Solar Orbiter
Overview
Solar Orbiter is designed to identify the origins and causes of the solar wind, the heliospheric magnetic field, the solar energetic particles, the transient interplanetary disturbances, and the Sun's magnetic field.RAL Space involvement
RAL Space leads an international consortium that designed, developed and calibrated an Extreme Ultraviolet Spectrometer, SPICE (Spectral Investigation of the Coronal Environment). The RAL Space team will also be involved in the post-launch operations of SPICE.
Spectral Investigation of the Coronal Environment (SPICE)
RAL Space led the development of the SPICE extreme‑ultraviolet spectrometer, working with an international consortium from concept to operations. SPICE delivers vital diagnostics of the Sun’s atmosphere. The two EUV wavelength bands, 70.4 – 79.0 nm and 97.3 – 104.9 nm, observed by SPICE are dominated by emission lines from a wide range of ionized atoms of H, C, O, N, Ne, S, Mg, Si, and Fe, formed in the Sun’s atmosphere at temperatures from 10 thousand to 10 million Kelvin. SPICE measures spectral line intensities, temperatures, electron density, plasma velocities along the line of sight and elemental composition.
The SPICE project continues RAL Space’s long heritage in solar spectroscopy, including its previous Principal Investigator role on the SOHO Coronal Diagnostic Spectrometer (1995 – 2014).