Zobrazeno 1 - 10
of 204
pro vyhledávání: '"C E J Watt"'
Autor:
S. Chakraborty, I. R. Mann, C. E. J. Watt, I. J. Rae, L. Olifer, L. G. Ozeke, J. K. Sandhu, B. H. Mauk, H. Spence
Publikováno v:
Scientific Reports, Vol 12, Iss 1, Pp 1-13 (2022)
Abstract Chorus waves play a key role in outer Van Allen electron belt dynamics through cyclotron resonance. Here, we use Van Allen Probes data to reveal a new and distinct population of intense chorus waves excited in the heart of the radiation belt
Externí odkaz:
https://doaj.org/article/b687d66c36e84ffc87ffc47fe292b654
Autor:
Yi-Jiun Su, S. T. Jones
Publikováno v:
Journal of Geophysical Research: Space Physics. 114
[1] In our recent paper [Jones and Su, 2008] (hereinafter referred to as JS) we discuss the effect of dispersive Alfven waves (DAW) in relation to observed particle acceleration at the Io-Jupiter auroral footprint using a two-fluid model. Watt and Ra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ac7670369be887608b1bfdf9d298fa6c
https://doi.org/10.1029/2009ja014161
https://doi.org/10.1029/2009ja014161
Publikováno v:
Earth and Space Science, Vol 8, Iss 6, Pp n/a-n/a (2021)
Abstract Characterizing the location of the outer boundary of the outer radiation belt is a key aspect of improving radiation belt models and helps to constrain our understanding of the mechanisms by which the source and seed electron populations are
Externí odkaz:
https://doaj.org/article/f3c1d93f018f48e1b1d3a0f4517572b6
Publikováno v:
Earth and Space Science, Vol 7, Iss 10, Pp n/a-n/a (2020)
Abstract Models of magnetospheric ultralow‐frequency (ULF) waves can be used to study wave phenomena and to calculate the effect of these waves on the energization and transport of radiation belt electrons. We present a decision tree ensemble (i.e.
Externí odkaz:
https://doaj.org/article/6002fd2a8ea140e5b132b8c6686cecab
Autor:
N. M. E. Kalmoni, I. J. Rae, C. E. J. Watt, K. R. Murphy, M. Samara, R. G. Michell, G. Grubbs, C. Forsyth
Publikováno v:
Nature Communications, Vol 9, Iss 1, Pp 1-11 (2018)
The origin of geomagnetic substorms is still uncertain due to lack of comprehensive quantitative analyses. Here, the authors construct an observational dispersion relation of auroral forms that correspond to the explosive energy release from substorm
Externí odkaz:
https://doaj.org/article/6552a7c988864dc6ab861b35e482c163
Akademický článek
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Autor:
S Killey, I J Rae, S Chakraborty, A W Smith, S N Bentley, M R Bakrania, R Wainwright, C E J Watt, J K Sandhu
Publikováno v:
XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
The behaviour of relativistic electrons in the radiation belt is difficult to diagnose as their dynamics are controlled by simultaneous physics processes, some of which may be still unknown. Signatures of these physical processes are difficult to ide
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d6629c3261f0916b8cf56234c06040ff
Autor:
C. T. S. Lorch, L. C. Ray, R. J. Wilson, F. Bagenal, F. Crary, P. A. Delamere, P. A. Damiano, C. E. J. Watt, F. Allegrini
Using a combination of Juno magnetometer and plasma data, we show evidence of Alfvénic turbulence within the mid‐to‐high latitude magnetosphere with sufficient conditions to trigger auroral particle acceleration. We analyze 12 events that, in ag
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e343ea147052de79bf621e9daba8528
Publikováno v:
Annales Geophysicae, Vol 25, Pp 2529-2539 (2007)
We present an interval whereby we can estimate the energy dissipation in the ionosphere through an externally-driven field line resonance. In this paper, we utilise an interval described in general by Rae et al. (2005), where the global magnetosph
Externí odkaz:
https://doaj.org/article/abb8537cf51b49c6aca9c2ef75a003d2
Autor:
McLeish, Alison C.1,2 alison.mcleish@louisville.edu, Hartson, Kimberly R.3, Walker, Kandi L.1,4, Hart, Joy L1,4
Publikováno v:
Psychology, Health & Medicine. 2023, Vol. 28 Issue 9, p2512-2525. 14p. 1 Chart.