Search Publications

SAID: A turbulent plasmaspheric boundary layer
DOI: 10.1029/2010GL042929 Bibcode: 2010GeoRL..37.7106M

Santolik, O.; Mishin, E. V.; Puhl-Quinn, P. A.

This paper presents novel features of subauroral ion drifts (SAID) observed from a unique conjunction of the Cluster, DMSP, and Polar satellites, including the discovery of SAID-related plasma waves. These observations confirm and expand on our proposed concept of the SAID channel being a turbulent boundary layer, formed via a short circuit of the…

2010 Geophysical Research Letters
Cluster 27
Breaking the σ8 m Degeneracy Using the Clustering of High-z X-ray Active Galactic Nuclei
DOI: 10.1088/2041-8205/714/2/L185 Bibcode: 2010ApJ...714L.185B

Basilakos, Spyros; Plionis, Manolis

The clustering of X-ray selected active galactic nuclei (AGNs) appears to be a valuable tool for extracting cosmological information. Using the recent high-precision angular clustering results of ~30,000 XMM-Newton soft (0.5-2 keV) X-ray sources, which have a median redshift of z ~ 1, and assuming a flat geometry, a constant in comoving coordinate…

2010 The Astrophysical Journal
XMM-Newton 27
Modeling the Enceladus plume-plasma interaction
DOI: 10.1029/2009GL041613 Bibcode: 2010GeoRL..37.3202F

Delamere, P. A.; Bagenal, F.; Fleshman, B. L.

We investigate the chemical interaction between Saturn's corotating plasma and Enceladus' volcanic plumes. We evolve a parcel of ambient plasma as it passes through a prescribed H2O plume using a physical chemistry model adapted for water-group reactions. The flow field is assumed to be that of a plasma around an electrically-conducting…

2010 Geophysical Research Letters
Cassini 27
Physical Origin of Differences Among Various Measures of Solar Meridional Circulation
DOI: 10.1088/0004-637X/722/1/774 Bibcode: 2010ApJ...722..774D

Ulrich, Roger K.; Dikpati, Mausumi; Gilman, Peter A.

We show that systematic differences between surface Doppler and magnetic element tracking measures of solar meridional flow can be explained by the effects of surface turbulent magnetic diffusion. Feature-tracking speeds are lower than plasma speeds in low and mid latitudes, because magnetic diffusion opposes poleward plasma flow in low latitudes …

2010 The Astrophysical Journal
SOHO 27
Herschel observations of EXtra-Ordinary Sources (HEXOS): detecting spiral arm clouds by CH absorption lines
DOI: 10.1051/0004-6361/201015107 Bibcode: 2010A&A...521L..14Q

Menten, K. M.; Falgarone, E.; Martin, P. G. +67 more

We have observed CH absorption lines (J = 3/2, N = 1 ≤ftarrow J = 1/2, N = 1) against the continuum source Sgr B2(M) using the Herschel/HIFI instrument. With the high spectral resolution and wide velocity coverage provided by HIFI, 31 CH absorption features with different radial velocities and line widths are detected and identified. The narrower …

2010 Astronomy and Astrophysics
Herschel 27
Water production in comet 81P/Wild 2 as determined by Herschel/HIFI
DOI: 10.1051/0004-6361/201015161 Bibcode: 2010A&A...521L..50D

Blommaert, J. A. D. L.; Küppers, M.; Thomas, N. +42 more

The high spectral resolution and sensitivity of Herschel/HIFI allows for the detection of multiple rotational water lines and accurate determinations of water production rates in comets. In this Letter we present HIFI observations of the fundamental 110-101 (557 GHz) ortho and 111-00 (1113 GHz) para rota…

2010 Astronomy and Astrophysics
Herschel 27
Dust is Forming Along the Red Giant Branch of 47 Tuc
DOI: 10.1088/0004-637X/718/1/522 Bibcode: 2010ApJ...718..522O

Dalessandro, Emanuele; Ferraro, Francesco R.; Origlia, Livia +4 more

We present additional evidence that dust is really forming along the red giant branch (RGB) of 47 Tuc at luminosities ranging from above the horizontal branch to the RGB tip. The presence of dust had been inferred from an infrared excess in the (K - 8) color, with K measured from high spatial resolution ground-based near-IR photometry and "8" refe…

2010 The Astrophysical Journal
ISO eHST 27
Cold fronts and multi-temperature structures in the core of Abell 2052
DOI: 10.1051/0004-6361/201015198 Bibcode: 2010A&A...523A..81D

Simionescu, A.; Kaastra, J. S.; de Plaa, J. +3 more

Context. The physics of the coolest phases in the hot intra-cluster medium (ICM) of clusters of galaxies is yet to be fully unveiled. X-ray cavities blown by the central active galactic nucleus (AGN) contain enough energy to heat the surrounding gas and stop cooling, but locally blobs or filaments of gas appear to be able to cool to low temperatur…

2010 Astronomy and Astrophysics
XMM-Newton 27
X-ray and multiwavelength view of NGC 4278. A LINER-Seyfert connection?
DOI: 10.1051/0004-6361/201014371 Bibcode: 2010A&A...517A..33Y

Grosso, N.; Porquet, D.; Reeves, J. N. +3 more

Context. The emission mechanism responsible for the bulk of energy from radio to X-rays in low ionization emission line regions (LINERs) and low luminosity active galactic nuclei (LLAGN) has been long debated. Based on UV to X-ray and radio to UV flux ratios, some argue that LINERs/LLAGN are a scaled-down version of their more luminous predecessor…

2010 Astronomy and Astrophysics
XMM-Newton eHST 27
An assessment of surface matching for the automated co-registration of MOLA, HRSC and HiRISE DTMs
DOI: 10.1016/j.epsl.2009.12.040 Bibcode: 2010E&PSL.294..520L

Muller, Jan-Peter; Lin, Shih-Yuan; Mills, Jon P. +1 more

Martian topographic data has been collected by various exploration missions over the last decade. These products provide detailed topographic information and are invaluable for scientists to interpret and understand the geological and climate evolution which has occurred on Mars. In order to fully utilise these multi-sensor, multi-resolution and m…

2010 Earth and Planetary Science Letters
MEx 27