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pro vyhledávání: '"Mcmanus, Michael"'
Autor:
Bowen, Trevor A., Vasko, Ivan Y., Bale, Stuart D., Chandran, Benjamin D. G., Chasapis, Alexandros, de Wit, Thierry Dudok, Mallet, Alfred, McManus, Michael, Meyrand, Romain, Pulupa, Marc, Squire, Jonathan
Circularly polarized, nearly parallel propagating waves are prevalent in the solar wind at ion-kinetic scales. At these scales, the spectrum of turbulent fluctuations in the solar wind steepens, often called the transition-range, before flattening at
Externí odkaz:
http://arxiv.org/abs/2406.10446
Autor:
McManus, Michael D., Klein, Kristopher G., Larson, Davin, Bale, Stuart D., Bowen, Trevor A., Huang, Jia, Livi, Roberto, Rahmati, Ali, Romeo, Orlando, Verniero, Jaye, Whittlesey, Phyllis
Ion scale wave events or "wave storms" in the solar wind are characterised by enhancements in magnetic field fluctuations as well as coherent magnetic field polarisation signatures at or around the local ion cyclotron frequencies. In this paper we st
Externí odkaz:
http://arxiv.org/abs/2310.14136
Autor:
Ofman, Leon, Boardsen, Scott A, Jian, Lan K, Mostafavi, Parisa, Verniero, Jaye L, Livi, Roberto, McManus, Michael, Rahmati, Ali, Larson, Davin, Stevens, Michael L
Past observations show that solar wind (SW) acceleration occurs inside the sub-Alfvenic region, reaching the local Alfven speed at typical distances ~ 10 - 20 Rs (solar radii). Recently, Parker Solar Probe (PSP) traversed regions of sub-Alfvenic SW n
Externí odkaz:
http://arxiv.org/abs/2307.13410
Autor:
Huang, Jia, Kasper, Justin C., Larson, Davin E., McManus, Michael D., Whittlesey, Phyllis, Livi, Roberto, Rahmati, Ali, Romeo, Orlando M., Liu, Mingzhe, Jian, Lan K., Verniero, J. L., Velli, Marco, Badman, Samuel T., Rivera, Yeimy J., Niembro, Tatiana, Paulson, Kristoff, Stevens, Michael L., Case, Anthony W., Bowen, Trevor A., Pulupa, Marc, Bale, Stuart D., Halekas, Jasper S.
Publikováno v:
ApJ 954 133 (2023)
Parker Solar Probe (PSP) observes unexpectedly prevalent switchbacks, which are rapid magnetic field reversals that last from seconds to hours, in the inner heliosphere, posing new challenges to understanding their nature, origin, and evolution. In t
Externí odkaz:
http://arxiv.org/abs/2306.04773
Autor:
Huang, Jia, Kasper, J. C., Larson, Davin E., McManus, Michael D., Whittlesey, P., Livi, Roberto, Rahmati, Ali, Romeo, Orlando, Klein, K. G., Sun, Weijie, van der Holst, Bart, Huang, Zhenguang, Jian, Lan K., Szabo, Adam, Verniero, J. L., Chen, C. H. K., Lavraud, B., Liu, Mingzhe, Badman, Samuel T., Niembro, Tatiana, Paulson, Kristoff, Stevens, M., Case, A. W., Pulupa, Marc, Bale, Stuart D., Halekas, J. S.
In general, slow solar wind from the streamer belt forms a high plasma beta equatorial plasma sheet around the heliospheric current sheet (HCS) crossing, namely the heliospheric plasma sheet (HPS). Current Parker Solar Probe (PSP) observations show t
Externí odkaz:
http://arxiv.org/abs/2302.07230
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