Zobrazeno 1 - 10
of 44
pro vyhledávání: '"Martinović, Mihailo M."'
Autor:
Sioulas, Nikos, Zikopoulos, Themistocles, Shi, Chen, Velli, Marco, Bowen, Trevor, Mallet, Alfred, Sorriso-Valvo, Luca, Verdini, Andrea, Chandran, B. D. G., Martinović, Mihailo M., Cerri, S. S., Davis, Nooshin, Dunn, Corina
We analyze in-situ observations of imbalanced solar wind turbulence to evaluate MHD turbulence models grounded in "Critical Balance" (CB) and "Scale-Dependent Dynamic Alignment" (SDDA). At energy injection scales, both outgoing and ingoing modes exhi
Externí odkaz:
http://arxiv.org/abs/2404.04055
Linear theory is a well developed framework for characterizing instabilities in weakly collisional plasmas, such as the solar wind. In the previous instalment of this series, we analyzed ~1.5M proton and alpha particle Velocity Distribution Functions
Externí odkaz:
http://arxiv.org/abs/2306.06060
Autor:
Huang, Jia, Kasper, J. C., Fisk, L. A., Larson, Davin E., McManus, Michael D., Chen, C. H. K., Martinović, Mihailo M., Klein, K. G., Thomas, Luke, Liu, Mingzhe, Maruca, Bennett A., Zhao, Lingling, Chen, Yu, Hu, Qiang, Jian, Lan K., Verniero, J. L., Velli, Marco, Livi, Roberto, Whittlesey, P., Rahmati, Ali, Romeo, Orlando, Niembro, Tatiana, Paulson, Kristoff, Stevens, M., Case, A. W., Pulupa, Marc, Bale, Stuart D., Halekas, J. S.
Switchbacks are rapid magnetic field reversals that last from seconds to hours. Current Parker Solar Probe (PSP) observations pose many open questions in regard to the nature of switchbacks. For example, are they stable as they propagate through the
Externí odkaz:
http://arxiv.org/abs/2301.10374
The heating of ions and electrons due to turbulent dissipation plays a crucial role in the thermodynamics of the solar wind and other plasma environments. Using magnetic field and thermal plasma observations from the first two perihelia of the Parker
Externí odkaz:
http://arxiv.org/abs/2301.09713
Instabilities described by linear theory characterize an important form of wave-particle interaction in the solar wind. We diagnose unstable behavior of solar wind plasma between 0.3 and 1 au via the Nyquist criterion, applying it to fits of $\sim1.5
Externí odkaz:
http://arxiv.org/abs/2110.07772
A growing body of evidence suggests that the solar wind is powered to a large extent by an Alfv\'en-wave (AW) energy flux. AWs energize the solar wind via two mechanisms: heating and work. We use high-resolution direct numerical simulations of reflec
Externí odkaz:
http://arxiv.org/abs/2103.09365
Autor:
Martinović, Mihailo M., Klein, Kristopher G., Huang, Jia, Chandran, Benjamin D. G., Kasper, Justin C., Lichko, Emily, Bowen, Trevor, Chen, Christopher H. K., Matteini, Lorenzo, Stevens, Michael, Case, Anthony W., Bale, Stuart D.
Parker Solar Probe (PSP) routinely observes magnetic field deflections in the solar wind at distances less than 0.3 au from the Sun. These deflections are related to structures commonly called 'switchbacks' (SBs), whose origins and characteristic pro
Externí odkaz:
http://arxiv.org/abs/2103.00374
Autor:
Vech, Daniel, Martinovic, Mihailo M., Klein, Kristopher G., Malaspina, David M., Bowen, Trevor A., Verniero, Jenny L., Paulson, Kristoff, de Wit, Thierry Dudok, Kasper, Justin C., Huang, Jia, Stevens, Michael L., Case, Anthony W., Korreck, Kelly, Mozer, Forrest S., Goodrich, Katherine A., Bale, Stuart D., Whittlesey, Phyllis L., Livi, Roberto, Larson, Davin E., Pulupa, Marc, Bonnell, John, Harvey, Peter, Goetz, Keith, MacDowall, Robert
Context. The first studies with Parker Solar Probe (PSP) data have made significant progress toward the understanding of the fundamental properties of ion cyclotron waves in the inner heliosphere. The survey mode particle measurements of PSP, however
Externí odkaz:
http://arxiv.org/abs/2010.15189
Autor:
Woolley, Thomas, Matteini, Lorenzo, Horbury, Timothy S., Bale, Stuart D., Woodham, Lloyd D., Laker, Ronan, Alterman, Benjamin L., Bonnell, John W., Case, Anthony W., Kasper, Justin C., Klein, Kristopher G., Martinović, Mihailo M., Stevens, Michael
During Parker Solar Probe's first two orbits there are widespread observations of rapid magnetic field reversals known as switchbacks. These switchbacks are extensively found in the near-Sun solar wind, appear to occur in patches, and have possible l
Externí odkaz:
http://arxiv.org/abs/2007.10906
Autor:
Huang, Jia, Kasper, J. C., Stevens, M., Vech, D., Klein, K. G., Martinović, Mihailo M., Alterman, B. L., Jian, Lan K., Hu, Qiang, Velli, Marco, Horbury, Timothy S., Lavraud, B., Parashar, T. N., Ďurovcová, Tereza, Niembro, Tatiana, Paulson, Kristoff, Hegedus, A., Bert, C. M., Holmes, J., Case, A. W., Korreck, K. E., Bale, Stuart D., Larson, Davin E., Livi, Roberto, Whittlesey, P., Pulupa, Marc, de Wit, Thierry Dudok, Malaspina, David M., MacDowall, Robert J., Bonnell, John W., Harvey, Peter R., Goetz, Keith
The slow solar wind is typically characterized as having low Alfv\'enicity. However, Parker Solar Probe (PSP) observed predominately Alfv\'enic slow solar wind during several of its initial encounters. From its first encounter observations, about 55.
Externí odkaz:
http://arxiv.org/abs/2005.12372