AL
Member Since 2019
Andrea Larosa
Postdoctoral research assistant, CNR National Research Council
AGU Research
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On the phase space cascade evolution with Parker Solar Probe
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Andrea Larosa, Oreste Pezzi, Trevor Bowen, Domenic...
In space plasmas, due to the absence of collisions, the phase space shows a complex structuring and strong deviations from the thermal equilibrium. Pr...
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Microstructure at a fully formed Forward-Reverse Shock pair due to the interaction between two Coronal Mass Ejections observed at 0.5 AU.
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Xochitl Blanco-Cano, Domenico Trotta, Heli Hietala...
Interplanetary (IP) shocks are often driven in the solar wind by fast coronal mass ejections, and by the interaction of fast solar wind with slow stre...
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Solar Orbiter Observations of Interplanetary Shocks at Short Heliocentric Distances
AGU 2024
spa-solar and heliospheric physics | 10 december 2024
Domenico Trotta, Heli Hietala, Timothy S. Horbury,...
Interplanetary (IP) shocks are important sites of particle acceleration in the Heliosphere and can be observed in-situ utilizing spacecraft measuremen...
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Acceleration of relativistic electron beams by a strong interplanetary shock at 1 AU
ACCELERATION AND TRANSPORT OF SUPRATHERMAL AND ENERGETIC PARTICLES IN THE INNER HELIOSPHERE: OBSERVATIONS AND MODELING III POSTER
spa-solar and heliospheric physics | 15 december 2023
Immanuel Christopher Jeba Raj, Domenico Trotta, Ni...
Collisionless shocks in the heliosphere such as planetary bow shocks and CME-driven shocks play a significant role as particle accelerators. These sho...
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Observations of the Turbulence Transition Range as Evidence for the Helicity Barrier
TURBULENCE, MAGNETIC RECONNECTION, PARTICLE ENERGIZATION, AND FUNDAMENTAL PLASMA PROCESSES IN SPACE PLASMA I POSTER
spa-solar and heliospheric physics | 14 december 2023
Jack McIntyre, Christopher H. Chen, Andrea Larosa
The means by which energy is dissipated in solar wind turbulence, a process which can heat and accelerate the solar wind, is not fully understood. Obs...
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On the Relation between Magnetic Switchbacks and Turbulence in the Inner Heliosphere in Different Solar Wind Streams
FUNDAMENTAL PHYSICS OF THE SOLAR CORONA AND INNER HELIOSPHERE I ORAL
spa-solar and heliospheric physics | 13 december 2023
Andrea Larosa, Christopher H. Chen, Jack McIntyre,...
In a previous work (Larosa+2023 in prep) we investigated the radial evolution of the magnetic field vector increment and rotation distributions for di...
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The interplay between magnetic switchbacks and solar wind turbulence in the inner Heliosphere
FUNDAMENTAL PHYSICS OF THE SOLAR CORONA AND INNER HELIOSPHERE II POSTER
spa-solar and heliospheric physics | 15 december 2022
Andrea Larosa, Christopher H. Chen
Since its launch Parker Solar Probe has surprised us with many new results. Among these are the ubiquitous large-amplitude deflections of the magnetic...
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First Results From the SCM Search‐Coil Magnetometer on Parker Solar Probe
JOURNAL OF GEOPHYSICAL RESEARCH: SPACE PHYSICS
17 april 2022
Thierry Dudok de Wit, Vladimir Krasnoselskikh, Ole...
Parker Solar Probe is the first mission to probe in situ the innermost heliosphere, revealing an exceptionally dynamic and structured outer solar c...