Zobrazeno 1 - 10
of 58
pro vyhledávání: '"Romanelli , Norberto"'
Autor:
Andrés, Nahuel, Romanelli, Norberto, Mazelle, Christian, Chen, Li-Jen, Gruesbeck, Jacob R., Espley, Jared R.
Using Mars Atmosphere and Volatile EvolutioN Magnetometer observations, we report the first statistical study of ultra-low frequency (ULF) waves at the Martian foreshock. The analyzed foreshock ULF wave events are observed in the 0.008-0.086 Hz frequ
Externí odkaz:
http://arxiv.org/abs/2408.09003
Autor:
Romanelli, Norberto, Andres, Nahuel, DiBraccio, Gina, Verniero, Jaye, Gruesbeck, Jacob, Szabo, Adam, Espley, Jared, Halekas, Jasper
Solar wind turbulence is a dynamical phenomenon that evolves with heliocentric distance. Orbiting Mars since September 2014, Mars Atmosphere and Volatile EvolutioN (MAVEN) offers a unique opportunity to explore some of its main properties beyond ~1.3
Externí odkaz:
http://arxiv.org/abs/2406.18349
Autor:
Romanelli, Norberto, Fowler, Christopher M., DiBraccio, Gina A., Espley, Jared R., Halekas, Jasper S.
The solar wind upstream of Mars's bow shock can be described in terms of Alfv\'enic turbulence, with an incompressible energy cascade rate of $10^{-17}$ J m$^{-3}$ s$^{-1}$ at magnetohydrodynamics (MHD) scales. The solar wind has more Alfv\'en waves
Externí odkaz:
http://arxiv.org/abs/2403.17304
We present a statistical analysis on the variability of the incompressible energy cascade rate in the solar wind around Mars, making use of an exact relation for fully developed turbulence and more than five years of Mars Atmosphere and Volatile Evol
Externí odkaz:
http://arxiv.org/abs/2201.11772
Autor:
Andrés, Nahuel, Romanelli, Norberto, Hadid, Lina Z., Sahraoui, Fouad, DiBraccio, Gina, Halekas, Jasper
The first estimation of the incompressible energy cascade rate at magnetohydrodynamic (MHD) scales is obtained in the plasma upstream of the Martian bow shock, using MAVEN observations and an exact relation derived for MHD turbulence. The energy casc
Externí odkaz:
http://arxiv.org/abs/2007.09476
The non-collisional interaction between conducting obstacles and magnetized plasma winds can be found in different scenarios, from the interaction occurring between regions inside galaxy clusters to the interaction between the solar wind and Mars, Ve
Externí odkaz:
http://arxiv.org/abs/1406.4779
Autor:
Bertucci, Cesar, Romanelli, Norberto, Chaufray, Jean-Yves, Gomez, Daniel, Mazelle, Christian, Delva, Magda, Modolo, Ronan, Gonzalez-Galindo, Francisco, Brain, David Andrew
We report on the temporal variability of the occurrence of waves at the local proton cyclotron frequency upstream from the Martian bow shock from Mars Global Surveyor observations during the first aerobraking and science phasing orbit periods. Observ
Externí odkaz:
http://arxiv.org/abs/1304.7264
We present a study on the properties of electromagnetic plasma waves in the region upstream of the Martian bow shock, detected by the magnetometer and electron reflectometer (MAG / ER) onboard the Mars Global Surveyor (MGS) spacecraft during the peri
Externí odkaz:
http://arxiv.org/abs/1302.3312
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