Results 161 to 170 of about 838 (214)

A Novel Determination of the Foreshock ULF Boundary: Statistical Approach. [PDF]

open access: yesJ Geophys Res Space Phys
Salohub A   +3 more
europepmc   +1 more source

Ohm's Law, the Reconnection Rate, and Energy Conversion in Collisionless Magnetic Reconnection. [PDF]

open access: yesSpace Sci Rev
Liu YH   +14 more
europepmc   +1 more source

Observations of Turbulence near Interplanetary Travelling Shocks

AIP Conference Proceedings, 2005
The observations on magnetic field fluctuations and suprathermal ion spectra near the shocks driven by the coronal mass ejections during the time periods of the Bastille Day 2000 event and the Halloween 2003 events are summarized.
Kallenbach, R.   +3 more
openaire   +3 more sources

Plasma wave turbulence associated with an interplanetary shock

Journal of Geophysical Research: Space Physics, 1979
In this paper we give a brief summary of the interplanetary shocks detected and analyzed to date from the Helios 1 and 2 spacecraft and present a detailed analysis of the plasma wave turbulence associated with one particular shock, on March 30, 1976. This event was selected because a very clearly defined burst of plasma wave turbulence occurs at the ...
Gurnett, D., Neubauer, F., Schwenn, R.
openaire   +2 more sources

Interplanetary plasma irregularities and ion acoustic turbulence

Physics Reports, 1990
Abstract In this paper we discuss an effect of the ion acoustic turbulence on the inhomogeneous stucture of complementary ionized interplanetary and interstellar plasmas. These media are practically collisionless and their irregularities are of scales (along the magnetic field lines) much smaller than the mean free path of the electrons. However, the
L.G. Genkin, L.M. Erukhimov
openaire   +1 more source

Nonlocal plasma turbulence associated with interplanetary shocks

Journal of Geophysical Research: Space Physics, 1982
The plasma wave instrument on ISEE 3 has detected regions of plasma turbulence that extend several tenths of an astronomical unit upstream or downstream of inteplanetary shocks. The plasma waves fall into four categories. Highly impulsive 1‐ 10‐kHz electric field bursts were found hours upstream of quasi‐parallel interplanetary shocks.
C. F. Kennel   +4 more
openaire   +1 more source

Turbulence properties associated with interplanetary shock waves

AIP Conference Proceedings, 2012
We calculate the power spectral densities of magnetic field fluctuations associated with interplanetary shock waves, utilizing in-situ magnetic field measurements from spacecraft ACE and Wind at 1AU. We derive related quantities both upstream and downstream of a shock as a function of time/distance away from the shock passage.
Qiang Hu   +3 more
openaire   +1 more source

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