Galileo EPD Particle Instrument

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Galileo - Mission to Jupiter

Energetic Particles Detector (EPD)

The Galileo spacecraft carries an Energetic Particles Detector (EPD) designed to measure the characteristics of energetic particle populations important in determining the size, shape, and dynamics of the Jovian magnetosphere. EPD was developed by the Johns Hopkins University Applied Physics Laboratory (JHU/APL) in collaboration with the Max-Planck-Institut für Sonnensystemforschung (MPS), Germany, as part of NASA's Galileo Program.

	Galileo/EPD science objectives
	Galileo/EPD instrument description
	Galileo/EPD related links
	Galileo/EPD publications by MPS members

Galileo/EPD science objectives

The main scientific goals of EPD are:

• Measure the energy and angular distribution, composition, and stability of trapped radiation at Jupiter.
• Study the interaction of these energetic particles with the Galilean satellites and the solar wind.
• Derive thermal plasma flow velocities and temperatures.
• Examine adiabatic and non-thermal processes in the trapped radiation.

Galileo/EPD instrument description

The energetic particles detector (EPD) is designed to measure the numbers and energies of ions and electrons whose energies exceed about 20 keV. (An electron volt, eV, is the unit of energy equal to the energy that an electron acquires in falling through an electrical potential of 1 volt.) The EPD can also measure the direction of travel of such particles and, in the case of ions, can determine their composition (whether the ion is oxygen or sulfur, for example).

The EPD uses silicon solid-state detectors and a time-of-flight detector system to measure changes in the energetic particle population at Jupiter as a function of position and time. These measurements will tell us how the particles get their energy and how they are transported through Jupiter's magnetosphere.

The EPD weighs 10.5 kilograms and uses 10.1 watts of power on average. EPD measures the detailed energy and angular distribution of the following:

• ions (Z >= 1) from 0.020 to 55 MeV
• electrons from 0.015 MeV to more than 11 MeV
• ion composition from 0.010 MeV/nuc to over 10 MeV/nuc
• the elemental species helium through iron from approximately 10 keV/nuc to 15 Mev/nuc

This data will help us to quantify several characteristics and properties of the Jovian magnetosphere

Galileo/EPD related links

Johns Hopkins University Applied Physics Laboratory EPD home page

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© 2009, Max Planck Institute for Solar System Research, Lindau

Krupp 02-10-2009

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