Search Publications

High-Energy 3He-Rich Solar Particle Events
DOI: 10.1023/A:1024091002078 Bibcode: 2003SoPh..214..177T

Kocharov, Leon; Torsti, Jarmo; Thompson, Barbara J. +2 more

Energetic particle observations of the ERNE instrument on board SOHO enable measurements of 3He and 4He fluxes beyond 15 MeV nucleon−1 with good statistical resolution. We report results of a survey of the ERNE observations covering the period from 8 February 1999 to 6 December 2000. We find 10 and 5 days during wh…

2003 Solar Physics
SOHO 6
The Sun's Distance from the Galactic Plane
DOI: 10.1023/B:ASTR.0000005097.18183.64 Bibcode: 2003Ap&SS.288..417B

Branham, R. L., Jr.

Use is made of 93,106 parallaxes from the Hipparcos catalog, with a mixture of spectrum-luminosity classes, to derive the position of the Galactic plane. The reduction technique, mixed total least squares-least squares, takes into account the errors in the parallaxes, and the condition that the direction cosines of the Galactic pole have unit Eucl…

2003 Astrophysics and Space Science
Hipparcos 6
Reconstructed 3-d magnetic field structure and hard X-ray two ribbons for 2000 Bastille-day event
DOI: 10.1023/A:1025515504413 Bibcode: 2003SSRv..107..111Y

Yan, Yihua; Huang, Guangli

The Bastille-day event in 2000 produced energetic 3B/X5.6 flare with a halo CME, which had great geo-effects consequently. This event has been studied extensively and it is considered that it follows the two-ribbon flare model. The flare/CME event was triggered by an erupting filament and TRACE observations showed formation of giant arcade structu…

2003 Space Science Reviews
SOHO 6
Steady-state event-excluded proton spectra at solar minimum at all heliolatitudes
DOI: 10.1029/2003GL017154 Bibcode: 2003GeoRL..30.8037P

Armstrong, T. P.; Patterson, J. D.

We present spectra of a steady foreground population of particles in the inner heliosphere observed by the Heliosphere Instrument for Spectra, Composition, and Anisotopy at Low Energies (HISCALE) on board the Ulysses spacecraft. The observed spectra come from the full range of heliolatitudes visited by Ulysses, -80 to +80 degrees, during Ulysses' …

2003 Geophysical Research Letters
Ulysses 6
The Star-forming Dwarf Galaxy Populations of Two z ~ 0.4 Clusters: MS 1512.4+3647 and A851
DOI: 10.1086/377510 Bibcode: 2003ApJ...596..143L

Ferguson, Henry C.; Martin, Crystal L.; Lotz, Jennifer M.

We present the results of a deep narrowband [O II] λ3727 emission line search for faint (g<27), star-forming galaxies in the field of the z=0.37 MS 1512.4+3647 cluster. We find no evidence for an overdensity of emission-line sources relative to the field at z~0.4 and therefore conclude that the MS 1512.4+3647 sample is dominated by field [O II]…

2003 The Astrophysical Journal
eHST 6
Comparative Absorption and Emission Abundance Analyses of Nebulae: Ion Emission Densities for IC 418
DOI: 10.1086/345915 Bibcode: 2003PASP..115..178W

Jenkins, Edward B.; Williams, Robert; Baldwin, Jack A. +1 more

Recent analyses of nebular spectra have resulted in discrepant abundances from CNO forbidden and recombination lines. We consider independent methods of determining ion abundances for emission nebulae, comparing ion emission measures with column densities derived from resonance absorption lines viewed against the central star continuum. Separate a…

2003 Publications of the Astronomical Society of the Pacific
eHST 6
Ion isotropy and ion resonant waves in the solar wind: Corrected Cassini observations
DOI: 10.1029/2002JA009312 Bibcode: 2003JGRA..108.1045K

Gurnett, D. A.; Dougherty, M. K.; Hospodarsky, G. B. +3 more

In an earlier paper [, 2001], observations of electric field fluctuations in the range 0.5 to 25 Hz were reported. We have recently found that the data presented in that paper are seriously contaminated by broadband interference which appears to be generated in the spacecraft wake. Wake instabilities have been found by others, but the plasma condi…

2003 Journal of Geophysical Research (Space Physics)
Cassini 6
The brightness temperature problem in extreme intra-day variable quasars: a model for PKS 0405-385
DOI: 10.1046/j.1365-8711.2003.06429.x Bibcode: 2003MNRAS.341..230P

Protheroe, R. J.

I re-examine the brightness temperature problem in PKS 0405-385, which is an extreme intra-day variable radio quasar with an inferred brightness temperature of ~5 × 1014 K at 5 GHz, well above the Compton catastrophe limit of ~1011 K that is reached when the synchrotron photon energy density exceeds the energy density of the …

2003 Monthly Notices of the Royal Astronomical Society
INTEGRAL 5
The in-flight background of IBIS/PICsIT
DOI: 10.1051/0004-6361:20031460 Bibcode: 2003A&A...411L.203S

Di Cocco, G.; Malizia, A.; Bassani, L. +3 more

The PICsIT instrument is the high-energy imaging detector of IBIS on board INTEGRAL and comprises 4096 individual scintillator elements each working in the energy range from about 175 keV to 10 MeV. Images of the sky are created using the coded aperture technique wherein each point in the detection plane contributes to the final image. For this re…

2003 Astronomy and Astrophysics
INTEGRAL 5
IBIS ground calibration
DOI: 10.1051/0004-6361:20031439 Bibcode: 2003A&A...411L.159B

Di Cocco, G.; Malaguti, G.; Bird, A. J. +13 more

We present an overview of results obtained from IBIS ground calibrations. The spectral and spatial characteristics of the detector planes and surrounding passive materials have been determined through a series of calibration campaigns. Measurements of pixel gain, energy resolution, detection uniformity, efficiency and imaging capability are presen…

2003 Astronomy and Astrophysics
INTEGRAL 5