Zobrazeno 1 - 10
of 86
pro vyhledávání: '"Korreck, Kelly E"'
Autor:
Telloni, Daniele, Andretta, Vincenzo, Antonucci, Ester, Bemporad, Alessandro, Capuano, Giuseppe E., Fineschi, Silvano, Giordano, Silvio, Habbal, Shadia, Perrone, Denise, Pinto, Rui F., Sorriso-Valvo, Luca, Spadaro, Daniele, Susino, Roberto, Woodham, Lloyd D., Zank, Gary P., Romoli, Marco, Bale, Stuart D., Kasper, Justin C., Auchère, Frédéric, Bruno, Roberto, Capobianco, Gerardo, Case, Anthony W., Casini, Chiara, Casti, Marta, Chioetto, Paolo, Corso, Alain J., Da Deppo, Vania, De Leo, Yara, de Wit, Thierry Dudok, Frassati, Federica, Frassetto, Fabio, Goetz, Keith, Guglielmino, Salvo L., Harvey, Peter R., Heinzel, Petr, Jerse, Giovanna, Korreck, Kelly E., Landini, Federico, Larson, Davin, Liberatore, Alessandro, Livi, Roberto, MacDowall, Robert J., Magli, Enrico, Malaspina, David M., Massone, Giuseppe, Messerotti, Mauro, Moses, John D., Naletto, Giampiero, Nicolini, Gianalfredo, Nisticò, Giuseppe, Panasenco, Olga, Pancrazzi, Maurizio, Pelizzo, Maria G., Pulupa, Marc, Reale, Fabio, Romano, Paolo, Sasso, Clementina, Schühle, Udo, Stangalini, Marco, Stevens, Michael L., Strachan, Leonard, Straus, Thomas, Teriaca, Luca, Uslenghi, Michela, Velli, Marco, Verscharen, Daniel, Volpicelli, Cosimo A., Whittlesey, Phyllis, Zangrilli, Luca, Zimbardo, Gaetano, Zuppella, Paola
Publikováno v:
Telloni, D., Andretta, V., Antonucci, E., et al. 2021, ApJL, 920, L14
This Letter addresses the first Solar Orbiter (SO) -- Parker Solar Probe (PSP) quadrature, occurring on January 18, 2021, to investigate the evolution of solar wind from the extended corona to the inner heliosphere. Assuming ballistic propagation, th
Externí odkaz:
http://arxiv.org/abs/2110.11031
Autor:
Fargette, Naïs, Lavraud, Benoit, Rouillard, Alexis, Réville, Victor, De Wit, Thierry Dudok, Froment, Clara, Halekas, Jasper S., Phan, Tai, Malaspina, David, Bale, Stuart D., Kasper, Justin, Louarn, Philippe, Case, Anthony W., Korreck, Kelly E., Larson, Davin E., Pulupa, Marc, Stevens, Michael L., Whittlesey, Phyllis L., Berthomier, Matthieu
Parker Solar Probe (PSP) data recorded within a heliocentric radial distance of 0.3 AU have revealed a magnetic field dominated by Alfv\'enic structures that undergo large local variations or even reversals of the radial magnetic field. They are call
Externí odkaz:
http://arxiv.org/abs/2109.01519
Autor:
Bercic, Laura, Maksimovic, Milan, Halekas, Jasper S., Landi, Smone, Owen, Christopher J., Verscharen, Daniel, Larson, Davin, Whittlesey, Phyllis, Badman, Samuel T., Bale, Stuart. D., Case, Anthony W., Goetz, Keith, Harvey, Peter R., Kasper, Justin C., Korreck, Kelly E., Livi, Roberto, MacDowall, Robert J., Malaspina, David M., Pulupa, Marc, Stevens, Michael L.
The solar wind escapes from the solar corona and is accelerated, over a short distance, to its terminal velocity. The energy balance associated with this acceleration remains poorly understood. To quantify the global electrostatic contribution to the
Externí odkaz:
http://arxiv.org/abs/2108.08528
The Contribution of Alpha Particles to the Solar Wind Angular Momentum Flux in the Inner Heliosphere
Autor:
Finley, Adam J., McManus, Michael D., Matt, Sean P., Kasper, Justin C., Korreck, Kelly E., Case, Anthony W., Stevens, Michael L., Whittlesey, Phyllis, Larson, Davin, Livi, Roberto, Bale, Stuart D., de Wit, Thierry Dudok, Goetz, Keith, Harvey, Peter R., MacDowall, Robert J., Malaspina, David M., Pulupa, Marc
Publikováno v:
A&A 650, A17 (2021)
An accurate assessment of the Sun's angular momentum (AM) loss rate is an independent constraint for models that describe the rotation evolution of Sun-like stars. In-situ measurements of the solar wind taken by Parker Solar Probe (PSP), at radial di
Externí odkaz:
http://arxiv.org/abs/2011.00016
Autor:
Laker, Ronan, Horbury, Timothy S., Bale, Stuart D., Matteini, Lorenzo, Woolley, Thomas, Woodham, Lloyd D., Badman, Samuel T., Pulupa, Marc, Kasper, Justin C., Stevens, Michael, Case, Anthony W., Korreck, Kelly E.
