Search Publications

Quasistatic electric field structures and field-aligned currents in the polar cusp region
DOI: 10.1029/2010JA015467 Bibcode: 2010JGRA..11510226J

Jacobsen, K. S.; Moen, J. I.; Pedersen, A.

Cluster data have been examined for quasi-stationary electric field structures and field-aligned currents (FACs) in the vicinity of the dayside cusp region. We have related the measurements to the Region 1/Region 2 (R1/R2) current system and the cusp current system. It has been theoretically proposed that the dayside R1 current may be located on o…

2010 Journal of Geophysical Research (Space Physics)
Cluster 3
Using a global magnetohydrodynamic model to study the start of the substorm recovery phase
DOI: 10.1029/2010JA015802 Bibcode: 2010JGRA..11512237F

Baker, D. N.; Wiltberger, M.; Farr, N. L.

Magnetospheric substorms are a key manifestation of the transfer of energy from the solar wind to the Earth. Substorms consist of a loading of energy from the solar wind via magnetic reconnection and then a rapid release of that energy. One of the results of this energy release is the intense brightening of the aurora observed in the Earth's high-…

2010 Journal of Geophysical Research (Space Physics)
Cluster 3
Energetic electron response to ULF waves induced by interplanetary shocks in the outer radiation belt
DOI: 10.1029/2009JA014393 Bibcode: 2009JGRA..11410204Z

Zong, Q. -G.; Daly, P. W.; Baker, D. N. +7 more

Strong interplanetary shock interactions with the Earth's magnetosphere have great impacts on energetic particle dynamics in the magnetosphere. An interplanetary shock on 7 November 2004 (with the maximum solar wind dynamic pressure of ∼70 nPa) was observed by the Cluster constellation to induce significant ULF waves in the plasmasphere boundary, …

2009 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 274
Nonlinear mechanisms of lower-band and upper-band VLF chorus emissions in the magnetosphere
DOI: 10.1029/2009JA014206 Bibcode: 2009JGRA..114.7217O

Katoh, Yuto; Omura, Yoshiharu; Hikishima, Mitsuru +2 more

We develop a nonlinear wave growth theory of magnetospheric chorus emissions, taking into account the spatial inhomogeneity of the static magnetic field and the plasma density variation along the magnetic field line. We derive theoretical expressions for the nonlinear growth rate and the amplitude threshold for the generation of self-sustaining ch…

2009 Journal of Geophysical Research (Space Physics)
Cluster 230
Radial evolution of nonthermal electron populations in the low-latitude solar wind: Helios, Cluster, and Ulysses Observations
DOI: 10.1029/2008JA013883 Bibcode: 2009JGRA..114.5104S

Maksimovic, Milan; Štverák, Štěpán; Marsch, Eckart +3 more

We have performed a statistical study of a substantial amount of solar wind electron velocity distribution functions (eVDFs). In our data set, we combine measurements acquired onboard three spacecrafts (Helios, Cluster II, and Ulysses) in the low ecliptic latitudes covering the heliocentric distance from 0.3 up to 4 AU. In this study, we focus on …

2009 Journal of Geophysical Research (Space Physics)
Cluster Ulysses 222
Ion heating resulting from pickup in magnetic reconnection exhausts
DOI: 10.1029/2008JA013701 Bibcode: 2009JGRA..114.5111D

Lin, R. P.; Phan, T. D.; Lepri, S. T. +6 more

The heating of ions downstream of the x-line during magnetic reconnection is explored using full-particle simulations, test particle simulations, and analytic analysis. Large-scale particle simulations reveal that the ion temperature increases sharply across the boundary layer that separates the upstream plasma from the Alfvénic outflow. This boun…

2009 Journal of Geophysical Research (Space Physics)
Cluster 171
Response of Jupiter's and Saturn's auroral activity to the solar wind
DOI: 10.1029/2008JA013694 Bibcode: 2009JGRA..114.5210C

Crary, F.; Cecconi, B.; Lamy, L. +18 more

While the terrestrial aurorae are known to be driven primarily by the interaction of the Earth's magnetosphere with the solar wind, there is considerable evidence that auroral emissions on Jupiter and Saturn are driven primarily by internal processes, with the main energy source being the planets' rapid rotation. Prior observations have suggested …

2009 Journal of Geophysical Research (Space Physics)
Cassini eHST 171
CME interactions with coronal holes and their interplanetary consequences
DOI: 10.1029/2008JA013686 Bibcode: 2009JGRA..114.0A22G

Gopalswamy, N.; Yashiro, S.; Mäkelä, P. +2 more

A significant number of interplanetary shocks (~17%) during cycle 23 were not followed by drivers. The number of such ``driverless'' shocks steadily increased with the solar cycle with 15%, 33%, and 52% occurring in the rise, maximum, and declining phase of the solar cycle. The solar sources of 15% of the driverless shocks were very close the cent…

2009 Journal of Geophysical Research (Space Physics)
SOHO 169
Oblique propagation of whistler mode waves in the chorus source region
DOI: 10.1029/2009JA014586 Bibcode: 2009JGRA..114.0F03S

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

Whistler mode chorus has been shown to play a role in the process of local acceleration of electrons in the outer Van Allen radiation belt. Most of the quasi-linear and nonlinear theoretical studies assume that the waves propagate parallel to the terrestrial magnetic field. We show a case where this assumption is invalid. We use data from the Clus…

2009 Journal of Geophysical Research (Space Physics)
Cluster 130
Bulk properties of the slow and fast solar wind and interplanetary coronal mass ejections measured by Ulysses: Three polar orbits of observations
DOI: 10.1029/2008JA013631 Bibcode: 2009JGRA..114.1109E

McComas, D. J.; Forsyth, R. J.; Gosling, J. T. +2 more

We examined plasma and magnetic field observations from all three Ulysses polar orbits of the Sun to study the properties of the slow and fast solar wind and interplanetary coronal mass ejections (ICMEs). We derived equations to characterize the radial and latitudinal variations for these three types of heliospheric plasma and identify distinguish…

2009 Journal of Geophysical Research (Space Physics)
Ulysses 129