Science Archives Publication System

Observing the Solar Wind Between 1 and 4 AU with the Radio Receiver on Ulysses

DOI: 10.1016/0273-1177(93)90430-J Bibcode: 1993AdSpR..13f.295H

Pantellini, F.; Forsyth, R. J.; Stone, R. G. +8 more

1993 • Advances in Space Research

Ulysses 1

Energetic particle results from ulysses (extended abstract)

DOI: 10.1016/0920-5632(93)90094-M Bibcode: 1993NuPhS..33..213W

Sierks, H.; Kunow, H.; Wibberenz, G. +6 more

1993 • Nuclear Physics B Proceedings Supplements

Ulysses 1

Charged-particle induced background expected in X-ray detecting CCDs in highly eccentric earth orbits

DOI: 10.1007/BF01588348 Bibcode: 1993ExA.....4..105D

Danner, R.

Charged particle fluxes on satellites in highly eccentric Earth orbits are studied, using data from ISEE1 and EXOSAT missions. The effects of minimum-ionizing particles, low-energy electrons and secondary radiation produced by these particles on CCDs used as X-ray detectors are identified. A technique to discriminate events caused by minimum-ioniz…

1993 • Experimental Astronomy

Exosat 1

Radio waves in the heliosphere

DOI: 10.1016/0273-1177(93)90409-5 Bibcode: 1993AdSpR..13f.191B

Bougeret, J. -L.

Solar radio emissions at long wavelengths (wavelengths greater than 10 m or frequencies smaller than 30 MHz) are produced in the upper corona and in the interplanetary medium (the Heliosphere), sometimes at very large distances from the Sun, up to the orbit of Jupiter and beyond. Solar radio emissions are produced by the passage of energetic parti…

1993 • Advances in Space Research

Ulysses 1

The new Be-type star HD 147196 in the rho Ophiuchi dark cloud region.

Bibcode: 1993A&A...269..181T

Perez, M. R.; The, P. S.; de Winter, D. +1 more

The newly discovered hot-emission line star, HD 147196 in the Rho Oph dark cloud region was observed spectroscopically and photometrically and high and low resolution IUE spectra were obtained. The finding of Irvine (1990) that this relatively bright star show its H-alpha-line in emission is confirmed. Previous H-alpha-surveys of the Rho Oph star-…

1993 • Astronomy and Astrophysics

IUE 1

The Proton and Alpha Spectra in and out of the Ecliptic, and the Appearance of the Anomalous He Component - Ulysses Observations

Bibcode: 1993ICRC....3..409F

Kunow, H.; Heber, B.; Ferrando, P. +6 more

1993 • 23rd International Cosmic Ray Conference (ICRC23), Volume 3

Ulysses 1

HST FOC/48 UV imagery of GR8.

Bibcode: 1993RMxAA..27..165P

Dufour, R. J.; Wyatt, R. J.; Patterson, B.

Imagery observations of GR8 were made in July 1991 with the Hubble Space Telescope. The Wide Field Camera imaged the entire galaxy at 5500 Å (F555W), 4390 Å (F439W), and 3360 Å (F336W); and two smaller fields around the H II regions HL5 and HL19 were imaged at 1400 Å (F150W) with the Faint Object Camera. B and V magnitudes for these stars are from…

1993 • Revista Mexicana de Astronomia y Astrofisica

eHST 1

Ulysses observations of a pure electron event and its associated type III radio emission on December 15, 1990

DOI: 10.1016/0273-1177(93)90503-4 Bibcode: 1993AdSpR..13i.351P

Chaizy, P.; Pick, M.; Forsyth, R. +5 more

We describe an electron event associated with a type III burst observed by Ulysses. This event was observed when the spacecraft crossed the region of strong compression between a fast and a slow solar wind stream, characterized by a relatively high density and a complex behaviour of the plasma density, magnetic field and energetic electron anisotr…

1993 • Advances in Space Research

Ulysses 1

Tuned Solar and Stellar Oscillations?

Bibcode: 1993IrAJ...21...83A

Doyle, J. G.; Andrews, A. D.

1993 • Irish Astronomical Journal

IUE 1

Einstein and EXOSAT observations of Geminga revisited

DOI: 10.1016/0273-1177(93)90136-Y Bibcode: 1993AdSpR..13l.343M

Bignami, G. F.; Mereghetti, S.; Caraveo, P.

We have re-analyzed the archive Einstein IPC and EXOSAT CMA x-ray data of Geminga, in the light of the recent discoveries on this source. The results of a search for the 237 msec periodicity are consistent with a pulsed fraction decreasing with x-ray energy. We have combined the EXOSAT CMA and the Einstein data in order to limit the spectral param…

1993 • Advances in Space Research

Exosat 1