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Ionospheric photoelectrons: Comparing Venus, Earth, Mars and Titan
DOI: 10.1016/j.pss.2010.07.016 Bibcode: 2011P&SS...59.1019C

Coates, A. J.; Barabash, S.; Lundin, R. +6 more

The sunlit portion of planetary ionospheres is sustained by photoionization. This was first confirmed using measurements and modelling at Earth, but recently the Mars Express, Venus Express and Cassini-Huygens missions have revealed the importance of this process at Mars, Venus and Titan, respectively. The primary neutral atmospheric constituents …

2011 Planetary and Space Science
MEx VenusExpress 57
Positron annihilation spectrum from the Galactic Centre region observed by SPI/INTEGRAL revisited: annihilation in a cooling ISM?
DOI: 10.1111/j.1365-2966.2010.17804.x Bibcode: 2011MNRAS.411.1727C

Sunyaev, R.; Tsygankov, S.; Sazonov, S. +2 more

We analyse SPI/INTEGRAL data on the 511-keV line from the Galactic Centre, accumulated over ∼6 yr of observations. We decompose the X-ray and soft gamma-ray emission of the central part of the Milky Way into relatively compact 'bulge' and more extended 'disc' components and report their spectral properties. The bulge component shows a prominent 51…

2011 Monthly Notices of the Royal Astronomical Society
INTEGRAL 57
Shoreline retreat at Titan's Ontario Lacus and Arrakis Planitia from Cassini Imaging Science Subsystem observations
DOI: 10.1016/j.icarus.2011.02.005 Bibcode: 2011Icar..212..957T

Hayes, A. G.; McEwen, A. S.; Turtle, E. P. +1 more

Recent observations by Cassini's Imaging Science Subsystem reveal that part of the shoreline of Titan's Ontario Lacus has retreated by several kilometers and may indicate that the dark area that appeared at Arrakis Planitia (80°S, 120°W) in late 2004 has subsequently faded. These changes provide constraints on aspects of Titan's methane cycle, as …

2011 Icarus
Cassini 57
Linear and nonlinear Landau resonance of kinetic Alfvén waves: Consequences for electron distribution and wave spectrum in the solar wind
DOI: 10.1063/1.3532819 Bibcode: 2011PhPl...18a2307R

Crabtree, C.; Rudakov, L.; Mithaiwala, M. +1 more

Kinetic Alfvén wave turbulence in solar wind is considered and it is shown that non-Maxwellian electron distribution function has a significant effect on the dynamics of solar wind plasmas. Linear Landau damping leads to the formation of a plateau in the parallel electron distribution function which diminishes the Landau damping rate significantly…

2011 Physics of Plasmas
Cluster 57
OH emission from warm and dense gas in the Orion Bar PDR
DOI: 10.1051/0004-6361/201116977 Bibcode: 2011A&A...530L..16G

Le Bourlot, J.; Contursi, A.; Bergin, E. A. +7 more

As part of a far-infrared (FIR) spectral scan with Herschel/PACS, we present the first detection of the hydroxyl radical (OH) towards the Orion Bar photodissociation region (PDR). Five OH (X 2Π; ν = 0) rotational Λ-doublets involving energy levels out to Eu/k ~ 511 K have been detected (at ~65, ~79, ~84, ~119 and ~163 µ…

2011 Astronomy and Astrophysics
Herschel ISO 57
The Dissipation of Solar Wind Turbulent Fluctuations at Electron Scales
DOI: 10.1088/0004-637X/730/2/114 Bibcode: 2011ApJ...730..114C

Burgess, David; Camporeale, Enrico

We present two-dimensional fully kinetic particle-in-cell simulations of decaying electromagnetic fluctuations. The computational box is such that wavelengths ranging from electron to ion gyroradii are resolved. The parameters used are realistic for the solar wind, and the ion-to-electron mass ratio is physical. The dissipation of turbulent fluctu…

2011 The Astrophysical Journal
Cluster 56
Narrow-line Seyfert 1 galaxies at hard X-rays
DOI: 10.1111/j.1365-2966.2011.19268.x Bibcode: 2011MNRAS.417.2426P

de Rosa, A.; Miniutti, G.; Ubertini, P. +7 more

Narrow-line Seyfert 1 (NLSy1) galaxies are a peculiar class of type 1 active galactic nuclei (broad-line Seyfert 1 galaxies, hereinafter BLSy1). The X-ray properties of individual objects belonging to this class are often extreme and associated with accretion at high Eddington ratios. Here, we present a study on a sample of 14 NLSy1 galaxies selec…

2011 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 56
Sorted clastic stripes, lobes and associated gullies in high-latitude craters on Mars: Landforms indicative of very recent, polycyclic ground-ice thaw and liquid flows
DOI: 10.1016/j.icarus.2010.09.010 Bibcode: 2011Icar..211..458G

Balme, M. R.; Conway, S. J.; Grindrod, P. M. +1 more

Self-organised patterns of stone stripes, polygons, circles and clastic solifluction lobes form by the sorting of clasts from fine-grained sediments in freeze-thaw cycles. We present new High Resolution Imaging Science Experiment (HiRISE) images of Mars which demonstrate that the slopes of high-latitude craters, including Heimdal crater - just 25 …

2011 Icarus
MEx 56
Observation of H2O in a strongly lensed Herschel-ATLAS source at z = 2.3
DOI: 10.1051/0004-6361/201116921 Bibcode: 2011A&A...530L...3O

Smail, I.; Omont, A.; Clements, D. L. +54 more

The Herschel survey, H-ATLAS, with its large areal coverage, has recently discovered a number of bright, strongly lensed high-z submillimeter galaxies. The strong magnification makes it possible to study molecular species other than CO, which are otherwise difficult to observe in high-z galaxies. Among the lensed galaxies already identified by H-A…

2011 Astronomy and Astrophysics
Herschel 56
Statistical Comparison of Magnetic Clouds with Interplanetary Coronal Mass Ejections for Solar Cycle 23
DOI: 10.1007/s11207-010-9684-3 Bibcode: 2011SoPh..269..141W

Lepping, R. P.; Wu, Chin-Chun

We compare the number and characteristics of interplanetary coronal mass ejections (ICMEs) to those of magnetic clouds (MCs) by using in-situ solar wind plasma and magnetic field observations made at 1 AU during solar cycle 23. We found that ≈ 28% of ICMEs appear to contain MCs, since 103 magnetic clouds (MCs) occurred during 1995 - 2006, and 307 …

2011 Solar Physics
SOHO 56