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Instabilities driven by ion shell distributions observed by Cluster in the midaltitude plasma sheet boundary layer
Fazakerley, A. N.; Marchaudon, A.; Cornilleau-Wehrlin, N. +5 more
Cluster observations in the near-Earth plasma sheet boundary layer (PSBL) region have shown the presence of ion shell distributions related to velocity-dispersed ion structures (VDIS) coincident with electrostatic emissions. We have examined ion shell instabilities in the presence of a cold ion and electron background using linear theory and parti…
On the Nature of the Hard X-Ray Source IGR J2018+4043
Kennea, J. A.; Terrier, R.; Rauw, G. +13 more
We found a very likely counterpart to the recently discovered hard X-ray source IGR J2018+4043 in the multiwavelength observations of the source field. The source, originally discovered in the 20-40 keV band, is now confidently detected also in the 40-80 keV band, with a flux of (1.4+/-0.4)×10-11 ergs cm-2 s-1. A 5…
Energisation of O+ and O+ 2 Ions at Mars: An Analysis of a 3-D Quasi-Neutral Hybrid Model Simulation
Kallio, E.; Fedorov, A.; Janhunen, P. +12 more
We have studied the loss of O+ and O+2 ions at Mars with a numerical model. In our quasi-neutral hybrid model ions (H+, He++, O+, O+2) are treated as particles while electrons form a massless charge-neutralising fluid. The employed model version does not includ…
A Blue Straggler Binary with Three Progenitors in the Core of a Globular Cluster?
Knigge, C.; Long, K. S.; Gilliland, R. L. +3 more
We show that the X-ray source W31 in the core of the globular cluster 47 Tucanae is physically associated with the bright blue straggler BSS 7. The two sources are astrometrically matched to 0.061", with a chance coincidence probability of less than 1%. We then analyze optical time-series photometry obtained with the Hubble Space Telescope (HST) a…
Short-term changes in the belt/zone structure of Saturn's Southern Hemisphere (1996-2004)
Sánchez-Lavega, A.; Pérez-Hoyos, S.; French, R. G.
Aims.The main goal of this paper is to study the reflectivity changes that affect Saturn's global belt/zone pattern on time-scales from weeks to a few months, and to determine their frequency and intensity, as well as the variations of the vertical cloud structure that cause such changes.
Methods: .We have used 177 images from Hubble Space Tel…
The dark clump near Abell 1942: dark matter halo or statistical fluke?
Castander, F. J.; von der Linden, A.; Schneider, P. +1 more
Using HST WFPC2 mosaic imaging, deep Chandra observations, and the
original CFHT imaging, we investigate the case for the dark clump candidate originally presented by (Erben et al. 2000, A&A, 355, 23). We show that the original detection is well reproducible in the CFHT data, and can confirm the presence of an alignment signal at the dark…X-Ray Pulsations in the Supersoft X-Ray Binary CAL 83
Cowley, A. P.; Schmidtke, P. C.
Chandra and XMM-Newton X-ray data reveal that the supersoft X-ray binary CAL 83 exhibits 38.4 minute pulsations at some epochs. These X-ray variations are similar to those found in some novae and are likely to be caused by nonradial pulsations of the white dwarf. This is the first detection of pulsations in a classical supersoft X-ray binary.
New upper limits for hydrogen halides on Saturn derived from Cassini-CIRS data
Fletcher, L. N.; Irwin, P. G. J.; Teanby, N. A. +2 more
Far infrared spectra (10-600 cm -1) from Cassini's Composite InfraRed Spectrometer (CIRS) were used to determine improved upper limits of hydrogen halides HF, HCl, HBr, and HI in Saturn's atmosphere. Three observations, comprising a total of 3088 spectra, gave 3 σ upper limits on HF, HCl, HBr, and HI volume mole fractions of 8.0×10, 6.7…
Mars 1064 nm spectral radiance measurements determined from the receiver noise response of the Mars Orbiter Laser Altimeter
Zuber, Maria T.; Sun, Xiaoli; Neumann, Gregory A. +1 more
A technique was developed to compute the radiance of the scene viewed by the optical receiver of the Mars Orbiter Laser Altimeter. The technique used the detection threshold and the false detection rate of the receiver to provide a passive radiometry measurement of Mars at the 1064 nm wavelength over a 2 nm bandwidth and subkilometer spatial resol…
EIT and TRACE responses to flare plasma
Mason, H. E.; Del Zanna, G.; Tripathi, D. +1 more
Aims.To understand the contribution of active region and flare plasmas to the λ195 channels of SOHO/EIT (Extreme-ultraviolet Imaging Telescope) and TRACE (Transition Region and Coronal Explorer).
Methods: .We have analysed an M8 flare simultaneously observed by the Coronal Diagnostic Spectrometer (CDS), EIT, TRACE and RHESSI. We obtained synth…