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Nec eu velit latine, sit an graeci legendos voluptaria. Eius tempor eu nec, vix no mutat lucilius comprehensam. Cum debet praesent tincidunt id, noster prompta denique quo ad, erant maluisset eloquentiam sit et. Postea noster usu in, quod laudem cu nam. Simul voluptatum mei ad....

Nec eu velit latine, sit an graeci legendos voluptaria. Eius tempor eu nec, vix no mutat lucilius comprehensam. Cum debet praesent tincidunt id, noster prompta denique quo ad, erant maluisset eloquentiam sit et. Postea noster usu in, quod laudem cu nam. Simul voluptatum mei ad....

Nec eu velit latine, sit an graeci legendos voluptaria. Eius tempor eu nec, vix no mutat lucilius comprehensam. Cum debet praesent tincidunt id, noster prompta denique quo ad, erant maluisset eloquentiam sit et. Postea noster usu in, quod laudem cu nam. Simul voluptatum mei ad....

Nec eu velit latine, sit an graeci legendos voluptaria. Eius tempor eu nec, vix no mutat lucilius comprehensam. Cum debet praesent tincidunt id, noster prompta denique quo ad, erant maluisset eloquentiam sit et. Postea noster usu in, quod laudem cu nam. Simul voluptatum mei ad....

Mitor 2015-2016Spectral Analysis of the Solar Wind beyond the Termination shock - Interstellar Medium/Heliosphere InteractionsThe solar wind fills the heliosphere surrounding the Sun with a supersonic flow of magnetized plasma. At the border of the heliosphere, after the termination shock, the solar wind meets the...

NASA ROSES 2015Title: Spectral analysis of the plasma and magnetic fields at the edge of the heliosphere using Voyager dataPartners:Politecnico di TorinoMIT Kavli Institute (J.Richardson)Boston University (M.Opher)We propose to characterize the turbulence in the solar wind, heliosheath, and local interstellar medium. We are developing an advanced spectral...