Search Publications

Hydrogen atom lifetimes in the three-dimensional heliosphere over the solar cycle
DOI: 10.1029/2003JA009878 Bibcode: 2003JGRA..108.8034P

Pryor, Wayne R.; Ajello, Joseph M.; Tobiska, W. Kent +2 more

The three-dimensional (3-D) structure of the heliosphere is investigated using in situ and remote sensing measurements. The 3-D structure of both neutral interplanetary gas and solar wind ions are affected by the solar latitude variation of the solar radiation fields (solar wind and solar EUV). Neutral hydrogen atom lifetimes against charge-exchan…

2003 Journal of Geophysical Research (Space Physics)
Ulysses 13
Hubble Space Telescope observations of sulfur ions in the Io plasma torus: New constraints on the plasma distribution
DOI: 10.1029/2002JA009510 Bibcode: 2003JGRA..108.1167H

Schneider, Nicholas M.; Hendrix, Amanda R.; Herbert, Floyd +1 more

During the Io plasma torus crossings by the Galileo spacecraft in late 1999 and early 2000 we observed the dawn ansa of the torus using the Hubble Space Telescope (HST). Here we analyze 74 FUV HST/Space Telescope Imaging Spectrograph observations (1150 ≤ λ ≤ 1720 Å) of the dawn ansa of the Io plasma torus made during Galileo's C23, I24, and I27 to…

2003 Journal of Geophysical Research (Space Physics)
eHST 12
Tail lobe convection observed by Cluster/EDI
DOI: 10.1029/2002JA009669 Bibcode: 2003JGRA..108.1288N

Nakamura, R.; Baumjohann, W.; Noda, H. +7 more

By using drift velocity data measured in the near-Earth tail lobe by the Electron Drift Instrument aboard the Cluster spacecraft, we study the average tail lobe convection of the Earth's magnetosphere. The data confirm the convection pattern toward the neutral sheet in the meridional (XZ) plane. By dividing the data according to the IMF clock angl…

2003 Journal of Geophysical Research (Space Physics)
Cluster 12
Near-source and remote observations of kilometric continuum radiation from multispacecraft observations
DOI: 10.1029/2003JA009826 Bibcode: 2003JGRA..108.1393M

Gurnett, D. A.; Pickett, J. S.; Menietti, J. D. +2 more

Kilometric continuum (KC) radiation was first identified from Geotail plasma wave observations. Past authors have shown that this emission has a frequency range that overlaps that of the auroral kilometric radiation (AKR) but is characterized by a fine structure of narrow-bandwidth, linear features that have nearly constant or drifting frequency. …

2003 Journal of Geophysical Research (Space Physics)
Cluster 11
Toward a self-consistent treatment of the cyclotron wave heating and acceleration of the solar wind plasma
DOI: 10.1029/2002JA009479 Bibcode: 2003JGRA..108.1081L

Laitinen, T.; Fichtner, H.; Vainio, R.

We have developed a steady state two-fluid description of the radial solar wind expansion close to the coronal base. The model is formulated self-consistently with respect to the radial evolution of turbulence by supplementing the moment equations of the plasma with an equation describing the radial evolution of the Alfvén wave power as originally…

2003 Journal of Geophysical Research (Space Physics)
SOHO 11
Solar cycle dependence of interplanetary Lyman α emission and solar wind anisotropies derived from NOZOMI/UVS and SOHO/SWAN observations
DOI: 10.1029/2003JA009882 Bibcode: 2003JGRA..108.8035N

Bertaux, Jean-Loup; Lallement, Rosine; Taguchi, Makoto +5 more

We have investigated the distributions of neutral interplanetary hydrogen Lyman α emission and their solar cycle dependence from observations with the ultraviolet imaging spectrometer (UVS) onboard the NOZOMI spacecraft and the solar wind anisotropy instrument (SWAN) onboard the solar and heliospheric observatory (SOHO) spacecraft. The SOHO/SWAN o…

2003 Journal of Geophysical Research (Space Physics)
SOHO 10
A possible way of understanding the differential motion of minor ions in the solar wind
DOI: 10.1029/2002JA009561 Bibcode: 2003JGRA..108.1161T

Tu, C. -Y.; Marsch, E.; Wang, L. -H.

Measurements with Solar and Heliospheric Observatory (SOHO)/Charge, Element, and Isotope Analysis System (CELIAS) in high-speed solar wind show that some minor ions such as O6+ have a relatively high drift velocity; however, other ions such as Fe9+ tend to lag behind oxygen by a few tens of km/s [, 1998]. This subtle observat…

2003 Journal of Geophysical Research (Space Physics)
SOHO 7
Ion isotropy and ion resonant waves in the solar wind: Corrected Cassini observations
DOI: 10.1029/2002JA009312 Bibcode: 2003JGRA..108.1045K

Gurnett, D. A.; Dougherty, M. K.; Hospodarsky, G. B. +3 more

In an earlier paper [, 2001], observations of electric field fluctuations in the range 0.5 to 25 Hz were reported. We have recently found that the data presented in that paper are seriously contaminated by broadband interference which appears to be generated in the spacecraft wake. Wake instabilities have been found by others, but the plasma condi…

2003 Journal of Geophysical Research (Space Physics)
Cassini 6
Fine structure of the diamagnetic cavity boundary in comet Halley
DOI: 10.1029/2002JA009622 Bibcode: 2003JGRA..108.1097I

Neubauer, F. M.; Gombosi, T. I.; Israelevich, P. L. +2 more

We calculated the electric current density in the diamagnetic cavity boundary layer (DCBL) using magnetic field data obtained during the Giotto mission to comet Halley. This current possesses both the component perpendicular to the local magnetic field and the parallel component. The perpendicular current is responsible for the screening of the di…

2003 Journal of Geophysical Research (Space Physics)
Giotto 2
Role of low-frequency modes in organizing the inner heliosphere
DOI: 10.1029/2001JA000058 Bibcode: 2003JGRA..108.1107H

Kunow, H.; Heber, B.; Lanzerotti, Louis J. +2 more

Cosmic ray proton data (125 to >2000 MeV) measured in the inner three-dimensional (3-D) heliosphere over the years from 1993 into 2000 by the KET instrument on the Ulysses spacecraft are examined. The data are parameterized and characterized by fitting products of spherical harmonic and sinusoidal frequency functions to three individual proton …

2003 Journal of Geophysical Research (Space Physics)
Ulysses 0