ASPERA-4: Analyzer of Space Plasmas and EneRgetic Atoms

ASPERA-4  -  a VenusExpress Orbiter Instrument

Analyzer of Space Plasmas and EneRgetic Atoms

ASPERA-4 logo ASPERA-4 is an advanced and compact ion, electron and neutral particle detector package developed for the Venus Express mission to investigate the plasma and neutral particle environment near Venus. ASPERA-4 will perform the first ever Energetic Neutral Atom (ENA) measurements at planet Venus in the low energy range (100 eV - 10 keV). The instrument is essentially identical to the >ASPERA-3 instrument on >Mars Express.


> Science objectives
> Instrument description
> MPS contribution
> Neutral Particle Detector (NPD)
> Neutral Particle Imager (NPI)
Email Joachim Woch
Email Markus Fraenz
> Related links
> ASPERA-4 publications by MPS members

Science objectives

The general scientific objective of ASPERA-4 is to study the solar wind - atmosphere interaction and to characterize the plasma and neutral gas environment in the near-Venus space through >Energetic Neutral Atom (ENA) Imaging and in-situ plasma measurements. ENA imaging is a novel technique to visualize and monitor processes in dilute gases. ENAs are produced via charge exchange processes between singly-charged ions and neutral gases of the exosphere / upper atmosphere. Due to their neutrality, ENAs are decoupled from the electromagnetic fields and propagate on straight paths like photons. Directional detection of the ENAs therefore yields a global image of the interaction region.

The specific objectives are:

These studies address the fundamental question why the atmospheres of Earth, Mars and Venus developed so differently. At Earth the atmosphere has always been protected by the magnetic field against erosion by the solar wind. At Mars the protection by a field vanished during the first 500 Million years after creation of the planet and after that the atmosphere has been almost completely lost. At Venus there are no traces of a primordial field (though the magnetometer on Venus Express might show differently) but the atmosphere was not eroded because of the higher gravity of Venus as compared to Mars. Still we know from previous misions that the Venus atmosphere has no traces of water. How the water has been lost is one of the questions our experiment tries to answer.


Instrument description

ASPERA-4 comprises four sensors:

To increase angular coverage NPI, NPD, and EIS are mounted on a scanning platform.

ASPERA-4 performance

Particles ENA ENA ions electrons
Energy, keV 0.1 - 60 0.1 - 10 0.01 - 40 0.001 - 20
Energy res. dE/E - 80% 10% 7%
Mass res. - H, O M/dM = 5 -
FoV 9 x 344 9 x 180 4.6 x 360 10 x 360
Angular Res. (FWHM) 4.6 x 11.5 5 x 30 5 x 22.5 5 x 22.5
G-Factor/pixel, cm2 sr 2.5 x 10-3 6.2 x 10-3 3.5 x 10-4 3 x 10-4
Efficiency, % 1 1 - 25 n/a n/a
Time res. for full 3D, s 32 32 32 32


MPS contribution

ASPERA-4 is realized by a large international consortium of more than 10 European and US institutes. The >team is led by R. Lundin (Swedish Institute of Space Physics, Kiruna). The MPS, in cooperation with IDA (University Braunschweig) and IFSI, Rom, is supplying the electronics of the NPD sensor and will take part in the scientific data analysis.


Related links

> Swedish Institute of Space Physics
> Aspera-4 site at IRF

2006, Max Planck Institute for
Solar System Research, Lindau