LM
Lorenzo Matteini
Imperial College London
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Magnetic confinement fusion research
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Publications (82)
- Solar-wind proton heating and its effect on the temperature anisotropy evolution between 0.05 and 1 au Save
- Magnetic Switchback Formation: A Review of Proposed Mechanisms Save
- Electron temperatures in the ionosphere of Venus from Solar Orbiter/Radio and Plasma Waves instrument Save
- Evolution of ion distribution functions in ionospheric plasmas perturbed by Alfvén waves Save
- Effect of Turbulence Amplitude and Correlation Length on Magnetic Reconnection Dynamics in Hybrid Simulations of Collisionless Plasmas Save
- Energy exchanges between particles and ion-scale waves and structures in space plasmas with multi-scale explorations: insights from numerical simulations Save
- Fluxgate Magnetic Field Instrument for Seven Small Plasma Observatory Spacecraft Save
- Evolution of an Alfvén Wave–driven Proton Beam in the Expanding Solar Wind Save
- Fluid and Kinetic Properties of the Near-Sun Heliospheric Current Sheet Save
- Properties of Magnetic Switchbacks in the Near-Sun Solar Wind Save
- Ion-scale Solitary Structures in the Solar Wind Observed by Solar Orbiter and Parker Solar Probe Save
- Observational Constraints on the Radial Evolution of O6+ Temperature and Differential Flow in the Inner Heliosphere Save
- Two Types of 1/f Range in Solar Wind Turbulence Save
- Evolution of ion distribution functions in ionospheric plasmas perturbed by Alfvén waves Save
- On the role of mirror mode instabilities in the reconnecting Heliospheric Current Sheet dynamics Save
- The MAG-M magnetometer onboard Plasma Observatory Save
- The Plasma Observatory FIELDS-M instrument suite Save
- Energy transfer in the Solar Wind: The interplay between turbulence and kinetic instabilities. Save
- Alpha–Proton Relative Drift: Implications for the Origins and Dynamics of the Solar Wind Save
- Temperature anisotropy instabilities driven by intermittent velocity shears in the solar wind Save