Search Publications

Tracking corotating interaction regions from the Sun through to the orbit of Mars using ACE, MEX, VEX, and STEREO
DOI: 10.1029/2010JA015719 Bibcode: 2011JGRA..116.8103W

Fränz, M.; Davies, J. A.; Lester, M. +3 more

We study the propagation of corotating interaction regions (CIRs) through the inner heliosphere during the solar minimum of 2007-2008 using the Advanced Composition Explorer (ACE), Mars Express (MEX), Venus Express (VEX), and the Solar Terrestrial Relations Observatory (STEREO). We present observations of 24 CIRs observed during the period from 1 …

2011 Journal of Geophysical Research (Space Physics)
MEx VenusExpress 14
Revisiting Time History of Events and Macroscale Interactions during Substorms (THEMIS) substorm events implying magnetic reconnection as the substorm trigger
DOI: 10.1029/2010JA016078 Bibcode: 2011JGRA..116.3211L

Lui, A. T. Y.

A recent trend in substorm research is the time history approach, motivated by the NASA mission Time History of Events and Macroscale Interactions during Substorms (THEMIS). We revisit three THEMIS substorm events recently reported to indicate magnetic reconnection as the substorm trigger. The evidence for the occurrence of magnetic reconnection i…

2011 Journal of Geophysical Research (Space Physics)
Cluster 14
On the simultaneity of substorm onset between two hemispheres
DOI: 10.1029/2010JA016174 Bibcode: 2011JGRA..116.4211M

Misawa, H.; Parks, G. K.; Décréau, P. M. E. +13 more

Simultaneous observations of auroral kilometric radiation from the Northern and Southern Hemispheres showed some cases in which the buildup of field-aligned acceleration occurred only in one hemisphere at the substorm onset. This indicates that a substorm does not always complete the current system by connecting the cross-tail current with both no…

2011 Journal of Geophysical Research (Space Physics)
Cluster 14
Electron energetics in the Enceladus torus
DOI: 10.1029/2011JA016498 Bibcode: 2011JGRA..116.9205C

Cravens, T. E.; Robertson, I. P.; Perry, M. +4 more

The inner magnetosphere of Saturn contains both neutral gas and plasma whose composition is dominated by water group ion species. This gas is distributed in a torus-shaped region located near the orbit of Enceladus. The source of this gas is the predominately water vapor plume located in the south polar region of Saturn's icy satellite Enceladus. …

2011 Journal of Geophysical Research (Space Physics)
Cassini 13
Evidence of surface wave on the dusk flank of Saturn's magnetopause possibly caused by the Kelvin-Helmholtz instability
DOI: 10.1029/2011JA016643 Bibcode: 2011JGRA..11610220C

Dougherty, M. K.; Lucek, E.; Masters, A. +1 more

Boundary waves on Saturn's dusk side magnetopause were identified from magnetopause crossings made by the Cassini spacecraft. These crossings occurred over a 48 h period from 14 July to 15 July 2007 when Cassini was on the inbound leg of revolution (Rev.) 48, and were located at around 17:00 SLT at low latitudes above the equatorial plane. The bou…

2011 Journal of Geophysical Research (Space Physics)
Cassini 13
In situ evidence for interplanetary magnetic field induced tail twisting associated with relative displacement of conjugate auroral features
DOI: 10.1029/2010JA016206 Bibcode: 2011JGRA..116.4209M

Rème, H.; Sato, N.; Ogawa, Y. +4 more

We provide in situ evidence for a twisted near-Earth tail configuration that is responsible for the time sequence of conjugate auroral features associated with relative interhemispheric displacement during a weak substorm, as reported by Motoba et al. (2010). We analyzed the magnetic field data observed using four Cluster satellites in the vicinit…

2011 Journal of Geophysical Research (Space Physics)
Cluster 13
What causes the flux excess in the heliospheric magnetic field?
DOI: 10.1029/2011JA016521 Bibcode: 2011JGRA..11612101S

Smith, Edward J.

Ulysses results indicate that the total magnetic flux inside the heliosphere, Φ, can be obtained from the radial field component measured at a single spacecraft multiplied by the square of the radial distance and averaged over a solar rotation, < r2BR >. However, that result is contrary to a large increase in Φ with dis…

2011 Journal of Geophysical Research (Space Physics)
Ulysses 13
Velocity distributions of superthermal electrons fitted with a power law function in the magnetosheath: Cluster observations
DOI: 10.1029/2010JA016118 Bibcode: 2011JGRA..116.3224L

Zhang, Tielong; Wang, Shui; Lu, Quanming +3 more

Satellite observations have revealed that superthermal electrons in space plasma generally possess a power law distribution. In this paper, we utilize a power law function to model the omnidirectional differential fluxes of superthermal electrons observed by Cluster in the magnetosheath. By assuming an isotropic pitch angle distribution and perfor…

2011 Journal of Geophysical Research (Space Physics)
Cluster 12
Unusual nonlinear waves in the Venusian magnetosheath
DOI: 10.1029/2010JA015916 Bibcode: 2011JGRA..116.1215W

Zhang, T. L.; Walker, S. N.; Balikhin, M. A. +4 more

Within the Venusian magnetosheath, Venus Express has observed the existence of high-amplitude, nonlinear waves which have been interpreted as large-scale nonlinear rotational structures within the magnetic field. A number of mechanisms have been proposed that can be used to explain their origin. Venus Express data have been searched for other exam…

2011 Journal of Geophysical Research (Space Physics)
VenusExpress 12
Modified solar flux index for upper atmospheric applications
DOI: 10.1029/2010JA016322 Bibcode: 2011JGRA..116.8303M

Maruyama, Takashi

The F10.7 solar flux index was modified in order to better describe short-term variations in solar extreme ultraviolet (EUV) irradiance for application in ionosphere and thermosphere studies. Several parameters were computed from the F10.7 time series with the assistance of an artificial neural network (ANN) technique, and th…

2011 Journal of Geophysical Research (Space Physics)
SOHO 11