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Fast solar wind after the rapid acceleration
DOI: 10.1029/2003JA010247 Bibcode: 2004JGRA..109.4103K

Breen, A. R.; Tokumaru, M.; Hayashi, K. +3 more

We have studied the radial dependence of the velocity of high-latitude fast solar wind in the heliocentric distance range of 0.13-0.9 AU. For this study a new tomographic analysis method which can evaluate uncertainties was developed to obtain velocity distribution maps on two reference spheres at 0.13 and 0.3 AU using interplanetary scintillation…

2004 Journal of Geophysical Research (Space Physics)
SOHO Ulysses 18
Cluster observations of velocity space-restricted ion distributions near the plasma sheet
DOI: 10.1029/2004GL020265 Bibcode: 2004GeoRL..3124802W

Lundin, R.; Sauvaud, J. -A.; Dandouras, I. +15 more

We present Cluster ion observations obtained at 18 RE in the magnetotail on 1 October 2001. According to a recent analysis, the quartet encountered a reconnection region and a tailward-moving neutral line. We examine in detail selected 3-D ion distributions, which through much of the hour following 0925 UT were non-gyrotropic. B-perpend…

2004 Geophysical Research Letters
Cluster 18
XMM-Newton observations of two X-ray-bright galaxy groups - pushing out to r500
DOI: 10.1111/j.1365-2966.2004.07544.x Bibcode: 2004MNRAS.349..722R

Ponman, T. J.; Rasmussen, J.

We report on the results of XMM-Newton observations of the z= 0.18 galaxy group WARPJ0943.7+1644 and the nearby poor cluster WARPJ0943.5+1640 at z= 0.256. Tracing the X-ray gas out to ~425 and ~500 h-1 kpc in the two systems, corresponding to roughly 70 per cent of the estimated virial radii, we find the surface-brightness profile of bo…

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton 18
Prominence atlas in the SUMER range 800 1250 Å: I. Observations, data reduction and preliminary results
DOI: 10.1023/B:sola.0000023444.58697.e7 Bibcode: 2004SoPh..220...61P

Vial, J. -C.; Parenti, S.; Lemaire, P.

The aim of this work is to build an EUV-UV spectral catalogue of a prominence. Here we focus on the preparatory work for the final result and we give an example of the results obtained. As a first step, we present the information needed for a full understanding of the results that will form the final entire catalogue. The data are composed of a fu…

2004 Solar Physics
SOHO 17
The microscope for Beagle 2
DOI: 10.1016/j.pss.2004.02.008 Bibcode: 2004P&SS...52..853T

Keller, H. U.; Hviid, S. F.; Thomas, N. +13 more

The microscope for the Beagle 2 lander, which was launched as part of the European Space Agency's Mars Express mission on 2 June 2003, will provide images of the Martian surface at around 6 µm resolution. It will provide optical images of the surface of Mars at a resolution 5 times higher than any other experiment currently planned. The devi…

2004 Planetary and Space Science
MEx 17
Transient reconnection in the cusp during strongly negative IMF By
DOI: 10.1029/2003JA009908 Bibcode: 2004JGRA..109.4204K

Farrugia, C. J.; Buchert, S.; Khotyaintsev, Y. +6 more

We investigate transient magnetic reconnection (flux transfer events, FTEs) in the cusp and its ionospheric signatures. We present in situ observations by the Polar spacecraft of multiple impulsive plasma injections and related magnetopause crossings in the outer stagnant cusp of the northern hemisphere. At this time the interplanetary magnetic fi…

2004 Journal of Geophysical Research (Space Physics)
Cluster 17
Prediction performance of space weather forecast centers following the extreme events of October and November 2003
DOI: 10.1029/2004SW000076 Bibcode: 2004SpWea...2.8001O

Oler, Cary

A review and analysis of the five strongest interplanetary coronal mass ejection (ICME) events of late October and early November 2003 (the strongest events of the "Halloween" epoch) are studied with respect to the prediction performance of five space weather forecast centers. Accurate time-of-arrival predictions and rapid responses to the upstrea…

2004 Space Weather
SOHO 17
Searching for radiative pumping lines of OH masers: II. The 53.3 µm absorption line towards 1612 MHz OH maser sources
DOI: 10.1016/j.newast.2004.03.002 Bibcode: 2004NewA....9..545H

Chen, P. S.; He, J. H.

This is the second paper in a series aiming at searching for infrared pumping lines for galactic 1612 MHz OH masers. Our paper I is devoted to the 34.6 µm absorption lines in ISO SWS spectra towards a large sample of galactic OH/IR sources. This paper analyzes the 53.3 µm line in the ISO LWS spectra towards a similar sample of OH/IR so…

2004 New Astronomy
ISO 17
Chromospheric Oscillations in an Equatorial Coronal Hole
DOI: 10.1086/422748 Bibcode: 2004ApJ...609L..95M

McIntosh, Scott W.; Tarbell, Theodore D.; Fleck, Bernhard

We report phase-difference and travel-time analyses of propagating chromospheric oscillations in and around an equatorial coronal hole as observed by TRACE. Our results suggest a significant change in atmospheric conditions at the base of the chromosphere inside the coronal hole relative to its boundary and quiet-Sun regions.

2004 The Astrophysical Journal
SOHO 17
Proper Motion and Kinematics of the Ansae in NGC 7009
DOI: 10.1086/381523 Bibcode: 2004ApJ...603..595F

Monteiro, Hektor; Schwarz, Hugo E.; Fernández, Rodrigo

We have measured the proper motion (PM) and kinematics of the ansae in NGC 7009 using high-dispersion echelle spectra and archive narrowband Hubble Space Telescope images. Assuming that the ansae are moving at equal and opposite velocities from the central star, we obtain a system radial velocity of -53+/-2 km s-1, the eastern ansa appr…

2004 The Astrophysical Journal
eHST 17