O-rich asymptotic giant branch (AGB) stars, but their presence after the end of the AGB phase is linked to non-spherical mass-loss processes. IRAS 15452 - 5459 is a post-AGB star with an hourglass nebula whose maser lines are quite peculiar. We observed all of the three maser speci…

2013 Monthly Notices of the Royal Astronomical Society
eHST 2
Interstellar Absorption Lines in the Direction of the Cataclysmic Variable SS Cygni
DOI: 10.1086/674364 Bibcode: 2013PASP..125.1429R

Ritchey, Adam M.; Wallerstein, George; McKeever, Jean

Not Available

Based on observations obtained with the Apache Point Observatory 3.5 m telescope, which is owned and operated by the Astrophysical Research Consortium, and on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Mikulski Archive for Space Telescopes. STScI is operated by the Association of Universities f…

2013 Publications of the Astronomical Society of the Pacific
eHST 2
Intensities of the Venusian N2 electron-impact excited dayglow emissions
DOI: 10.1002/2013JA019277 Bibcode: 2013JGRA..118.7850F

Fox, Jane L.; F. Hać, Nicholas E.

Dayglow emissions are signatures of both the energy deposition into an atmosphere and the abundances of the species from which they arise. The first N2 dayglow emissions from Mars, the (0,5) and (0,6) bands of the N2 Vegard-Kaplan band system, were detected by the Spectroscopy for Investigations of the Characteristics of the …

2013 Journal of Geophysical Research (Space Physics)
VenusExpress 2
X-ray study of clusters at the outer edge and beyond
DOI: 10.1002/asna.201211850 Bibcode: 2013AN....334..325O

Akamatsu, H.; Ohashi, T.; Takei, Y. +2 more

We report on recent Suzaku results on cluster outer regions. Relaxed clusters show a monotonous temperature decline to the virial radii, reaching 1/3 to 1/4 of the central levels. Significant temperature jumps have been confirmed for a number of radio relics, including A 3667, A 3376, and CIZA J2242.8+5301. This confirms that the radio relics gene…

2013 Astronomische Nachrichten
Suzaku 2
INTEGRAL/SPI data segmentation to retrieve source intensity variations
DOI: 10.1051/0004-6361/201219605 Bibcode: 2013A&A...555A..52B

Bouchet, L.; Chauvin, M.; Amestoy, P. R. +2 more

Context. The INTEGRAL/SPI, X/γ-ray spectrometer (20 keV-8 MeV) is an instrument for which recovering source intensity variations is not straightforward and can constitute a difficulty for data analysis. In most cases, determining the source intensity changes between exposures is largely based on a priori information.
Aims: We propose techniqu…

2013 Astronomy and Astrophysics
INTEGRAL 2