Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity

Nahuel Andrés (1) , Norberto Romanelli (2, 3) , L. Z. Hadid (4, 5) , Fouad Sahraoui (4) , Gina Dibraccio (3) , Jasper Halekas (6)

1 UBA - Universidad de Buenos Aires [Buenos Aires]
2 CRESST, University of Maryland, Baltimore County, Baltimore, MD, USA
3 GSFC - NASA Goddard Space Flight Center
4 LPP - Laboratoire de Physique des Plasmas
5 ESA - ESTEC (Netherlands)
6 University of Iowa [Iowa City]

Domaines: Astrophysique stellaire et solaire [astro-ph.SR]; Planétologie et astrophysique de la terre [astro-ph.EP]; Physique des plasmas [physics.plasm-ph]

Nahuel Andrés, Norberto Romanelli, L. Z. Hadid, Fouad Sahraoui, Gina Dibraccio, et al.. Solar Wind Turbulence Around Mars: Relation between the Energy Cascade Rate and the Proton Cyclotron Waves Activity. The Astrophysical Journal, 2020, 902 (2), pp.134. ⟨10.3847/1538-4357/abb5a7⟩. ⟨hal-03779500⟩