Search Publications

Identification of a new outflow channel on Mars in Syrtis Major Planum using HRSC/MEx data
DOI: 10.1016/j.pss.2008.01.011 Bibcode: 2008P&SS...56.1030M

Mangold, N.; Neukum, G.; Hiesinger, H. +6 more

Syrtis Major Planum is a volcanic plain dominated by lava flows. High resolution stereo camera (HRSC) images of the northern Syrtis Major region display erosional features such as grooves, teardrop-shaped islands and valleys. These landforms are characteristics of outflow channels seen on Mars, therefore implying that a flood event took place in t…

2008 Planetary and Space Science
MEx 27
Hubble Space Telescope Near-infrared Snapshot Survey of 3CR Radio Source Counterparts. II. An Atlas and Inventory of the Host Galaxies, Mergers, and Companions
DOI: 10.1086/587622 Bibcode: 2008ApJS..177..148F

O'Dea, Christopher P.; Baum, Stefi; Chiaberge, Marco +10 more

We present the second part of an H-band (1.6 µm) "atlas" of z < 0.3 3CR radio galaxies, using the Hubble Space Telescope Near Infrared Camera and Multi-Object Spectrometer (HST NICMOS2). We present new imaging for 21 recently acquired sources and host galaxy modeling for the full sample of 101 (including 11 archival)—an 87% completion rat…

2008 The Astrophysical Journal Supplement Series
eHST 27
A nanoflare model for active region radiance: application of artificial neural networks
DOI: 10.1051/0004-6361:200810911 Bibcode: 2008A&A...492L..13B

Solanki, S. K.; Innes, D. E.; Safari, H. +2 more

Context: Nanoflares are small impulsive bursts of energy that blend with and possibly make up much of the solar background emission. Determining their frequency and energy input is central to understanding the heating of the solar corona. One method is to extrapolate the energy frequency distribution of larger individually observed flares to lower…

2008 Astronomy and Astrophysics
SOHO 27
Thermal observations of Saturn's main rings by Cassini CIRS: Phase, emission and solar elevation dependence
DOI: 10.1016/j.pss.2007.05.029 Bibcode: 2008P&SS...56..134A

Altobelli, Nicolas; Spilker, Linda J.; Leyrat, Cedric +1 more

Two and a half years after Saturn orbit insertion (SOI) the Cassini composite infrared spectrometer (CIRS) has acquired an extensive set of thermal measurements (including physical temperature and filling factor) of Saturn's main rings for a number of different viewing geometries, most of which are not available from Earth. Thermal mapping of both…

2008 Planetary and Space Science
Cassini 27
Effect of a northward turning of the interplanetary magnetic field on cusp precipitation as observed by Cluster
DOI: 10.1029/2007JA012771 Bibcode: 2008JGRA..113.7S13E

Berchem, J.; Escoubet, C. P.; Pitout, F. +10 more

The immediate effect of the rotation of the interplanetary magnetic field (IMF) from southward to northward on cusp precipitation has been rarely observed by a polar orbiting satellite in the past. The four Cluster spacecraft observed such an event on 23 September 2004 as they were crossing the polar cusp within 2-16 min from each other. Between t…

2008 Journal of Geophysical Research (Space Physics)
Cluster 27
DN Bootis: A low mass-ratio W UMa-type contact binary
DOI: 10.1016/j.newast.2008.01.001 Bibcode: 2008NewA...13..468S

Selam, S. O.; Özavcı, İ.; Nelson, R. H. +2 more

New photoelectric BVR light curves and radial velocity curves were obtained for the HIPPARCOS discovery DN Boo at the TÜBİTAK National Observatory of Turkey (TUG) and Dominion Astrophysical Observatory (DAO), respectively, to determine physical nature of the variable. The character of the obtained light curves and double-lined spectroscopic struct…

2008 New Astronomy
Hipparcos 27
Suzaku Observation of the TeV Blazar 1ES 1218+304: Clues on Particle Acceleration in an Extreme TeV Blazar
DOI: 10.1086/589689 Bibcode: 2008ApJ...680L...9S

Kataoka, J.; Madejski, G. M.; Sato, R. +3 more

We observed the TeV blazar 1ES 1218+304 with the X-ray astronomy satellite Suzaku in 2006 May. At the beginning of the 2 day continuous observation, we detected a large flare in which the 5-10 keV flux changed by a factor of ~2 on a timescale of 5 × 104 s. During the flare, the increase in the hard X-ray flux clearly lagged behind that …

2008 The Astrophysical Journal
Suzaku 27
Positron astronomy with SPI/INTEGRAL
DOI: 10.1016/j.newar.2008.06.019 Bibcode: 2008NewAR..52..454W

Knödlseder, J.; Schanne, S.; Cordier, B. +7 more

We provide an overview of positron astronomy results that have been obtained using the INTEGRAL spectrometer SPI, and discuss their implications for the still mysterious origin of positrons in our Galaxy. It has long been known that the 511 keV positron annihilation emission is strongest from the central region of our Galaxy. Recently, it has been…

2008 New Astronomy Reviews
INTEGRAL 27
Survey of ELF-VLF plasma waves in outer radiation belt observed by Cluster STAFF-SA experiment
DOI: 10.5194/angeo-26-3269-2008 Bibcode: 2008AnGeo..26.3269P

Cornilleau-Wehrlin, N.; Pokhotelov, D.; Lefeuvre, F. +1 more

Various types of plasma waves have profound effects on acceleration and scattering of radiation belt particles. For the purposes of radiation belt modeling it is necessary to know statistical distributions of plasma wave parameters. This paper analyzes four years of plasma wave observations in the Earth's outer radiation belt obtained by the STAFF…

2008 Annales Geophysicae
Cluster 27
Neon and oxygen in low activity stars: towards a coronal unification with the Sun
DOI: 10.1051/0004-6361:200809690 Bibcode: 2008A&A...486..995R

Schmitt, J. H. M. M.; Robrade, J.; Favata, F.

Aims: The disagreement between helioseismology and a recent downward revision of solar abundances has resulted in a controversy about the true neon abundance of the Sun and other stars. We study the coronal Ne/O abundance ratios of nearby stars with modest activity levels and investigate a possible peculiarity of the Sun among the stellar populati…

2008 Astronomy and Astrophysics
XMM-Newton 27