Search Publications

Charged-Particle Motion in Multidimensional Magnetic Field Turbulence
DOI: 10.1086/187457 Bibcode: 1994ApJ...430L.137G

Giacalone, J.; Jokipii, J. R.

We present a new analysis of the fundamental physics of charged-particle motion in a turbulent magnetic field using a numerical simulation. The magnetic field fluctuations are taken to be static and to have a power spectrum which is Kolmogorov. The charged particles are treated as test particles. It is shown that when the field turbulence is indep…

1994 The Astrophysical Journal
Ulysses 115
The Coronal Electron Density Distribution Determined from Dual-Frequency Ranging Measurements during the 1991 Solar Conjunction of the ULYSSES Spacecraft
DOI: 10.1086/174073 Bibcode: 1994ApJ...426..373B

Bird, M. K.; Asmar, S. W.; Volland, H. +3 more

Dual-frequency ranging and Doppler measurements were conducted in support of the Ulysses Solar Corona Experiment (SCE) at and around the spacecraft's first solar conjunction in 1991 August. The differential group delay time between range codes on the two downlink carrier signals at the wavelengths 13.1 and 3.6 cm, a direct measure of the total ele…

1994 The Astrophysical Journal
Ulysses 71
Network Synthesis Localization of Two Soft Gamma Repeaters
DOI: 10.1086/187465 Bibcode: 1994ApJ...431L..31H

Cline, T.; Kouveliotou, C.; Sommer, M. +5 more

We introduce the method of 'network synthesis,' which allows the detection of very weak gamma-ray transient signals in the data of the Ulysses gamma-ray burst (GRB) experiment from repeating sources. It consists of defining a grid of alpha, delta values, and for each BATSE detection of a burst from a soft gamma repeater, predicting the arrival tim…

1994 The Astrophysical Journal
Ulysses 50
A Search for the Radio Counterpart to the 1994 March 1 Gamma-Ray Burst
DOI: 10.1086/187678 Bibcode: 1994ApJ...437L..43F

Cline, T.; Frail, D. A.; Kulkarni, S. R. +7 more

We report on the results of a search for the radio counterpart to the bright γ-ray burst of 1994 March 1. Using the Dominion Radio Astrophysical Observatory Synthesis Telescope sensitive, wide-field radio images at 1.4 GHz and 0.4 GHz were made of a region around GRB 940301. A total of 15 separate radio images were obtained at each frequency, samp…

1994 The Astrophysical Journal
Ulysses 41
Rapid Searches for Counterparts of GRB 930131
DOI: 10.1086/187215 Bibcode: 1994ApJ...422L..71S

Schaefer, Bradley E.; Coe, M. J.; Ricker, George R. +39 more

A fading counterpart to a gamma-ray burst (GRB) would appear as a point source inside a GRB error region soon after the burst which dims on a timescale from minutes to days. The favorable circumstances of the burst GRB 930131 allowed for an international campaign to search for fading counterparts starting 6.8 hr after the burst. We report observat…

1994 The Astrophysical Journal
Ulysses 31
Directivity of 100--500 keV Solar Flare Hard X-Ray Emission
DOI: 10.1086/174112 Bibcode: 1994ApJ...426..758L

Hurley, K.; Niel, M.; Li, P. +3 more

We have identified 28 solar flares simultaneously observed by a SIGNE detector aboard the Venera 13 and Venera 14 spacecraft and the Hard X-Ray Burst Spectrometer (HXRBS) aboard the Solar Maximum Mission (SMM), over a wide range of observing angles. Fourteen of them were also observed by the Gamma Ray Spectrometer (GRS) on SMM and were included in…

1994 The Astrophysical Journal
Ulysses 16
Searching for Hard X-Ray Directivity during the Rise, Peak, and Decay Phases of Solar Flares
DOI: 10.1086/173656 Bibcode: 1994ApJ...421..381L

Li, Peng

We have identified 72 large solar flares (peak counting rates more than 1000 counts/s) observed by Hard X-ray Burst Spectroscopy (HXRBS) on-board the Solar Maximum Mission (SMM). Using a database of these flares, we have studied hard X-ray (50-850 keV) spectral center-to-limb variation and its evolution with time. The major results are the followi…

1994 The Astrophysical Journal
Ulysses 7
Diffusive Shock Acceleration in the Presence of Current Sheets
DOI: 10.1086/174328 Bibcode: 1994ApJ...429..385K

Jokipii, J. R.; Kota, J.

We study the nature of diffusive shock acceleration in the presence of current sheets which are oriented normal to the shock, so that the drift along the sheets carries particles either away from or toward the shock plane. We consider a system with periodic regions of alternating magnetic field direction. This can be taken to be a very crude repre…

1994 The Astrophysical Journal
Ulysses 4