N. Ness

Publications527
h-index79
Citations24,107
Highly Influential Citations1,019
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Observational constraints on the dynamics of the interplanetary magnetic field dissipation range
The dissipation range for interplanetary magnetic field fluctuations is formed by those fluctuations with spatial scales comparable to the gyroradius or ion inertial length of a thermal ion. It is… Expand
New models of Jupiter's magnetic field constrained by the Io flux tube footprint
Spherical harmonic models of the planetary magnetic field of Jupiter are obtained from in situ magnetic field measurements and remote observations of the position of the foot of the Io flux tube in… Expand
The WIND magnetic field investigation
The magnetic field experiment on WIND will provide data for studies of a broad range of scales of structures and fluctuation characteristics of the interplanetary magnetic field throughout the… Expand
A model of interplanetary and coronal magnetic fields
A model of the large-scale magnetic field structure above the photosphere uses a Green's function solution to Maxwell's equations. Sources for the magnetic field are related to the observed… Expand
The ACE Magnetic Fields Experiment
The magnetic eld experiment on ACE provides continuous measurements of the local magnetic eld in the interplanetary medium. These measurements are essential in the interpretation of simultaneous ACE… Expand
Radial evolution of power spectra of interplanetary Alfvénic turbulence
The radial evolution of the power spectra of the MHD turbulence within the trailing edge of high-speed streams in the solar wind has been investigated with the magnetic field data of HELIOS 1 and 2… Expand
Modeling the Jovian current sheet and inner magnetosphere
Voyager 1 and 2 magnetic field observations confirm and extend the earlier Pioneer 10 detection of the Jovian magnetodisc, a region of enhanced charged particles and plasma and reduced magnetic field… Expand
Dissipation range dynamics: Kinetic Alfvn waves and the importance of
In a previous paper we argued that the damping of obliquely propagating kinetic Alfven waves, chiefly by resonant mechanisms, was a likely explanation for the formation of the dissipation range for… Expand
Currents in Saturn's magnetosphere
A model of Saturn's magnetospheric magnetic field is obtained from the Voyager 1 and 2 observations. A representation consisting of the Z3 zonal harmonic model of Saturn's planetary magnetic field… Expand
Probing Mars' crustal magnetic field and ionosphere with the MGS Electron Reflectometer
The Electron Reflectometer (ER) on board Mars Global Surveyor measures the energy and angular distributions of solar wind electrons and ionospheric photoelectrons. These data can be used in… Expand
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