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The '10-hour' Modulation of the Jovian Electron Spectrum in Interplanetary Space-Ulysses Observations
Bibcode: 1993ICRC....3..346R

Ferrando, P.; Raviart, A.; Ducros, R. +1 more

1993 23rd International Cosmic Ray Conference (ICRC23), Volume 3
Ulysses 2
A global analysis method for astrolabe observations
Bibcode: 1993A&A...280..675C

Chollet, F.

In a previous paper (Chollet & Najid 1992), we gave the general principles of a new global method to analyze the astrolabe observations. The fundamental equation was obtained from the classical one in which the corrections to the star positions at the observational epoch are replaced by developments that contain the corrections to the star pos…

1993 Astronomy and Astrophysics
Hipparcos 2
Observations of 0.3 to 2.0 MeV Protons in the 1 to 5 AU Region with Voyager 1 and Ulysses Compared to IMP 8
Bibcode: 1993ICRC....3..334B

Armstrong, T.; Boufaida, M.

1993 23rd International Cosmic Ray Conference (ICRC23), Volume 3
Ulysses 2
Calibration of Hipparcos Long Period Variable Start Fields Using Multi-Color CCD Observations
Bibcode: 1993JAVSO..22....2H

Howell, Steve B.; Mattei, Janet; Benson, Priscilla J. +1 more

The first set of 4-color AAVSO CCD finder charts has been prepared using the 0.9-m telescope at Kitt peak national Observatory in Arizona. The stars selected were northern long period variable stars observed with the Hipparcos astrometric satellite, since multicolor photometry was needed on these stars to calibrate and reduce the photometric and a…

1993 Journal of the American Association of Variable Star Observers (JAAVSO)
Hipparcos 2
Precise measurement of the right ascension of the Geminga pulsar using COS-B data.
Bibcode: 1993A&A...277L..13C

Li, T. P.; Cheng, L. X.; Ma, Y. Q. +2 more

We have obtained a more precise value of the right ascension and a new spin evolution law of the Geminga pulsar using COS-B data on the assumption 0r high stability of the absolute phase. The new value is a(1950)=6h30m59s .057, with error about 0.5 arcsec, compared with the 3.2 arcsecs from the Einstein HRI result.…

1993 Astronomy and Astrophysics
COS-B 2
Comparisons of IUE & HST ultraviolet spectra of extragalactic H II regions.
Bibcode: 1993RMxAA..27..115D

Terlevich, E.; Terlevich, R.; Garnett, D. R. +5 more

The authors compare recently obtained HST FOS and IUE SWP ultraviolet spectra of two extragalactic H II regions: SBS 0335-052 and 30 Doradus in the LMC. They also present IUE SWP NEWSIPS processed spectra of I Zw 18, which show significant improvements in the data quality, suggesting that reprocessed IUE archival spectra will offer enhanced scienc…

1993 Revista Mexicana de Astronomia y Astrofisica
eHST 2
Model Atmospheres: Tool for Identifying Interstellar Features
DOI: 10.1086/191745 Bibcode: 1993ApJS...84...55F

Frisch, P. C.; Slojkowski, S. E.; Rodriguez-Bell, T. +1 more

Model atmosphere parameters are derived for 14 early A stars with rotation velocities, from optical spectra, in excess of 80 km/s. The models are compared with IUE observations of the stars in regions where interstellar lines are expected. In general, with the assumption of solar abundances, excellent fits are obtained in regions longward of 2580 …

1993 The Astrophysical Journal Supplement Series
IUE 2
The Ultraviolet Spectrum of the Binary System Ty-Pyxidis
DOI: 10.1007/BF00658109 Bibcode: 1993Ap&SS.200...47D

Danezis, E.; Theodossiou, E.; Antonopoulou, E.

A detailed list and analysis of line identifications of five UV spectra of the RS CVn-type binary system TY Pyxidis are presented. These spectra are recorded at different phases with the International Ultraviolet Explorer (IUE). Two of them are in the wavelength rangeλλ1235–1950 Å while the other three in the rangeλλ2700–3110 Å. The far-UV spectru…

1993 Astrophysics and Space Science
IUE 1
Anisotropy measurements and spectra from a solar proton event in March 1991
DOI: 10.1016/0273-1177(93)90397-T Bibcode: 1993AdSpR..13f..99S

Balogh, A.; Forsyth, R. J.; Cowley, S. W. H. +2 more

We use observations from the Anisotropy Telescopes on the Ulysses spacecraft to determine the omnidirectional flux profile of protons in the energy range 0.7 - 1.3 MeV, during the solar proton event that began on 23 Mar 1991. We also show the spectral index throughout the event at 0.7 - 2.2 MeV and at 2.2 - 6.5 MeV, with three example spectra, one…

1993 Advances in Space Research
Ulysses 1
Gas dynamics of solar wind interaction with interstellar gas: theory and experiment.
Bibcode: 1993ASPRv...8....1B

Baranov, V. B.

A survey of the current situation in gas dynamic models of solar wind interaction with the local interstellar medium (LISM) is presented. The role of these models in interpreting a number of observed physical phenomena is investigated. Attention is concentrated on the self-consistent gas dynamic model of solar wind interaction with the supersonic …

1993 Astrophysics and Space Physics Reviews
Ulysses 1