Zobrazeno 1 - 10
of 329
pro vyhledávání: '"Maksimovic Milan"'
Autor:
Vecchio, Antonio, Maksimovic, Milan, Chrysaphi, Nicolina, Kontar, Eduard P., Krupar, Vratislav
Publikováno v:
The Astrophysical Journal Letters, 974:L18 (18pp), 2024 October 10
Radio observations from space allow to characterize solar radio bursts below the ionospheric cutoff, which are otherwise inaccessible, but suffer from low, insufficient temporal resolution. In this Letter we present novel, high-temporal resolution ob
Externí odkaz:
http://arxiv.org/abs/2410.18765
Autor:
Chrysaphi, Nicolina, Maksimovic, Milan, Kontar, Eduard P., Vecchio, Antonio, Chen, Xingyao, Pesini, Aikaterini
Radio photons interact with anisotropic density fluctuations in the heliosphere, which can alter their trajectory and influence properties deduced from observations. This is particularly evident in solar radio observations, where anisotropic scatteri
Externí odkaz:
http://arxiv.org/abs/2404.01497
Publikováno v:
A&A 686, A114 (2024)
Configurations where two spacecraft, such as Parker Solar Probe (PSP) and Solar Orbiter (SolO), are radially aligned provide opportunities to study the evolution of a single solar wind parcel during so called plasma line-ups. The most critical part o
Externí odkaz:
http://arxiv.org/abs/2402.12382
Autor:
Zaslavsky, Arnaud, Kasper, Justin C., Kontar, Eduard P., Larson, Davin E., Maksimovic, Milan, Marques, José M. D. C., Nicolaou, Georgios, Owen, Christopher J., Romeo, Orlando, Whittlesey, Phyllis L.
This study explores the impact of a turbulent scattering mechanism, akin to those influencing solar and galactic cosmic rays propagating in the interplanetary medium, on the population of suprathermal electrons in the solar wind. We employ a Fokker-P
Externí odkaz:
http://arxiv.org/abs/2401.04222
Autor:
Lorfing, Camille Y., Reid, Hamish A. S., Gomez-Herrero, Raul, Maksimovic, Milan, Nicolaou, Georgios, Owen, Christopher J., Rodriguez-Pacheco, Javier, Ryan, Daniel F., Trotta, Domenico, Verscharen, Daniel
Solar Orbiter's four in-situ instruments have recorded numerous energetic electron events at heliocentric distances between 0.5 and 1au. We analyse energetic electron fluxes, spectra, pitch angle distributions, associated Langmuir waves, and type III
Externí odkaz:
http://arxiv.org/abs/2311.14444
Autor:
Vinogradov, Alexander, Alexandrova, Olga, Démoulin, Pascal, Artemyev, Anton, Maksimovic, Milan, Mangeney, André, Vasiliev, Alexei, Petrukovich, Anatoly, Bale, Stuart
We study intermittent coherent structures in solar wind magnetic turbulence from MHD to kinetic plasma scales using Parker Solar Probe data during its first perihelion (at 0.17 au), when the satellite was in the Alfv\'enic slow wind of 340 km/s. The
Externí odkaz:
http://arxiv.org/abs/2307.10478
Autor:
Chen, Xingyao, Kontar, Eduard P., Chrysaphi, Nicolina, Zhang, Peijin, Krupar, Vratislav, Musset, Sophie, Maksimovic, Milan, Jeffrey, Natasha L. S., Azzollini, Francesco, Vecchio, Antonio
Publikováno v:
A&A 680, A1 (2023)
Interplanetary solar radio type III bursts provide the means for remotely studying and tracking energetic electrons propagating in the interplanetary medium. Due to the lack of direct radio source imaging, several methods have been developed to deter
Externí odkaz:
http://arxiv.org/abs/2306.09160
Autor:
Bale, Stuart D., Bassett, Neil, Burns, Jack O., Jones, Johnny Dorigo, Goetz, Keith, Hellum-Bye, Christian, Hermann, Sven, Hibbard, Joshua, Maksimovic, Milan, McLean, Ryan, Monsalve, Raul, O'Connor, Paul, Parsons, Aaron, Pulupa, Marc, Pund, Rugved, Rapetti, David, Rotermund, Kaja M., Saliwanchik, Ben, Slosar, Anze, Sundkvist, David, Suzuki, Aritoki
The Lunar Surface Electromagnetics Explorer 'LuSEE Night' is a low frequency radio astronomy experiment that will be delivered to the farside of the Moon by the NASA Commercial Lunar Payload Services (CLPS) program in late 2025 or early 2026. The pay
Externí odkaz:
http://arxiv.org/abs/2301.10345
Autor:
Shi, Chen, Velli, Marco, Lionello, Roberto, Sioulas, Nikos, Huang, Zesen, Halekas, Jasper S., Tenerani, Anna, Réville, Victor, Dakeyo, Jean-Baptiste, Maksimović, Milan, Bale, Stuart D.
The heating and acceleration of the solar wind remains one of the fundamental unsolved problems in heliophysics. It is usually observed that the proton temperature $T_i$ is highly correlated with the solar wind speed $V_{SW}$, while the electron temp
Externí odkaz:
http://arxiv.org/abs/2301.00852
Autor:
Shi, Chen, Velli, Marco, Bale, Stuart D., Réville, Victor, Maksimović, Milan, Dakeyo, Jean-Baptiste
The acceleration of the solar coronal plasma to supersonic speeds is one of the most fundamental yet unresolved problem in heliophysics. Despite the success of Parker's pioneering theory on an isothermal solar corona, the realistic solar wind is obse
Externí odkaz:
http://arxiv.org/abs/2209.03508