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    Instruments

    Introduction

    Ulysses hosts a suite of science instruments dedicated to the study of a wide range of topics: the heliospheric magnetic field, heliospheric radio and plasma waves, the solar wind plasma including its minor heavy ion constituents, solar and interplanetary energetic particles, galactic cosmic rays and the anomalous cosmic ray component.

    Other investigations are directed towards studies of cosmic dust and interstellar neutral gas, as well as solar x-rays and cosmic gamma-ray bursts.  Radio science experiments to probe the solar corona and to conduct a search for gravitational waves have also been carried out exploiting the spacecraft's radio communications links with the ground stations.

    Summary

    Last Update: 08 Dec 2006

    • Shortcut URL
    • http://sci.esa.int/jump.cfm?oid=40406
    • Related Articles
    • Introduction
    • Summary
    • VHM/FGM
    • SWOOPS
    • SWICS
    • URAP
    • EPAC/GAS
    • HI-SCALE
    • COSPIN
    • GRB
    • DUST
    • SCE
    • GWE
    • Interdisciplinary Investigations
    • Related Links
    • VHM/FGM at Imperial College
    • SWOOPS at Los Alamos
    • SWICS at the University of Michigan
    • URAP at Goddard Space Flight Center
    • EPAC at the Max Planck Institute for Solar System Research
    • GAS at the Max Planck Institute for Solar System Research
    • HI-SCALE at Johns Hopkins University
    • COSPIN at the University of Chicago
    • COSPIN/KET at IEAP
    • COSPIN/AT at Imperial College
    • COSPIN/HET at the University of New Hampshire
    • COSPIN/HFT at Herzberg Institute of Astrophysics
    • COSPIN/KET at CNR
    • GRB at the University of California
    • DUST at the Max Planck Institute
    • SCE at the University of Bonn

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