Search Publications

Properties of the magnetospheric backward wave oscillator inferred from CLUSTER measurements of VLF chorus elements
DOI: 10.1029/2012JA017713 Bibcode: 2012JGRA..117.8210T

Gurnett, D.; MacúšOvá, E.; SantolíK, O. +6 more

According to the backward wave oscillator (BWO) model, a sharp gradient (or step-like deformation) on the electron distribution function is the most important factor in chorus generation, but such a feature is very difficult to observe directly. The properties of the step in the BWO model determine the dimensionless parameterqquantifying the exces…

2012 Journal of Geophysical Research (Space Physics)
Cluster 8
Different Bz response regions in the nightside magnetosphere after the arrival of an interplanetary shock: Multipoint observations compared with MHD simulations
DOI: 10.1029/2011JA017303 Bibcode: 2012JGRA..117.5227S

Wang, C.; Wang, Y.; Sun, T. R.

We present different magnetic field changes in the nightside magnetosphere in response to the interplanetary (IP) shock on 17 December 2007, using multiple spacecraft observations and global MHD simulations. The coexistence of two distinct Bz response regions in the nightside magnetosphere in a single event has been observationally iden…

2012 Journal of Geophysical Research (Space Physics)
DoubleStar 8
Upstream-generated Pc3 ULF wave signatures observed near the Earth's cusp
DOI: 10.1029/2011JA017327 Bibcode: 2012JGRA..117.3202Y

Yeoman, T. K.; Wright, D. M.; Kim, H. +3 more

Pc3 pulsations (frequency ∼20-100 mHz) which originate in the ion foreshock upstream of the Earth's bow shock due to the interaction between reflected ions and the solar wind are frequently observed in ground-based pulsation magnetometer data. Previous studies have noted increased Pc3 wave power in the vicinity of the dayside cusp and inferred tha…

2012 Journal of Geophysical Research (Space Physics)
Cluster 8
Cassini UVIS observations of Titan nightglow spectra
DOI: 10.1029/2012JA017888 Bibcode: 2012JGRA..11712315A

West, Robert A.; Esposito, Larry W.; Gustin, Jacques +6 more

In this paper we present the first nightside EUV and FUV airglow limb spectra of Titan showing molecular emissions. The Cassini Ultraviolet Imaging Spectrograph (UVIS) observed photon emissions of Titan's day and night limb-airglow and disk-airglow on multiple occasions, including during an eclipse observation. The 71 airglow observations analyzed…

2012 Journal of Geophysical Research (Space Physics)
Cassini 8
A study of the changes of the near-Earth plasma sheet and lobe driven by multiple substorms: Comparison with a full particle simulation of reconnection
DOI: 10.1029/2011JA017033 Bibcode: 2012JGRA..117.1221S

Sauvaud, J. -A.; Balogh, A.; Kistler, L. M. +9 more

Comparisons of multispacecraft observations and full-particle simulations are used to understand magnetotail changes during substorms and the related cross-tail current disruptions/reductions. We first show that the electric field accompanying current disruptions can be measured in the tail lobe from the drift velocity of oxygen beams. A stormy pe…

2012 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 7
Deformation of plasma bubbles and the associated field aligned current system during substorm recovery phase
DOI: 10.1029/2011JA017410 Bibcode: 2012JGRA..117.9223P

Deng, X. H.; Huang, S. Y.; Zhou, M. +2 more

Multiple plasma bubbles have been detected by CLUSTER satellites on August 15th 2001 in midtail (∼-18 Re). Those bubbles can be classified into two types. Type-I bubbles are similar to those bubbles in previous studies [ Sergeev et al., 1996; Walsh et al., 2009]. Unlike type-I bubbles, the trailing parts/tails of type-II bubbles are much more dyna…

2012 Journal of Geophysical Research (Space Physics)
Cluster 6
Polarization and direction of arrival of Jovian quasiperiodic bursts observed by Cassini
DOI: 10.1029/2012JA017506 Bibcode: 2012JGRA..11711209K

Cecconi, B.; Kimura, T.; Misawa, H. +4 more

Jovian quasiperiodic (QP) radio bursts are suspected to be associated with relativistic particle accelerations occurring with a quasiperiodicity between a few minutes and a few tens of minutes in Jupiter's polar magnetosphere. Understanding the excitation and propagation of QP bursts could help us to better understand this periodic energization pr…

2012 Journal of Geophysical Research (Space Physics)
Cassini 6
Experimental evaluation of common spacecraft data analysis techniques for reconnection region analysis in a laboratory plasma
DOI: 10.1029/2012JA017742 Bibcode: 2012JGRA..11712202Y

Yoo, Jongsoo; Yamada, Masaaki

A laboratory plasma is utilized to assess the effectiveness of several prominent spacecraft data analysis techniques. These include minimum variance analysis on the magnetic field (MVAB) and various boundary-crossing time analyses (BCTA) such as the constant velocity approach (CVA), constant thickness approach (CTA), and minimum thickness variance…

2012 Journal of Geophysical Research (Space Physics)
Cluster 6
Cluster observations of band-limited Pc 1 waves associated with streaming H+ and O+ ions in the high-altitude plasma mantle
DOI: 10.1029/2012JA017982 Bibcode: 2012JGRA..11710219E

Glassmeier, K. -H.; Lavraud, B.; Rème, H. +12 more

Bursts of band-limited Pc 1 waves (0.2 to ∼1.0 Hz) with normalized frequency f/fH+ ∼ 0.5 have been observed by the Cluster spacecraft during many passes through the high-latitude plasma mantle. These transverse, left-hand polarized waves are associated with regions of H+ and O+ ions streaming away from Earth along …

2012 Journal of Geophysical Research (Space Physics)
Cluster 6
Entropy conservation and rate of propagation of bubbles in the Earth's magnetotail: A case study
DOI: 10.1029/2011JA017287 Bibcode: 2012JGRA..117.5226S

Wing, Simon; Sanchez, Ennio R.; Spanswick, Emma +1 more

Earthward propagation of low-density flux tubes, called “plasma bubbles,” is a candidate mechanism to reduce total entropy in the plasma sheet. MHD models predict that bubbles conserve total entropy (S) as they propagate earthward, that the amount of density depletion governs the speed of propagation, and that bubbles slow down as their S nears th…

2012 Journal of Geophysical Research (Space Physics)
Cluster 5