Zobrazeno 1 - 10
of 2 314
pro vyhledávání: '"Klein, K. P."'
Autor:
Retino, A., Kepko, L., Kucharek, H., Marcucci, M. F., Nakamura, R., Amano, T., Angelopoulos, V., Bale, S. D., Caprioli, D., Cassak, P., Chasapis, A., Chen, L. -J., Dai, L., Dunlop, M. W., Forsyth, C., Fu, H., Galvin, A., Contel, O. Le, Yamauchi, M., Kistler, L., Khotyaintsev, Y., Klein, K., Mann, I. R., Matthaeus, W., Mouikis, K., Nykyri, K., Palmroth, M., Plaschke, F., Saito, Y., Soucek, J., Spence, H., Turner, D. L., Vaivads, A., Valentini, F.
Energetic plasma is everywhere in the Universe. The terrestrial Magnetospheric System is a key case where direct measures of plasma energization and energy transport can be made in situ at high resolution. Despite the large amount of available observ
Externí odkaz:
http://arxiv.org/abs/2311.09920
Space plasma studies frequently use in situ magnetic field measurements taken from many spacecraft simultaneously. A useful data product of these measurements is the reconstructed magnetic field in a volume near the spacecraft observatory. We compare
Externí odkaz:
http://arxiv.org/abs/2310.15187
Autor:
Halekas, J. S., Bale, S. D., Berthomier, M., Chandran, B. D. G., Drake, J. F., Kasper, J. C., Klein, K. G., Larson, D. E., Livi, R., Pulupa, M. P., Stevens, M. L., Verniero, J. L., Whittlesey, P.
A variety of energy sources, ranging from dynamic processes like magnetic reconnection and waves to quasi-steady terms like the plasma pressure, may contribute to the acceleration of the solar wind. We utilize a combination of charged particle and ma
Externí odkaz:
http://arxiv.org/abs/2305.13424
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
Autor:
Raouafi, N. E., Matteini, L., Squire, J., Badman, S. T., Velli, M., Klein, K. G., Chen, C. H. K., Matthaeus, W. H., Szabo, A., Linton, M., Allen, R. C., Szalay, J. R., Bruno, R., Decker, R. B., Akhavan-Tafti, M., Agapitov, O. V., Bale, S. D., Bandyopadhyay, R., Battams, K., Berčič, L., Bourouaine, S., Bowen, T., Cattell, C., Chandran, B. D. G., Chhiber, R., Cohen, C. M. S., D'Amicis, R., Giacalone, J., Hess, P., Howard, R. A., Horbury, T. S., Jagarlamudi, V. K., Joyce, C. J., Kasper, J. C., Kinnison, J., Laker, R., Liewer, P., Malaspina, D. M., Mann, I., McComas, D. J., Niembro-Hernandez, T., Panasenco, O., Pokorný, P., Pusack, A., Pulupa, M., Perez, J. C., Riley, P., Rouillard, A. P., Shi, C., Stenborg, G., Tenerani, A., Verniero, J. L., Viall, N., Vourlidas, A., Wood, B. E., Woodham, L. D., Woolley, T.
Publikováno v:
Space Science Reviews 2023
Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to determine the structure and dynamics of the Sun's coronal magnetic field, understand
Externí odkaz:
http://arxiv.org/abs/2301.02727
Autor:
Matthaeus, W. H., Adhikari, S., Bandyopadhyay, R., Brown, M. R., Bruno, R., Borovsky, J., Carbone, V., Caprioli, D., Chasapis, A., Chhiber, R., Dasso, S., Dmitruk, P., Del Zanna, L., Dmitruk, P. A., Franci, Luca, Gary, S. P., Goldstein, M. L., Gomez, D., Greco, A., Horbury, T. S., Ji, Hantao, Kasper, J. C., Klein, K. G., Landi, S., Li, Hui, Malara, F., Maruca, B. A., Mininni, P., Oughton, Sean, Papini, E., Parashar, T. N., Pecora, F., Petrosyan, Arakel, Pouquet, Annick, Retino, A., Roberts, Owen, Ruffolo, David, Servidio, Sergio, Spence, Harlan, Smith, C. W., Stawarz, J. E., TenBarge, Jason, Vasquez, B. J., Vaivads, Andris, Valentini, F., Velli, Marco, Verdini, A., Verscharen, Daniel, Whittlesey, Phyllis, Wicks, Robert, Yang, Y., Zimbardo, G.
Space plasmas are three-dimensional dynamic entities. Except under very special circumstances, their structure in space and their behavior in time are not related in any simple way. Therefore, single spacecraft in situ measurements cannot unambiguous
Externí odkaz:
http://arxiv.org/abs/2211.12676
Autor:
Verniero, J. L., Chandran, B. D. G., Larson, D. E., Paulson, K., Alterman, B. L., Badman, S., Bale, S. D., Bonnell, J. W., Bowen, T. A., de Wit, T. Dudok, Kasper, J. C., Klein, K. G., Lichko, E., Livi, R., McManus, M. D., Rahmati, A., Verscharen, D., Walters, J., Whittlesey, P. L.
The SWEAP instrument suite on Parker Solar Probe (PSP) has detected numerous proton beams associated with coherent, circularly polarized, ion-scale waves observed by PSP's FIELDS instrument suite. Measurements during PSP Encounters 4-8 revealed prono
Externí odkaz:
http://arxiv.org/abs/2110.08912
Autor:
Dresing, Nina, Warmuth, A., Effenberger, F., Klein, K. -L., Musset, S., Glesener, L., Brüdern, M.
Publikováno v:
A&A 654, A92 (2021)
We compare the characteristics of flare-accelerated energetic electrons at the Sun with those injected into interplanetary space. We have identified 17 energetic electron events well-observed with the SEPT instrument aboard STEREO which show a clear
Externí odkaz:
http://arxiv.org/abs/2108.09045
Autor:
Klein, K. G., Verniero, J. L., Alterman, B., Bale, S., Case, A., Kasper, J. C., Korreck, K., Larson, D., Lichko, E., Livi, R., McManus, M., Martinović, M., Rahmati, A., Stevens, M., Whittlesey, P.
The hot and diffuse nature of the Sun's extended atmosphere allows it to persist in non-equilibrium states for long enough that wave-particle instabilities can arise and modify the evolution of the expanding solar wind. Determining which instabilitie
Externí odkaz:
http://arxiv.org/abs/2101.10937