Marco Nicoletto
Measuring and modeling techniques for extremely low frequency characterization of electromagnetic field emissions in space applications.
Rel. Patrizia Savi. Politecnico di Torino, Corso di laurea magistrale in Mechatronic Engineering (Ingegneria Meccatronica), 2018
Abstract
Recent and upcoming European Space Agency (ESA) programs like BepiColombo, Solar Orbiter, Jupiter ICy moons Explorer (JUICE), Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) and Turbulence Heating ObserveR (THOR) need not only magnetic cleanliness of almost time-constant magnetic fields, but have even more demanding requirements on slowly time-varying magnetic fields and low frequency electric fields. The frequency spectra typically have an upper limit of several hundreds of kilohertz, while the lower limit is in the sub-milliHertz range with time periods of several hours or longer. Space missions with such challenging requirements are becoming more and more relevant for the scientific community with an important presence in the current cycle of ESA's long-term planning for space science missions which is called Cosmic Vision 2015-2025.
The “magnetic suite” is typically composed by three magnetometers: a pair of fluxgate magnetometers for measuring the range from DC to some tens of hertz and a single search coil magnetometer (SCM) designed to measured AC time varying magnetic field up to some tens of kilohertz
Relatori
Anno Accademico
Tipo di pubblicazione
Numero di pagine
Informazioni aggiuntive
Corso di laurea
Classe di laurea
Aziende collaboratrici
URI
![]() |
Modifica (riservato agli operatori) |
