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pro vyhledávání: '"McManus, M"'
Autor:
Bale, S. D., Drake, J. F., McManus, M. D., Desai, M. I., Badman, S. T., Larson, D. E., Swisdak, M., Horbury, T. S., Raouafi, N. E., Phan, T., Velli, M., McComas, D. J., Cohen, C. M. S., Mitchell, D., Panasenco, O., Kasper, J. C.
The fast solar wind that fills the heliosphere originates from deep within regions of open magnetic field on the Sun called coronal holes. The energy source responsible for accelerating the plasma to high speeds is widely debated, however there is ev
Externí odkaz:
http://arxiv.org/abs/2208.07932
Autor:
McManus, M. D., Verniero, J. L., Bale, S. D., Bowen, T. A., Larson, D. E., Kasper, J. C., Livi, R., Matteini, L., Rahmati, A., Romeo, O., Whittlesey, P. L., Woolley, T.
Magnetic switchbacks, or sudden reversals in the magnetic field's radial direction, are one of the more striking observations of Parker Solar Probe (PSP) thus far in its mission. While their precise production mechanisms are still unknown, the two ma
Externí odkaz:
http://arxiv.org/abs/2204.13801
Autor:
Mostafavi, P., Allen, R. C., McManus, M. D., Ho, G. C., Raouafi, N. E., Larson, D. E., Kasper, J. C., Bale, S. D.
The velocity of alpha particles relative to protons can vary depending on the solar wind type and distance from the Sun (Marsch 2012). Measurements from the previous spacecraft provided the alpha-proton's differential velocities down to 0.3 au. Parke
Externí odkaz:
http://arxiv.org/abs/2202.03551
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:
Bale, S. D., Horbury, T. S., Velli, M., Desai, M. I., Halekas, J. S., McManus, M. D., Panasenco, O., Badman, S. T., Bowen, T. A., Chandran, B. D. G., Drake, J. F., Kasper, J. C., Laker, R., Mallet, A., Matteini, L, Phan, T. D., Raouafi, N. E., Squire, J., Woodham, L. D., Wooley, T.
One of the striking observations from the Parker Solar Probe (PSP) spacecraft is the prevalence in the inner heliosphere of large amplitude, Alfv\'enic magnetic field reversals termed 'switchbacks'. These $\delta B_R/B \sim \mathcal{O}(1$) fluctuatio
Externí odkaz:
http://arxiv.org/abs/2109.01069
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
Autor:
Woodham, L. D., Horbury, T. S., Matteini, L., Woolley, T., Laker, R., Bale, S. D., Nicolaou, G., Stawarz, J. E., Stansby, D., Hietala, H., Larson, D. E., Livi, R., Verniero, J. L., McManus, M., Kasper, J. C., Korreck, K. E., Raouafi, N., Moncuquet, M., Pulupa, M. P.
Publikováno v:
A&A 650, L1 (2021)
Switchbacks are discrete angular deflections in the solar wind magnetic field that have been observed throughout the heliosphere. Recent observations by Parker Solar Probe (PSP) have revealed the presence of patches of switchbacks on the scale of hou
Externí odkaz:
http://arxiv.org/abs/2010.10379
Autor:
Verniero, J. L., Larson, D. E., Livi, R., Rahmati, A., McManus, M. D., Pyakurel, P. Sharma, Klein, K. G., Bowen, T. A., Bonnell, J. W., Alterman, B. L., Whittlesey, P. L., Malaspina, David M., Bale, S. D., Kasper, J. C., Case, A. W., Goetz, K., Harvey, P. R., Korreck, K. E., MacDowall, R. J., Pulupa, M., Stevens, M. L., de Wit, T. Dudok
Parker Solar Probe (PSP), NASA's latest and closest mission to the Sun, is on a journey to investigate fundamental enigmas of the inner heliosphere. This paper reports initial observations made by the Solar Probe Analyzer for Ions (SPAN-I), one of th
Externí odkaz:
http://arxiv.org/abs/2004.03009
Autor:
Chen, C. H. K., Bale, S. D., Bonnell, J. W., Borovikov, D., Bowen, T. A., Burgess, D., Case, A. W., Chandran, B. D. G., de Wit, T. Dudok, Goetz, K., Harvey, P. R., Kasper, J. C., Klein, K. G., Korreck, K. E., Larson, D., Livi, R., MacDowall, R. J., Malaspina, D. M., Mallet, A., McManus, M. D., Moncuquet, M., Pulupa, M., Stevens, M., Whittlesey, P.
The first two orbits of the Parker Solar Probe (PSP) spacecraft have enabled the first in situ measurements of the solar wind down to a heliocentric distance of 0.17 au (or 36 Rs). Here, we present an analysis of this data to study solar wind turbule
Externí odkaz:
http://arxiv.org/abs/1912.02348
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