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Structure and dynamics of a new class of thin current sheets
DOI: 10.1029/2005JA011517 Bibcode: 2006JGRA..111.8204S

Sitnov, M. I.; Runov, A.; Swisdak, M. +1 more

New results on a steady state Vlasov theory of current sheets, which generalizes the Harris (1962) model by assuming anisotropic and nongyrotropic plasmas and using the invariant of particle motion in regions of strong gradients, are presented with the aim to explain multiprobe observations of thin current sheets in the geomagnetotail and laborato…

2006 Journal of Geophysical Research (Space Physics)
Cluster 80
Properties of Flares-Generated Seismic Waves on the Sun
DOI: 10.1007/s11207-006-0190-6 Bibcode: 2006SoPh..238....1K

Kosovichev, A. G.

The helioseismic waves excited by solar flares ("sunquakes") are observed as circular, expanding waves on the Sun's surface. The first sunquake was observed for a flare on July 9, 1996, by the Solar and Heliospheric Observatory (SOHO) space mission. This paper presents results of new observations and a detailed qualitative analysis of the basic pr…

2006 Solar Physics
SOHO 80
An Overdensity of Galaxies near the Most Distant Radio-loud Quasar
DOI: 10.1086/500167 Bibcode: 2006ApJ...640..574Z

Ford, H. C.; Demarco, R.; Infante, L. +41 more

A 5 arcmin2 region around the luminous radio-loud quasar SDSS J0836+0054 (z=5.8) hosts a wealth of associated galaxies, characterized by very red (1.3<i775-z850<2.0) color. The surface density of these z~5.8 candidates is approximately 6 times higher than the number expected from deep ACS fields. This is one …

2006 The Astrophysical Journal
eHST 80
Magnetic Causes of Solar Coronal Mass Ejections: Dominance of the Free Magnetic Energy over the Magnetic Twist Alone
DOI: 10.1086/503699 Bibcode: 2006ApJ...644.1258F

Falconer, D. A.; Moore, R. L.; Gary, G. A.

We examine the magnetic causes of coronal mass ejections (CMEs) by examining, along with the correlations of active-region magnetic measures with each other, the correlations of these measures with active-region CME productivity observed in time windows of a few days, either centered on or extending forward from the day of the magnetic measurement…

2006 The Astrophysical Journal
SOHO 80
The Second Ring-Moon System of Uranus: Discovery and Dynamics
DOI: 10.1126/science.1122882 Bibcode: 2006Sci...311..973S

Showalter, Mark R.; Lissauer, Jack J.

Deep exposures of Uranus taken with the Hubble Space Telescope reveal two small moons and two faint rings. All of them orbit outside of Uranus's previously known (main) ring system but are interior to the large, classical moons. The outer new moon, U XXVI Mab, orbits at roughly twice the radius of the main rings and shares its orbit with a dust ri…

2006 Science
eHST 79
Ion composition and pressure changes in storm time and nonstorm substorms in the vicinity of the near-Earth neutral line
DOI: 10.1029/2006JA011939 Bibcode: 2006JGRA..11111222K

Lundin, R.; Dandouras, I.; Lucek, E. +9 more

Using CLUSTER/CODIF data from close to ∼19 Re in the magnetotail, we have performed a superposed epoch analysis of storm time and nonstorm substorms to determine how the ion composition changes during a substorm. We find that the median O+ density and pressure in the plasma sheet are a factor of 5 higher during storm times than during n…

2006 Journal of Geophysical Research (Space Physics)
Cluster 79
A Galactic Origin for the Local Ionized X-Ray Absorbers
DOI: 10.1086/500310 Bibcode: 2006ApJ...644..174F

Canizares, Claude R.; Wolfire, Mark; Fang, Taotao +1 more

Recent Chandra and XMM-Newton observations of distant quasars have shown strong local (z~0) X-ray absorption lines from highly ionized gas, primarily He-like oxygen. The nature of these X-ray absorbers, i.e., whether they are part of the hot gas associated with the Milky Way or part of the intragroup medium in the Local Group, remains a puzzle due…

2006 The Astrophysical Journal
XMM-Newton 79
Structure of the martian wake
DOI: 10.1016/j.icarus.2005.09.021 Bibcode: 2006Icar..182..329F

Coates, A. J.; Kallio, E.; Fedorov, A. +42 more

We present the first results from the ion mass analyzer IMA of the ASPERA-3 instrument on-board of Mars Express. More than 200 orbits for May 2004-September 2004 time interval have been selected for the statistical study of the distribution of the atmospheric origin ions in the planetary wake. This study shows that the martian magnetotail consists…

2006 Icarus
MEx 79
A combined re-analysis of existing blank-field SCUBA surveys: comparative 850-µm source lists, combined number counts, and evidence for strong clustering of the bright submillimetre galaxy population on arcminute scales
DOI: 10.1111/j.1365-2966.2006.10478.x Bibcode: 2006MNRAS.370.1057S

Dunlop, J. S.; Serjeant, S.; Scott, S. E.

Since the advent of Submillimetre Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope (JCMT), a series of complementary surveys has resolved the bulk of the far-infrared extragalactic background into discrete sources. This has revealed a population of heavily dust-obscured sources at high redshift (z > 1) undergoing an inte…

2006 Monthly Notices of the Royal Astronomical Society
eHST 79
XMM-Newton Observations of Four Millisecond Pulsars
DOI: 10.1086/449308 Bibcode: 2006ApJ...638..951Z

Zavlin, Vyacheslav E.

I present an analysis of the XMM-Newton observations of four millisecond pulsars, J0437-4715, J2124-3358, J1024-0719, and J0034-0534. The new data provide strong evidence of thermal emission in the X-ray flux detected from the first three objects. This thermal component is best interpreted as radiation from pulsar polar caps covered with a nonmagn…

2006 The Astrophysical Journal
XMM-Newton 79