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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
EIT Observations of the 15 November 1999 Mercury Transit
DOI: 10.1023/B:SOLA.0000022945.53373.17 Bibcode: 2004SoPh..219..217A

Auchère, F.; Artzner, G. E.

The Mercury transit of 15 November 1999 has been observed from space by the SOHO and TRACE spacecraft. We exploited the data recorded by EIT/SOHO to determine the stray-light level and the plate-scale of the instrument. The asymmetric distribution of stray light across the images is confirmed, but the absolute amount was found to be higher than pr…

2004 Solar Physics
SOHO 17
The phase curve of cometary dust: Observations of comet 96P/Machholz 1 at large phase angle with the SOHO LASCO C3 coronagraph
DOI: 10.1051/0004-6361:20047131 Bibcode: 2004A&A...427..755G

Schwenn, R.; Jockers, K.; Grynko, Ye.

We have analyzed brightness and polarization data of comet 96P/Machholz, obtained with the SOHO-LASCO C3 coronagraph at phase angles up to 167° and 157°, respectively. The polarization data are characteristic of a typical dusty comet. Within error limits the corresponding trigonometric fit describes the new data measured at l…

2004 Astronomy and Astrophysics
SOHO 17
Pulsational Evidence for Mass Loss in NGC 1866 Cepheids
DOI: 10.1086/423917 Bibcode: 2004AJ....128.1597B

Marconi, M.; Musella, I.; Caputo, F. +2 more

Available observational data for the 20 known Cepheids in the LMC cluster NGC 1866 have been compared with Hubble Space Telescope observations, discovering in the cluster central region five additional variables, one of which appears to be a Cepheid candidate. We also reach the conclusion that only the photometric data for the seven variables in t…

2004 The Astronomical Journal
eHST 17
CDS wide slit time-series of EUV coronal bright points
DOI: 10.1051/0004-6361:20041069 Bibcode: 2004A&A...425.1083U

Foley, C. R.; Doyle, J. G.; Nakariakov, V. M. +1 more

Wide slit (90''×240'') movies of four Extreme Ultraviolet coronal bright points (BPs) obtained with the Coronal Diagnostic Spectrometer (CDS) on board the Solar and Heliospheric Observatory (SoHO) have been inspected. The wavelet analysis of the He I 584.34 Å, O V 629.73 Å and Mg VII/IX 368 Å time-series confirms the oscillat…

2004 Astronomy and Astrophysics
SOHO 17