Publikováno v:
A&A 650, A1 (2021)
One of the main discoveries from the first two orbits of Parker Solar Probe (PSP) was the presence of magnetic switchbacks, whose deflections dominated the magnetic field measurements. Determining their shape and size could provide evidence of their
Externí odkaz:
http://arxiv.org/abs/2010.10211
Autor:
Finley, Adam J., Matt, Sean P., Réville, Victor, Pinto, Rui F., Owens, Mathew, Kasper, Justin C., Korreck, Kelly E., Case, A. W., Stevens, Michael L., Whittlesey, Phyllis, Larson, Davin, Livi, Roberto
The long-term evolution of the Sun's rotation period cannot be directly observed, and is instead inferred from trends in the measured rotation periods of other Sun-like stars. Assuming the Sun spins-down as it ages, following rotation rate $\propto$
Externí odkaz:
http://arxiv.org/abs/2009.08991
Autor:
Chen, Yu, Hu, Qiang, Zhao, Lingling, Kasper, Justin C., Bale, Stuart D., Korreck, Kelly E., Case, Anthony W., Stevens, Michael L., Bonnell, John W., Goetz, Keith, Harvey, Peter R., Klein, Kristopher G., Larson, Davin E., Livi, Roberto, MacDowall, Robert J., Malaspina, David M., Pulupa, Marc, Whittlesey, Phyllis L.
Small-scale magnetic flux ropes (SFRs) are a type of structures in the solar wind that possess helical magnetic field lines. In a recent report (Chen & Hu 2020), we presented the radial variations of the properties of SFR from 0.29 to 8 au using in s
Externí odkaz:
http://arxiv.org/abs/2007.04551
Autor:
Bercic, Laura, Larson, Davin, Whittlesey, Phyllis, Maksimovic, Milan, Badman, Samuel T., Landi, Simone, Matteini, Lorenzo, Bale, Stuart. D., Bonnell, John W., Case, Anthony W., de Wit, Thierry Dudok, Goetz, Keith, Harvey, Peter R., Kasper, Justin C., Korreck, Kelly E., Livi, Roberto, MacDowall, Robert J., Malaspina, David M., Pulupa, Marc, Stevens, Michael L.
The shape of the electron velocity distribution function plays an important role in the dynamics of the solar wind acceleration. Electrons are normally modelled with three components, the core, the halo, and the strahl. We investigate how well the fa
Externí odkaz:
http://arxiv.org/abs/2003.04016
Autor:
Whittlesey, Phyllis L, Larson, Davin E, Kasper, Justin C, Halekas, Jasper, Abatcha, Mamuda, Abiad, Robert, Berthomier, M., Case, A. W., Chen, Jianxin, Curtis, David W, Dalton, Gregory, Klein, Kristopher G, Korreck, Kelly E, Livi, Roberto, Ludlam, Michael, Marckwordt, Mario, Rahmati, Ali, Robinson, Miles, Slagle, Amanda, Stevens, M L, Tiu, Chris, Verniero, J L
Electrostatic analyzers of different designs have been used since the earliest days of the space age, beginning with the very earliest solar wind measurements made by Mariner 2 en route to Venus in 1962. The Parker Solar Probe (PSP) mission, NASA's f
Externí odkaz:
http://arxiv.org/abs/2002.04080
Autor:
Duan, Die, Bowen, Trevor A., Chen, Christopher H. K., Mallet, Alfred, He, Jiansen, Bale, Stuart D., Vech, Daniel, Kasper, J. C., Pulupa, Marc, Bonnell, John W., Case, Anthony W., de Wit, Thierry Dudok, Goetz, Keith, Harvey, Peter R., Korreck, Kelly E., Larson, Davin, Livi, Roberto, MacDowall, Robert J., Malaspina, David M., Stevens, Michael, Whittlesey, Phyllis
Magnetic field fluctuations in the solar wind are commonly observed to follow a power law spectrum. Near proton-kinetic scales, a spectral break occurs which is commonly interpreted as a transition to kinetic turbulence. However, this transition is n
Externí odkaz:
http://arxiv.org/abs/2001.08239