Search Publications

Variations of the High Energy Electron Flux Along the ULYSSES Trajectory
DOI: 10.1007/BF00768813 Bibcode: 1995SSRv...72..409R

Sierks, H.; Kunow, H.; Wibberenz, G. +7 more

We describe for the first time the analysis of high energy electrons (above 240 MeV) from the COSPIN/KET experiment onboard Ulysses. The electron time profiles in four energy windows are presented from Oct. 90 to the end of March 94, up to a maximum heliographic latitude of 57 °S. The recovery rates we derived for the electrons are compared to the…

1995 Space Science Reviews
Ulysses 4
Radio Occultation Studies with Solar Corona Sounders
DOI: 10.1007/BF00768757 Bibcode: 1995SSRv...72...77P

Pätzold, M.; Neubauer, F. M.; Bird, M. K.

Solar Corona Sounders (SCS), a mission designed to utilize the radio occultation technique for investigations of the inner heliosphere, was submitted to ESA in response to a call for new mission concepts. The SCS platforms are two small multifrequency transmitters placed at the “anti-Earth” position (superior solar conjunction) for continuous radi…

1995 Space Science Reviews
Ulysses 4
Evolution of the Electron/Proton Ratios Between 1 and 7 GV Measured at Ulysses, as a Function of Time and Latitude
Bibcode: 1995ICRC....4..752F

Sierks, H.; Kunow, H.; Wibberenz, G. +10 more

1995 International Cosmic Ray Conference
Ulysses 3
A photoionization model of the nebula around the WC11 star M4-18
DOI: 10.1093/mnras/275.3.685 Bibcode: 1995MNRAS.275..685S

Rao, N. Kameswara; Surendiranath, R.

A photoionization code has been developed incorporating provision for the presence of dust mixed with gas. M4-18 has been modelled utilizing optical CCD spectra and other observations ranging from UV to radio wavelengths. T_e and N_e from the model are 6600K and 6050 cm^-3, respectively. The abundances of C, N and Ne are found to be the same as th…

1995 Monthly Notices of the Royal Astronomical Society
IUE 3
Radiation Hydrodynamic Models of Eclipsing Low-Mass X-Ray Binaries
DOI: 10.1086/309778 Bibcode: 1995ApJ...454L.133M

McKee, Christopher F.; Murray, Stephen D.; Woods, D. Tod +2 more

We present the results of self-consistent two-dimensional radiation hydrodynamic models of winds and coronae above accretion disks in low-mass X-ray binaries. The numerical method combines adaptive mesh refinement for the hydrodynamics with combined ray tracking/flux-limited diffusion for the radiation. The results of the models are compared with …

1995 The Astrophysical Journal
Exosat 3
Tomography/Power Spectrum Techniques for Removal of Fixed Pattern Noise from Hubble Space Telescope Spectra
DOI: 10.1086/175925 Bibcode: 1995ApJ...447..880L

Smith, Andrew M.; Bruhweiler, Frederick C.; Lyu, Cheng-Hsuan

We have developed tomography/power spectrum algorithms to differentiate the intrinsic stellar spectrum from the pronounced fluctuations in the spectrum counts due to photocathode granularity and diode-to-diode gain variations. We have presented the results of four typical high signal-to-noise (S/N) and high-resolution data sets, obtained from the …

1995 The Astrophysical Journal
eHST 3
A particle event at 5 AU and 20° southern latitude from measurements with the EPAC instrument on Ulysses
DOI: 10.1007/BF00768803 Bibcode: 1995SSRv...72..343R

Krupp, N.; Fränz, M.; Balogh, A. +9 more

In November 1992, the Ulysses spacecraft observed a multiple solar particle event and a CME event at 5.2 AU and a heliographic latitude of 20° S which were superimposed to the recurrent corotating interacting region. Distinct particle flux increases caused by these events were observed in all energy channels of the EPAC experiment. The experimenta…

1995 Space Science Reviews
Ulysses 3
Interaction Between Whistler-Mode Waves and Electrons in the Vicinity of Interplanetary Shocks as Seen by Ulysses: A Preliminary Study
DOI: 10.1007/BF00768775 Bibcode: 1995SSRv...72..181S

Balogh, A.; Forsyth, R. J.; Bame, S. J. +5 more

We present a study of wave particle interaction in the vicinity of interplanetary shocks in the ecliptic plane, as observed by the Ulysses spacecraft. We focus here on some events, for which electromagnetic waves are observed, mainly down-stream of the shock. The whistler mode waves are studied by means of the Unified RAdio and Plasma wave experim…

1995 Space Science Reviews
Ulysses 3
On the minimum fluxes of low-energy ions (0.5 MeV/nuc - 8 MeV/nuc) at high heliospheric latitudes
DOI: 10.1016/0273-1177(94)00024-U Bibcode: 1995AdSpR..15g..81B

Krupp, N.; Keppler, E.; Fraenz, M. +3 more

The quiet-time fluxes of ions from 0.5 MeV/nuc to 7 MeV/nuc (for oxygen) have been studied for the time period between mid-1993 through the first 104 days of 1994. During this time period Ulysses was below the heliographic current sheet. We find that at the quietest times, the ion population is dominated by the ACR component. For more active times…

1995 Advances in Space Research
Ulysses 3
The application of network synthesis to repeating classical gamma-ray bursts
DOI: 10.1016/0273-1177(94)00051-2 Bibcode: 1995AdSpR..15e.127H

Hurley, K.; Kouveliotou, C.; Laros, J. +3 more

It has been suggested that the BATSE gamma-ray burst catalog contains several groups of bursts clustered in space or in space and time, which provide evidence that a substantial fraction of the classical gamma-ray burst sources repeat. Because many of the bursts in these groups are weak, they are not directly detected by the Ulysses GRB experiment…

1995 Advances in Space Research
Ulysses 3