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The Pulkovo catalog of 284 positions of Pluto in 1930 - 1994 based on observations from three observatories.
DOI: 10.1515/astro-1997-0260 Bibcode: 1997BaltA...6..349R

Ryl'Kov, V. P.; Dement'eva, A. A.; Narizhnaja, N. V.

A unique data archive of measurements and reduced positions of Pluto for the period from 1930 to 1994 has been collected from a new reduction of all photographic observations of Pluto obtained by Pulkovo astronomers. All 250 plates taken with the Pulkovo Normal astrograph were remeasured in 1993-1994. These measurements form data files that can be…

1997 Baltic Astronomy
Hipparcos 1
On the Possible Correlation Between Gamma-Ray Bursts and Radio-Quiet Quasars
Bibcode: 1997ICRC....3...45H

Cline, T.; Hurley, K.; Kouveliotou, C. +4 more

1997 International Cosmic Ray Conference
Ulysses 1
The Cluster Data Processing System: a Distributed System in Support of a Challenging Scientific Mission
DOI: 10.1023/A:1004906620952 Bibcode: 1997SSRv...79..527S

Sorensen, E. M.; Merri, M.; di Girolamo, G.

1997 Space Science Reviews
Cluster 1
The Lyman-α line from the solar wind acceleration region: Results from an eight-moment approximation two-fluid solar wind model
DOI: 10.1029/97GL02583 Bibcode: 1997GeoRL..24.2873O

Olsen, Espen Lyngdal

We investigate neutral hydrogen in an eight-moment, two-fluid, high speed solar wind model. In this model the proton heat flux decreases rapidly in the solar wind acceleration region, and extended coronal heating of the proton gas leads to high coronal proton temperatures and large solar wind flow speeds. The properties of the Lyman-α line from th…

1997 Geophysical Research Letters
SOHO 1
The Major Discoveries of the Ulysses Mission
Bibcode: 1997ICRC....8...27F

Fisk, L. A.

1997 International Cosmic Ray Conference
Ulysses 1
Study of Coronal Transients in UV Line Emission
DOI: 10.1023/A:1004951017307 Bibcode: 1997SoPh..172..215M

Noci, Giancarlo; Martin, Renato; Maccari, Lisa

We investigate the expected emission from coronal transients in the following spectral lines observable with the Ultraviolet Coronagraph Spectrometer (UVCS) on board SOHO: Hi Lα 1216 Å, Ovi 1032-1037 Å, Nv 1239-1243 Å, Mgx 610-625 Å, Sixii 499-521 Å, and Fexii 1242 Å. We calculate line intensities and profiles for typical CME conditions, and we an…

1997 Solar Physics
SOHO 1
Plasma wave characteristics of the jovian magnetopause boundary layer: Can wave-particle interactions cause the jovian aurora?
Bibcode: 1997JGR...102.4765T

Krupp, N.; Balogh, A.; Tsurutani, B. T. +10 more

1997 Journal of Geophysical Research
Ulysses 1
Alfvén waves in the solar corona and solar wind
DOI: 10.1088/0741-3335/39/12B/024 Bibcode: 1997PPCF...39B.317V

Velli, M.; Pruneti, F.

1997 Plasma Physics and Controlled Fusion
Ulysses 1
Improvement of proper motions for Hipparcos stars with photographic plates.
Bibcode: 1997AcASn..38..297W

Wang, Jia-Ji; Tang, Zheng-Hong; Wang, Shu-He +1 more

Using the PPM catalogue as a preliminary reference catalogue, the authors have reduced 17 exposures on 9 plates taken with the 40 cm refractor at Zo-Sè Station of Shanghai Astronomical Observatory in about 30 years. By means of the central overlapping technique and the iterative process, high-precision positions and proper motions of 28 PPM stars,…

1997 Acta Astronomica Sinica
Hipparcos 1
Compton-Getting Factor and Latitude Variation of Cosmic Rays
Bibcode: 1997ICRC....2...93P

Potgieter, M. S.; Heber, B.; Ferrando, P. +3 more

1997 International Cosmic Ray Conference
Ulysses 1