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A case study of EMIC wave-associated He+ energization in the outer magnetosphere: Cluster and Double Star 1 observations
DOI: 10.1029/2009JA014784 Bibcode: 2010JGRA..115.6212Z

Sauvaud, J. -A.; Klecker, B.; Kistler, L. M. +3 more

On December 4, 2004, the COmposition and DIstribution Function (CODIF) Analyzer on board the Cluster spacecraft observed a prolonged He+ energization event from 06:00 to 10:30 UT. In this paper, we perform a case study of the event by using in situ plasma and magnetic field measurements from the Cluster and Double Star Program (DSP) Tan…

2010 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 52
Latitudinal variations in Saturn's ionosphere: Cassini measurements and model comparisons
DOI: 10.1029/2010JA015692 Bibcode: 2010JGRA..11511317M

Galand, Marina; Moore, Luke; Mendillo, Michael +2 more

We present a study of latitudinal variations in Saturn's ionosphere using Cassini Radio Science Subsystem (RSS) measurements and Saturn-Thermosphere-Ionosphere-Model (STIM) simulations. On the basis of Cassini RSS observations, the peak electron density (NMAX) and the total electron content (TEC) both exhibit a clear increase with latit…

2010 Journal of Geophysical Research (Space Physics)
Cassini 52
Evolution of the spectrum of solar wind velocity fluctuations from 0.3 to 5 AU
DOI: 10.1029/2009JA015120 Bibcode: 2010JGRA..11512101R

Roberts, D. Aaron

Recent work has shown that at 1 AU from the Sun, the power spectrum of the solar wind magnetic field has the -5/3 spectral slope expected for Kolmogorov turbulence but that the velocity has closer to a -3/2 spectrum. This paper traces the changes in solar wind velocity spectra from 0.3 to 5 AU using data from the Helios and Ulysses spacecraft to s…

2010 Journal of Geophysical Research (Space Physics)
Ulysses 52
Numerical simulation of the 12 May 1997 CME Event: The role of magnetic reconnection
DOI: 10.1029/2010JA015464 Bibcode: 2010JGRA..11510104C

Owens, M. J.; Crooker, N. U.; Gombosi, T. I. +4 more

We perform a numerical study of the evolution of a Coronal Mass Ejection (CME) and its interaction with the coronal magnetic field based on the 12 May 1997, CME event using a global MagnetoHydroDynamic (MHD) model for the solar corona. The ambient solar wind steady-state solution is driven by photospheric magnetic field data, while the solar erupt…

2010 Journal of Geophysical Research (Space Physics)
SOHO 51
Wave-particle interactions in the equatorial source region of whistler-mode emissions
DOI: 10.1029/2009JA015218 Bibcode: 2010JGRA..115.0F16S

Gurnett, D. A.; Pickett, J. S.; Santolík, O. +8 more

Wave-particle interactions can play a key role in the process of transfer of energy between different electron populations in the outer Van Allen radiation belt. We present a case study of wave-particle interactions in the equatorial source region of whistler-mode emissions. We select measurements of the Cluster spacecraft when these emissions are…

2010 Journal of Geophysical Research (Space Physics)
Cluster 50
Limitations of multispacecraft data techniques in measuring wave number spectra of space plasma turbulence
DOI: 10.1029/2009JA014724 Bibcode: 2010JGRA..115.4206S

Belmont, G.; Sahraoui, F.; Rezeau, L. +1 more

Unambiguous determination of spatial properties of space plasma turbulence from temporal measurements has been one of the major goals of the Cluster mission. For that purpose, techniques, such as the k filtering, have been developed. Such multipoint measurement techniques combine several time series recorded simultaneously at different points in s…

2010 Journal of Geophysical Research (Space Physics)
Cluster 50
Pitch angle transport of electrons due to cyclotron interactions with the coherent chorus subelements
DOI: 10.1029/2009JA014885 Bibcode: 2010JGRA..115.0F15L

Lakhina, G. S.; Tsurutani, B. T.; Verkhoglyadova, O. P. +1 more

Chorus is a right-hand, circularly-polarized electromagnetic plane wave. Dayside chorus is a bursty emission composed of rising frequency “elements” with duration of ∼0.1 to 1.0 s. Each element is composed of coherent subelements with durations of ∼1 to 100 ms or more. Due to the coherent nature of the chorus subelements/wave packets, energetic el…

2010 Journal of Geophysical Research (Space Physics)
Cluster 49
Observations of the relationship between frequency sweep rates of chorus wave packets and plasma density
DOI: 10.1029/2010JA015468 Bibcode: 2010JGRA..11512257M

Gurnett, D. A.; Pickett, J. S.; Demekhov, A. G. +8 more

Chorus emissions are generated by a nonlinear mechanism involving wave-particle interactions with energetic electrons. Discrete chorus wave packets are narrowband tones usually rising (sometimes falling) in frequency. We investigate frequency sweep rates of chorus wave packets measured by the Wideband data (WBD) instrument onboard the Cluster spac…

2010 Journal of Geophysical Research (Space Physics)
Cluster 49
Magnetopause oscillations near the planetary period at Saturn: Occurrence, phase, and amplitude
DOI: 10.1029/2009JA014745 Bibcode: 2010JGRA..115.8209C

Coates, A. J.; Andrews, D. J.; Cowley, S. W. H. +2 more

Using magnetic field and plasma electron data from ∼40 Cassini orbits that crossed Saturn's magnetopause during 2004-2007, we make a first systematic study of the magnetopause oscillations that are related to the oscillations in the magnetic field and plasma inside the magnetosphere near the ∼11 h planetary rotation period, here termed the magneto…

2010 Journal of Geophysical Research (Space Physics)
Cassini 48
THEMIS observations of substorms on 26 February 2008 initiated by magnetotail reconnection
DOI: 10.1029/2009JA014217 Bibcode: 2010JGRA..115.2212P

Russell, C. T.; Wei, Y.; Glassmeier, K. -H. +25 more

On 26 February 2008, the THEMIS satellites observed two substorms that occurred at about 0405 and 0455 UT. Angelopoulos et al. (2008) made a comprehensive study of the second event. In this paper we display detailed features of the two substorms with emphasis on the first. In both substorms, a distinct auroral intensification occurred during the e…

2010 Journal of Geophysical Research (Space Physics)
Cluster 46