Search Publications

Cavities of weak magnetic field strength in the wake of FTEs: Results from global magnetospheric MHD simulations
DOI: 10.1029/2009GL037489 Bibcode: 2009GeoRL..3610104K

Toth, G.; Hesse, M.; Wang, Y. +4 more

We use the global magnetohydrodynamic (MHD) code BATS-R-US to model multipoint observations of Flux Transfer Event (FTE) signatures. Simulations with high spatial and temporal resolution predict that cavities of weak magnetic field strength protruding into the magnetosphere trail FTEs. These predictions are consistent with recently reported multi-…

2009 Geophysical Research Letters
Cluster 11
“Hook” structure in MARSIS ionogram and its interpretation
DOI: 10.1029/2009GL038844 Bibcode: 2009GeoRL..3613103W

Wang, X. -D.; Zou, H.; Wang, J. -S. +1 more

MARSIS/MEX is a low frequency radar used to sound the ionosphere of Mars. In general the echo trace associated with reflections in nadir indicates an ionosphere with a main maximum electron density at typically about 130 km altitude, and a monotonously decreasing density with increasing altitude. Another maximum is sometimes detected at higher alt…

2009 Geophysical Research Letters
MEx 10
Modeling the response of the induced magnetosphere of Venus to changing IMF direction using MESSENGER and Venus Express observations
DOI: 10.1029/2008GL036718 Bibcode: 2009GeoRL..36.4109B

Boardsen, Scott A.; Gloeckler, George; Ho, George C. +14 more

The second MESSENGER flyby of Venus on 5 June 2007 provided a new opportunity to study the response of the induced magnetosphere of the planet to changes in the direction of the interplanetary magnetic field (IMF). At the time of the MESSENGER flyby, the European Space Agency's Venus Express spacecraft was located outside the magnetosphere and pro…

2009 Geophysical Research Letters
VenusExpress 8
Solar wind periodicity in energetic electrons at Saturn
DOI: 10.1029/2009GL041086 Bibcode: 2009GeoRL..3622104C

Krupp, N.; Krimigis, S. M.; Mitchell, D. G. +2 more

Fluxes of energetic electrons (110-365 keV) have been subjected to a long-term Lomb periodogram analysis from the middle of 2004 to the middle of 2009. Fluxes within 20 RS and outside the magnetopause were excluded, so only fluxes within the magnetosphere were included in the analysis. The periodicity “box” was expanded from 5 hours to …

2009 Geophysical Research Letters
Cassini 7
Magnetopause reconnection impact parameters from multiple spacecraft magnetic field measurements
DOI: 10.1029/2009GL040228 Bibcode: 2009GeoRL..3620108W

Wendel, Deirdre E.; Reiff, Patricia H.

We present a novel technique that exploits multiple spacecraft data to determine the impact parameters of the most general form of magnetic reconnection at the magnetopause. The method consists of a superposed epoch of multiple spacecraft magnetometer measurements that yields the instantaneous magnetic spatial gradients near a magnetopause reconne…

2009 Geophysical Research Letters
Cluster 5
Reconnection Hall current system observed in the magnetotail and in the ionosphere
DOI: 10.1029/2009GL037239 Bibcode: 2009GeoRL..36.8104S

Snekvik, K.; Østgaard, N.; Amm, O. +1 more

On 07 Sep 2001 around 21:40 UT, Cluster was located 19 R E downtail, and observed earthward fast flows and strong perturbations in the dawn-dusk component of the magnetic field (B Y ). The perturbations corresponded to a sheet of tailward field aligned current close to the neutral sheet and another sheet of earthward field…

2009 Geophysical Research Letters
Cluster 2
Tsallis distribution of the interplanetary magnetic field at 0.72 AU: Venus Express observation
DOI: 10.1029/2009GL038395 Bibcode: 2009GeoRL..3611103L

Zhang, T. L.; Wang, C.; Li, X. Y.

Previous work shows that Probability Distribution Functions (PDFs) of the interplanetary magnetic field strength differences can be described by a single function - Tsallis distribution at Earth and beyond. Launch of Venus Express enables us to extend the application of Tsallis distribution to the inner heliosphere at 0.72 AU. This paper analyzes …

2009 Geophysical Research Letters
VenusExpress 0