Search Publications

C IV and O VI Transitions in the Region lambda lambda 1100--2000 and Examples Found in IUE Spectra of Hot Stars
DOI: 10.1086/192226 Bibcode: 1995ApJS..100..405F

Feibelman, Walter A.; Johansson, Sveneric

We present Ritz wavelengths for more than 130 transitions of C IV and O VI in the range λλ1100-2000 and show examples of absorption features as seen in representative examples of high-dispersion IUE spectra of very hot (∼100,000 K) nuclei of planetary nebulae, white dwarfs, and PG 1159-type stars. The regions near He II λ640 and interstellar Si II…

1995 The Astrophysical Journal Supplement Series
IUE 18
The Elemental Composition in Energetic Particle Events at High Heliospheric Latitudes
DOI: 10.1007/BF00768802 Bibcode: 1995SSRv...72..339F

Krupp, N.; Fränz, M.; Keppler, E. +2 more

The relative abundances of low energy ions (0.6 2.0 MeV/n) in solar energetic particle (SEP) and corotating interaction region (CIR) events have been measured by the EPAC experiment aboard Ulysses since launch in October 1990 until the present time. We give an overview of the abundances of heavy ions (He, C, Ne, Fe) relative to oxygen during energ…

1995 Space Science Reviews
Ulysses 18
ULYSSES observations of latitude gradients in the heliospheric magnetic field
DOI: 10.1016/0273-1177(95)00328-C Bibcode: 1995AdSpR..16i.165S

Phillips, J.; Balogh, A.; Tsurutani, B. T. +3 more

Several parameters measured by Ulysses as it traveled southward to heliographic latitudes of -50 deg are presented and analyzed. The radial component of the magnetic field, averaged over 5 deg latitude increments and extrapolated back to 1 AU, is found to agree with baseline measurements provided by IMP-8. There is little, if any, evidence of a la…

1995 Advances in Space Research
Ulysses 18
High-Latitude Observations of Energetic Ions During the First ULYSSES Polar Pass
DOI: 10.1007/BF00768793 Bibcode: 1995SSRv...72..291S

Balogh, A.; Forsyth, R. J.; Goldstein, B. E. +3 more

We present observations of energetic ions from the Ulysses COSPIN Low Energy Telescope in the mid and high-latitude regions of the heliosphere prior to and during the first polar pass of the Ulysses spacecraft. After the encounter with Jupiter, Ulysses started on its journey out-of-the-ecliptic. Between ∼13°S and ∼29°S the spacecraft sampled the s…

1995 Space Science Reviews
Ulysses 18
An Atlas of Alpha Orionis Obtained with the Goddard High Resolution Spectrograph on the Hubble Space Telescope
DOI: 10.1086/117484 Bibcode: 1995AJ....109.2706B

Savage, B. D.; Ebbets, D. C.; Carpenter, K. G. +18 more

An atlas of observations of the late-type supergiant a Orionis taken with the Goddard High Resolution Spectrograph in 1992 September is presented. We have included identifications of the major features along with the fully reduced spectrum. The 33 exposures consist of 3 high resolution (R∼80,000) and 30 medium resolution (R ∼20,000∼35,000) observa…

1995 The Astronomical Journal
IUE eHST 18
The Ultraviolet Reflectivity of Jupiter at 3.5 Angstrom Resolution from Astro-1 and Astro-2
DOI: 10.1086/309763 Bibcode: 1995ApJ...454L..65M

Wolven, Brian C.; Feldman, Paul D.; McGrath, Melissa A. +2 more

The reflectivity of Jupiter in the wavelength band from 1450 to 1850 A at 3.5 A resolution has been determined from measurements of Jovian equatorial spectra obtained by the Hopkins Ultraviolet Telescope, which was flown on the Space Shuttle Columbia during the 1990 December Astro-1 mission and then on the Endeavour during the 1995 March Astro-2 m…

1995 The Astrophysical Journal
IUE 18
A Search for a Pulsar in the Remnant of SN 1987A with the Hubble Space Telescope High-Speed Photometer
DOI: 10.1086/175840 Bibcode: 1995ApJ...446..832P

Dolan, J. F.; Boyd, P. T.; Nelson, M. J. +8 more

The High Speed Photometer (HSP) on the Hubble Space Telescope (HST) observed the remnant of SN 1987A on four different epochs between 1992 June 2 and 1993 November 4 in a 1600-7000 Å bandpass. Each observation was ∼40 minutes in duration and used a 100 microseconds sampling time. Assuming a spectrum like PSR B0540 -69 with similar reddening, the o…

1995 The Astrophysical Journal
eHST 18
Tangential discontinuities at high heliographic latitudes (∼-80°)
DOI: 10.1029/95GL02981 Bibcode: 1995GeoRL..22.3409H

Balogh, A.; Tsurutani, B. T.; Goldstein, B. E. +2 more

In this study, tangential discontinuities (TDs) near -80° heliographic latitude have been studied. Based on our quantitative definitions, we find that the TDs may generally be divided into two clear types. There is a distinct population of TDs small (<40°) directional changes. About 19% of all high-latitude TDs are in this category. These types…

1995 Geophysical Research Letters
Ulysses 18
ULYSSES solar wind plasma observations during the declining phase of solar cycle 22
DOI: 10.1016/0273-1177(95)00318-9 Bibcode: 1995AdSpR..16i..85P

McComas, D. J.; Goldstein, B. E.; Bame, S. J. +5 more

Since launch in October 1990, the Ulysses mission has included an in-ecliptic cruise enroute to Jupiter encounter in February 1992 and a post-Jupiter transit through a wide range of southerly latitudes and heliocentric distances. Here we present results from the solar wind plasma experiment through June 14, 1994, at which time Ulysses was at -68.2…

1995 Advances in Space Research
Ulysses 18
Solar Wind Charge States Measured by Ulysses/SWICS in the South Polar Hole
DOI: 10.1007/BF00768755 Bibcode: 1995SSRv...72...65G

Galvin, A. B.; Cohen, C. M. S.; Ipavich, F. M. +2 more

The Ulysses mission now has an extensive data base covering several passes of the south polar coronal hole as the spacecraft proceeds to higher latitudes. Using composition measurements from the SWICS experiment on the Ulysses spacecraft, we have obtained charge state distributions, and hence inferred coronal ionization temperatures, for several s…

1995 Space Science Reviews
Ulysses 18