Search Publications

The termination shock near 35° latitude
DOI: 10.1029/2003GL018679 Bibcode: 2004GeoRL..31.3805W

Burlaga, L. F.; Sheeley, N. R.; Wang, Y. -M. +1 more

The termination shock moves outwards and inwards over timescales of a solar cycle in response to the variations in the average solar wind speed. The amplitude is greater than 50 AU near 35° latitude; the maximum (minimum) distance occurs during the rising (declining) phase of the solar cycle. Shock parameters are distinctly different when the shoc…

2004 Geophysical Research Letters
Ulysses 27
Oblique propagation of 30 s period fast magnetosonic foreshock waves: A Cluster case study
DOI: 10.1029/2003GL018897 Bibcode: 2004GeoRL..31.4804E

Balogh, A.; Dandouras, I.; Eastwood, J. P. +2 more

It is accepted that the 30 s period Ultra-Low-Frequency waves observed in the terrestrial foreshock are generated by backstreaming ions through the ion-ion right hand instability. However, such waves are generally observed to propagate obliquely to the field, in direct contrast to theoretical predictions of parallel propagation. A case study, base…

2004 Geophysical Research Letters
Cluster 27
Transient ion beamlet injections into spatially separated PSBL flux tubes observed by Cluster-CIS
DOI: 10.1029/2004GL020192 Bibcode: 2004GeoRL..3112804K

Lundin, R.; Dandouras, I.; Klecker, B. +8 more

Ion measurements from Cluster-CIS were used to characterize and interpret the signatures of PSBL energy-dispersed ions and their fine structure. On 14 February 2001, several ion injections were encountered by SC 1 and SC 3, separated by ~530 km, during an outbound orbit at 4.5 RE. Both satellites recorded the same ion structures. The en…

2004 Geophysical Research Letters
Cluster 26
Cluster observations of complex 3D magnetic structures at the magnetopause
DOI: 10.1029/2004GL020625 Bibcode: 2004GeoRL..3119805L

Fedorov, A.; Budnik, E.; Balogh, A. +7 more

On June 30, 2001, around 0530 UT, Cluster was moving along the magnetopause with spacecraft on both sides of the discontinuity. The configuration was `quasi-ideal' with magnetic field and plasma flow almost aligned in the magnetosheath and nearly anti-parallel to the magnetospheric field. Cluster observed several perturbations with leading and tra…

2004 Geophysical Research Letters
Cluster 25
Chemical composition of Titan's haze: Are PAHs present?
DOI: 10.1029/2004GL019859 Bibcode: 2004GeoRL..3117S08T

McKay, Christopher P.; Toon, Owen B.; Trainer, Melissa G. +4 more

Previous laboratory studies of haze aerosols analogous to those in Titan's atmosphere have shown evidence of the formation of polycyclic aromatic hydrocarbons (PAHs). If present, PAHs may provide a mechanism for both particle formation and nitrogen incorporation. We have conducted new experiments simulating Titan haze production using an Aerosol M…

2004 Geophysical Research Letters
Huygens 25
Two examples of magnetic clouds with double rotations observed by the Ulysses spacecraft
DOI: 10.1029/2003GL018330 Bibcode: 2004GeoRL..31.6804R

Forsyth, R. J.; Rees, A.

A survey of Ulysses magnetometer data has been carried out between Oct 1990 (launch) and Apr 2003 (just after the second northern polar pass) cataloguing magnetic cloud (MC) signatures, i.e., a smooth magnetic field rotation and enhanced magnetic field magnitude. After confirming that each of these events was a true MC by checking for a low proton…

2004 Geophysical Research Letters
Ulysses 22
Discrete modes and turbulence in a wave-driven strongly magnetized plasma
DOI: 10.1029/2004GL021119 Bibcode: 2004GeoRL..3121805D

Matthaeus, William H.; Lanzerotti, Louis J.; Dmitruk, Pablo

We show the coexistence of discrete modes and turbulence in numerical experiments of magnetohydrodynamics with a strong background magnetic field. The particular system we consider is a model of an open magnetic region which we have previously used in coronal heating studies. In the simulations shown here, Alfven waves at discrete frequencies with…

2004 Geophysical Research Letters
Ulysses 19
Cluster observations of velocity space-restricted ion distributions near the plasma sheet
DOI: 10.1029/2004GL020265 Bibcode: 2004GeoRL..3124802W

Lundin, R.; Sauvaud, J. -A.; Dandouras, I. +15 more

We present Cluster ion observations obtained at 18 RE in the magnetotail on 1 October 2001. According to a recent analysis, the quartet encountered a reconnection region and a tailward-moving neutral line. We examine in detail selected 3-D ion distributions, which through much of the hour following 0925 UT were non-gyrotropic. B-perpend…

2004 Geophysical Research Letters
Cluster 18
CLUSTER observations of lower hybrid waves excited at high altitudes by electromagnetic whistler mode signals from the HAARP facility
DOI: 10.1029/2003GL018855 Bibcode: 2004GeoRL..31.6811B

Pickett, J. S.; Inan, U. S.; Platino, M. +3 more

We report new observations from the CLUSTER spacecraft of strong excitation of lower hybrid (LH) waves by electromagnetic (EM) whistler mode waves at altitudes >=20,000 km outside the plasmasphere. Previous observations of this phenomenon occurred at altitudes <=7000 km. The excitation mechanism appears to be linear mode coupling in the pres…

2004 Geophysical Research Letters
Cluster 17
The dependence of Langmuir wave amplitudes on position in Earth's foreshock
DOI: 10.1029/2004GL019413 Bibcode: 2004GeoRL..31.7805S

Gurnett, D. A.; Balogh, A.; Pickett, J. S. +3 more

We present the first results of Langmuir wave observations in the foreshock from the Cluster WBD Plasma Wave Receiver. When the data were binned by distance to the foreshock boundary, the Langmuir wave amplitude probability distributions followed the log-normal statistics predicted by stochastic growth theory for all regions of the foreshock. The …

2004 Geophysical Research Letters
Cluster 15