The Energetic and Relativistic Nuclei and Electron (ERNE) experiment w
ill. investigate the solar atmosphere and the heliosphere by detecting
particles produced in various kinds of energy release processes. ERNE
is at the upper end in energy among the SOHO particle instruments. Th
e instrument will measure the energy spectra of elements in the range
Z=1-30. The energy coverage varies dependent on the particle species f
rom a few MeV/n up to a few hundred MeV/n and electrons from 2 to 50 M
eV. At high energies, ERNE records also the direction of the incident
particles for accurate measurements of the pitch angle distribution of
the ambient flux within the viewing cone. Especially the isotope iden
tification capability has been one of the instrument design goals, thu
s providing new data regarding various fundamental questions in solar
physics.