SOHO/Energetic and Relativistic Nuclei and Electron (ERNE) Data Archive

ERNE will investigate the solar atmosphere by detecting charged particles produced in various solar energy release processes. The scientific objectives of the experiment are: 1. energy spectra of ions and electrons above 1 MeV/nucleon 2. elemental and isotopic abundance H to Fe 3. particle acceleration in the solar atmosphere and interplanetary shocks 4. particle propagation in the solar corona and in the interplanetary space 5. study both large and small scale properties of the IMF 6. short-period temporal variations of particle flux 7. flux anisotropy within the apparatus viewing cone 8. flux of protons penetrating the instrument (even decay solar neutrons) Data consists of two-hour averaged Proton and Helium intensities, data archived by Carrington rotation, HED Proton events in the energy range 12-100 MeV and Level-2 EXPORT data.

All SOHO/ERNE data are available from the public SOHO data archive: sohowww.nascom.nasa.gov/data/data.html Mirror archives are available at: SOHO Archive at Rutherford Appleton Laboratory, UK.: trace.solararchive.rl.ac.uk/soho/ SOHO Archive at the Institut d'Astrophysique Spatiale, France: idc-medoc.ias.u-psud.fr/ SOHO Archive at Osservatorio Astronomico di Torino, Torino, Italy: solar.to.astro.it/