HelioWebUniversity of Florence, Department of Astronomy and Space Science
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- 3D MHD description of the region beyond the termination shock: The behaviour of the Current Sheet
- Simulations of wave particle interactions in the expanding solar wind in the presence of particle beams
- Alfvén Wave Reflection and Turbulence in the Solar Corona and Solar Wind
- Magnetic Effects at the Edge of the Solar System: MHD Instabilities, the de Laval nozzle effect and an Extended Jet
- Successful Measurement of the Full Magnetic Vector Near the Base of the Solar Corona
- A Detection of the Same Hot Plasma in the Corona - During a CME - and Later at Ulysses
- Acceleration of the Weakly Collisional Solar Wind
- HERSCHEL Suborbital Program: 3-D Applications for the STEREO Mission
- High Latitude Magnetic Field Polarity Reversals: A Solar Source or In Situ Generation?
- Alfvénic Turbulence and Micro-Stream Structure in the Polar Solar Wind.
- Reduced MHD and Shell-Model Simulations of Coronal Heating in Magnetized Loops: Scaling Laws.
- Coronal heating and solar wind acceleration by turbulence
- Density and magnetic field signatures of interplanetary 1/f noise
- Acceleration of the Solar Wind: a Review of Kinetic Collisionless (Exospheric) Models
- The evolution of the solar wind proton temperature anisotropy from 0.3 to 2.5 AU
- Fine-Structured Plasma Flows in Prominences
- Proton Cyclotron Heating and Beam Generation in the Solar Wind
- Kinetics of the Solar Wind Expansion: Wave-Particle Interactions and Ion Distribution Functions
- On the competition between radial expansion and Coulomb collisions in shaping the electron velocity distribution function: Kinetic simulations
- Parametric Decay of Obliquely Propagating Alfvén Waves: Transverse Coupling and Proton Parallel Acceleration
- The anisotropic turbulent cascade at high frequencies, the effects of instabilities and the correct way to measure magnetic fields when considering small scales.
- Alfvénic Turbulence and Kinetic Instabilities in the Expanding Solar Wind: Two-Dimensional Hybrid Simulations
- Beyond the Maltese Cross: Geometry of Turbulence between 0.2 and 1 AU
- MURAVES: An experiment of muon radiography at Vesuvius
- Muon radiography of the Temperino mine in Campiglia Marittima: average density measurement and detection of unknown cavities
- Numerical Simulations of Kinetic Turbulence in the Low Beta Regime: Predictions for Observations by Parker Solar Probe
- An experiment of muography at Vesuvius (Italy)
- Disentangling coherent structures and wave-like perturbations in Hall-MHD and Hybrid-PIC simulations of plasma turbulence with Multidimensional Iterative Filters.
- Interpreting Parker Solar Probe's observations with high-resolution hybrid particle-in-cell simulations
- Plasma Turbulence vs. Fire Hose Instabilities: Hybrid Expanding Box Simulations
- Karman-Howarth-Monin equation for compressible Hall MHD turbulence