Search Publications

The AKARI Deep Field-South: Spitzer 24- and 70-µm observations, catalogues and counts
DOI: 10.1111/j.1365-2966.2010.17689.x Bibcode: 2011MNRAS.411..373C

Clements, D. L.; Pearson, C.; Shirahata, M. +3 more

The AKARI Deep Field-South (ADF-S) is a ∼12 deg2 region near the South Ecliptic Pole that has been observed with deep scans in the far-infrared by the AKARI satellite. As such it is becoming one of the key extragalactic survey fields. We here present complementary observations of the ADF-S conducted by the Spitzer Space Telescope at wav…

2011 Monthly Notices of the Royal Astronomical Society
AKARI 25
Fast tailward flows in the plasma sheet boundary layer during a substorm on 9 March 2008: THEMIS observations
DOI: 10.1029/2010JA015969 Bibcode: 2011JGRA..116.3216D

Zhang, T. L.; Glassmeier, K. -H.; Nakamura, R. +12 more

Tailward flows in the plasma sheet boundary layer (PSBL) were observed simultaneously by the five Time History of Events and Macroscale Interactions during Substorms (THEMIS) probes at down-tail distances X ∼ 7.6 to ∼17.6 RE for ∼10 min during an interval of successive substorm intensification in a storm time on 9 March 2008. The flows …

2011 Journal of Geophysical Research (Space Physics)
Cluster 25
Particle Acceleration and Propagation in Strong Flares without Major Solar Energetic Particle Events
DOI: 10.1007/s11207-011-9710-0 Bibcode: 2011SoPh..269..309K

Klein, K. -L.; Malandraki, O.; Trottet, G. +1 more

Solar energetic particles (SEPs) detected in space are statistically associated with flares and coronal mass ejections (CMEs). But it is not clear how these processes actually contribute to the acceleration and transport of the particles. The present work addresses the question why flares accompanied by intense soft X-ray bursts may not produce SE…

2011 Solar Physics
SOHO 25
One-dimensional Modeling for Temperature-dependent Upflow in the Dimming Region Observed by Hinode/EUV Imaging Spectrometer
DOI: 10.1088/0004-637X/743/1/57 Bibcode: 2011ApJ...743...57I

Shimizu, T.; Hara, H.; Watanabe, T. +4 more

We previously found a temperature-dependent upflow in the dimming region following a coronal mass ejection observed by the Hinode EUV Imaging Spectrometer (EIS). In this paper, we reanalyzed the observations along with previous work on this event and provided boundary conditions for modeling. We found that the intensity in the dimming region drama…

2011 The Astrophysical Journal
Hinode SOHO 25
Broad iron emission lines in Seyfert galaxies - re-condensation of gas onto an inner disk below the ADAF?
DOI: 10.1051/0004-6361/201015478 Bibcode: 2011A&A...527A.127M

Meyer, F.; Meyer-Hofmeister, E.

Context. The number of strong iron Kα line detections in Seyfert AGN is clearly growing in the Chandra, XMM-Newton and Suzaku era. The iron emission lines are broad, some are relativistically blurred. These relativistic disk lines have also been observed for galactic black hole X-ray binaries. Thermal components found in hard spectra we…

2011 Astronomy and Astrophysics
Suzaku 25
Enhancement of Terrestrial Diffuse X-Ray Emission Associated with Coronal Mass Ejection and Geomagnetic Storm
DOI: 10.1093/pasj/63.sp3.S691 Bibcode: 2011PASJ...63S.691E

Miyoshi, Yoshizumi; Ezoe, Yuichiro; Ohashi, Takaya +4 more

We present an analysis of a Suzaku observations taken during the geomagnetic storm of 2005 August 23-24. We found a time variation of diffuse soft X-ray emission when a coronal mass ejection hit Earth and caused a geomagnetic storm. The diffuse emission consisted of fluorescent scattering of solar X-rays and an exospheric solar wind charge exchang…

2011 Publications of the Astronomical Society of Japan
Suzaku 25
Testing a Scale-independent Method to Measure the Mass of Black Holes
DOI: 10.1088/0004-637X/735/1/16 Bibcode: 2011ApJ...735...16G

Titarchuk, L.; Satyapal, S.; Gliozzi, M. +2 more

Estimating the black hole mass at the center of galaxies is a fundamental step not only for understanding the physics of accretion, but also for the cosmological evolution of galaxies. Recently, a new method, based solely on X-ray data, was successfully applied to determine the black hole mass in Galactic systems. Since X-rays are thought to be pr…

2011 The Astrophysical Journal
XMM-Newton 25
Resolution of the lunar hydrogen enigma
DOI: 10.1029/2011GL046688 Bibcode: 2011GeoRL..38.6201H

Hodges, R. R.

The recent discovery, by instruments on the IBEX and Chandrayaan-1 spacecraft, of significant fluxes of energetic hydrogen atoms escaping from the moon suggests that there are flaws in the common wisdom regarding the interaction of solar wind with lunar regolith that have prevailed in attempts to explain the failure of the Apollo 17 far-ultraviole…

2011 Geophysical Research Letters
Chandrayaan-1 25
Geomorphologic mapping of the Menrva region of Titan using Cassini RADAR data
DOI: 10.1016/j.icarus.2011.01.014 Bibcode: 2011Icar..212..744W

Lopes, Rosaly M. C.; Williams, David A.; Radebaugh, Jani +1 more

We made a detailed geomorphologic map of the Menrva region of Titan, using Cassini RADAR data as our map base. Using similar techniques and approaches that were applied to mapping Magellan radar images of Venus, and earlier, more generalized Titan maps, we were able to define and characterize 10 radar morphologic units, along with inferred dunes a…

2011 Icarus
Cassini 25
Suzaku Observation of the Intermediate Polar V1223 Sagittarii
DOI: 10.1093/pasj/63.sp3.S739 Bibcode: 2011PASJ...63S.739H

Ishida, Manabu; Hayashi, Takayuki; Terada, Yukikatsu +2 more

We report on the Suzaku observation of the intermediate polar V1223 Sagittarii. Using a multi-temperature plasma emission model with its reflection from a cold matter, we obtained the shock temperature to be 37.9 $^{+5.1}_{-4.6}\ $ keV. This constrains the mass and the…

2011 Publications of the Astronomical Society of Japan
Suzaku 25