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AKARI (ASTRO-F): Flight performance and preliminary results
DOI: 10.1016/j.asr.2007.03.073 Bibcode: 2007AdSpR..40..595S

Shibai, Hiroshi

ASTRO-F, which is the first Japanese satellite mission dedicated to the infrared wavelength region, was successfully launched on February 21, 2006 (UT), and was named "AKARI". The telescope has a 69 cm aperture, and is cooled to 6 K with super-fluid helium and mechanical coolers. AKARI is designed for the most advanced all-sky survey in the mid- a…

2007 Advances in Space Research
AKARI 7
Total Solar Irradiance and the Fe XIV Corona
DOI: 10.1007/s11207-007-0248-0 Bibcode: 2007SoPh..241..269M

Rušin, Vojtech; Minarovjech, Milan; Saniga, Metod

Analyzing daily values of the total solar irradiance (TSI), the coronal index of solar activity (CI), and the Mg II 280-nm core-to-wing ratio (Mg II index), we have found that the temporal variations of these indices are very similar to each other during the period from 1978 to 2005. The correlation between CI and TSI, with the PSI correction lyin…

2007 Solar Physics
SOHO 7
Albedo and photometric study of Mars with the Planetary Fourier Spectrometer on-board the Mars Express mission
DOI: 10.1016/j.icarus.2006.08.028 Bibcode: 2007Icar..186..527E

Colangeli, L.; Formisano, V.; Palomba, E. +3 more

The Short Wavelength Channel of the Planetary Fourier Spectrometer (PFS) covers the 8333-1750 cm-1 (1.2-5.7 µm) spectral range, that is well suited to study the reflectance properties of the martian soil. These properties vary with time due to the dust dynamics in the martian environment. Wind can blow off dust exposing soil and f…

2007 Icarus
MEx 7
Effects of Dispersion of Wave Packets in the Determination of Lifetimes of High-Degree Solar p Modes from Time Distance Analysis: MDI Data
DOI: 10.1007/s11207-007-0324-5 Bibcode: 2007SoPh..241....7C

Chou, Dean-Yi; Ladenkov, Oleg

The cross-correlation function of solar p modes in a time - distance analysis changes with travel distance (or travel time). The exponential decrease in the amplitude of the cross-correlation function with travel distance has been interpreted as the dissipation of solar p-mode power and used to determine the lifetimes of high-degree p modes. It is…

2007 Solar Physics
SOHO 7
PSR J1119–6127 and the X-ray emission from high magnetic field radio pulsars
DOI: 10.1007/s10509-007-9305-2 Bibcode: 2007Ap&SS.308...89G

Camilo, F.; Gaensler, B. M.; Gonzalez, M. E. +2 more

The existence of radio pulsars having inferred magnetic fields in the magnetar regime suggests that possible transition objects could be found in the radio pulsar population. The discovery of such an object would contribute greatly to our understanding of neutron star physics. Here we report on unusual X-ray emission detected from the radio pulsar…

2007 Astrophysics and Space Science
XMM-Newton 7
Morphological Study of Quiescent Streamers during Solar Minimum by Ultraviolet Emission Lines
DOI: 10.1086/521386 Bibcode: 2007ApJ...668.1196A

Akinari, Nakagawa

We perform, by utilizing spectroscopic measurements made with SOHO/UVCS, a morphological characterization of the quiescent streamer during solar minimum, by means of both a comprehensive survey of daily synoptic observations over 33 weeks from 1996 April to November and detailed analysis of several specialized observations targeting quiescent stre…

2007 The Astrophysical Journal
SOHO 7
A three-dimensional kinetic-fluid numerical code to study the equilibrium structure of the magnetotail: The role of electrons in the formation of the bifurcated current sheet
DOI: 10.1029/2007JA012394 Bibcode: 2007JGRA..112.6218G

Veltri, P.; Zimbardo, G.; Greco, A. +1 more

In this work we present a new stationary three-dimensional kinetic-fluid code with ions represented by particles and electrons by a massless fluid. The magnetotail current sheet is modeled as a magnetic field reversal with a normal magnetic field component Bn. A cross tail electric field Ey is included. An ion test particle s…

2007 Journal of Geophysical Research (Space Physics)
Cluster 7
Sulfur Abundance in the Slow Solar Wind
DOI: 10.1086/523597 Bibcode: 2007AJ....134.2451G

Wurz, P.; Ipavich, F. M.; Opitz, A. +2 more

Using 4 years of data from the Mass Time-of-Flight and Proton Monitor, two CELIAS sensors on board SOHO, we report the sulfur abundances in comparison to magnesium and calcium (two low first ionization potential elements) for the slow solar wind, and for the first time we measure the sulfur isotopic abundance ratio. For the period in which the pro…

2007 The Astronomical Journal
SOHO 7
An X-ray survey in SA 57 with XMM-Newton
DOI: 10.1051/0004-6361:20077359 Bibcode: 2007A&A...469.1211T

Fiore, F.; Puccetti, S.; Trevese, D. +3 more

Context: The maximum number density of Active Galactic Nuclei (AGNs), as deduced from X-ray studies, occurs at z ⪉ 1, with lower luminosity objects peaking at smaller redshifts. Optical studies lead to a different evolutionary behaviour, with a number density peaking at z ≈ 2 independently of the intrinsic luminosity, but this result is limited to…

2007 Astronomy and Astrophysics
XMM-Newton 7
Conversations on the Habitability of Worlds: The Importance of Volatiles
DOI: 10.1007/s11214-007-9193-3 Bibcode: 2007SSRv..129..123B

Bertaux, J. -L.; Carr, M.; Gaidos, E. +1 more

Our scientific forefathers discuss the interrelationships between water, climate, the atmosphere, and life on Earth and other terrestrial planets at a workshop in Nichtchâtel, Switzerland.

2007 Space Science Reviews
MEx 7