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A novel principle for an ion mirror design in time-of-flight mass spectrometry
DOI: 10.1016/j.ijms.2006.01.025 Bibcode: 2006IJMSp.251...73S

Wurz, P.; Altwegg, K.; Balsiger, H. +7 more

A novel design for a gridless two-stage ion mirror, or reflectron, for time-of-flight mass spectrometry (TOFMS) will be presented. The development of this novel design was driven by the stringent engineering requirements for the ion mirror's utilization by the reflectron time-of-flight (RTOF) sensor in the Rosetta orbiter spectrometer for ion and …

2006 International Journal of Mass Spectrometry
Rosetta 34
INTEGRAL and RXTE Observations of Centaurus A
DOI: 10.1086/500534 Bibcode: 2006ApJ...641..801R

Rothschild, Richard E.; Staubert, Rüdiger; Wilms, Jörn +6 more

INTEGRAL and RXTE performed three simultaneous observations of the nearby radio galaxy Centaurus A in 2003 March, 2004 January, and 2004 February with the goals of investigating the geometry and emission processes via the spectral/temporal variability of the X-ray/low-energy gamma-ray flux, and intercalibration of the INTEGRAL instruments with res…

2006 The Astrophysical Journal
INTEGRAL 34
The ISO 170 µm luminosity function of galaxies
DOI: 10.1051/0004-6361:20054272 Bibcode: 2006A&A...448..525T

Dole, H.; Lagache, G.; Puget, J. -L. +3 more

We constructed a local luminosity function (LF) of galaxies using a flux-limited sample (S170 ≥ 0.195~Jy) of 55 galaxies at z < 0.3 taken from the <sl>ISO</sl> FIRBACK survey at 170 µm. The overall shape of the 170-µm LF is found to be different from that of the total 60-µm LF (Takeuchi et al. 2003): the…

2006 Astronomy and Astrophysics
ISO 34
Stratification in the broad line region of AGN: The two-component model
DOI: 10.1016/j.newar.2006.06.015 Bibcode: 2006NewAR..50..716B

Bon, E.; Popović, L. Č.; Ilić, D. +1 more

Here we present our investigation of the kinematic structure of the broad emission line region (BLR) in a sample of 14 single-peaked Active Galactic Nuclei (AGN), which have been previously observed in the X-ray (Fe Kα line) and where, according to the X-ray emission, a disk geometry is expected. To explain the BLR complex structure we apply a two…

2006 New Astronomy Reviews
eHST 34
Plasma intrusion above Mars crustal fields—Mars Express ASPERA-3 observations
DOI: 10.1016/j.icarus.2005.11.016 Bibcode: 2006Icar..182..406F

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

Using data of the ASPERA-3 instrument on board the European Mars Express spacecraft we investigate the effect of the martian crustal fields on electrons intruding from the magnetosheath. For the crustal field strength we use published data obtained by the Mars Global Surveyor MAG/ER instrument for a fixed altitude of 400 km. We use statistics on 1…

2006 Icarus
MEx 34
Capella Corona Revisited: A Combined View from XMM-Newton RGS and Chandra HETGS and LETGS
DOI: 10.1086/506602 Bibcode: 2006ApJ...649..979G

Sako, M.; Kahn, S. M.; Gupta, R. +2 more

We present a combined analysis of the X-ray emission of the Capella corona obtained with XMM-Newton RGS and Chandra HETGS and LETGS. An improved atomic line database and a new differential emission measure (DEM) deconvolution method are developed for this purpose. Our new atomic database is based on the Astrophysical Plasma Emission Database and i…

2006 The Astrophysical Journal
XMM-Newton 34
Long-lived Solar Neutron Emission in Comparison with Electron-produced Radiation in the 2005 September 7 Solar Flare
DOI: 10.1086/509145 Bibcode: 2006ApJ...651L..69S

Tanaka, Y. T.; Yoshikawa, I.; Mukai, T. +23 more

Strong signals of neutral emissions were detected in association with a solar flare that occurred on 2005 September 7. They were produced by both relativistic ions and electrons. In particular, relativistic neutrons were observed with the solar neutron telescopes (SNTs) located at Mount Chacaltaya in Bolivia and Mount Sierra Negra in Mexico and wi…

2006 The Astrophysical Journal
INTEGRAL 34
Winds on Titan from ground-based tracking of the Huygens probe
DOI: 10.1029/2005JE002649 Bibcode: 2006JGRE..111.7S02F

Plettemeier, D.; Bird, M. K.; Asmar, S. W. +14 more

Large radio telescopes on Earth tracked the radio signal transmitted by the Huygens probe during its mission at Titan. Frequency measurements were conducted as a part of the Huygens Doppler Wind Experiment (DWE) in order to derive the velocity of the probe in the direction to Earth. The DWE instrumentation on board Huygens consisted of an ultrasta…

2006 Journal of Geophysical Research (Planets)
Huygens 34
Cassini thermal observations of Saturn's main rings: Implications for particle rotation and vertical mixing
DOI: 10.1016/j.pss.2006.05.033 Bibcode: 2006P&SS...54.1167S

Altobelli, Nicolas; Michael Flasar, F.; Cuzzi, Jeffrey N. +9 more

In late 2004 and 2005 the Cassini composite infrared spectrometer (CIRS) obtained spatially resolved thermal infrared radial scans of Saturn's main rings (A, B and C, and Cassini Division) that show ring temperatures decreasing with increasing solar phase angle, α, on both the lit and unlit faces of the ring plane. These temperature differences su…

2006 Planetary and Space Science
Cassini 34
A Quantitative Study on Magnetic Configuration for Active Regions
DOI: 10.1007/s11207-006-2081-2 Bibcode: 2006SoPh..237...25G

Guo, Juan; Zhang, Hongqi; Chumak, Oleg V. +1 more

As compared with the Mount Wilson Magnetic Classification (MWMC), effective distance (dE) is a useful parameter because it gives a quantitative measure of magnetic configuration in active regions. We have analyzed magnetograms of 24 active regions of different types with MWMC. We have studied the evolution of magnetic fields of five act…

2006 Solar Physics
SOHO 34