Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements

Details Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005phrvl..95w1101m&link_type=abstract

Physical Review Letters, vol. 95, Issue 23, id. 231101

Astronomy and Astrophysics

Astrophysics

66

Solar Wind Plasma, Sources Of Solar Wind, Magnetohydrodynamics, Plasma Turbulence, Magnetohydrodynamics And Plasmas

Scientific paper

Interplanetary turbulence, the best studied case of low frequency plasma turbulence, is the only directly quantified instance of astrophysical turbulence. Here, magnetic field correlation analysis, using for the first time only proper two-point, single time measurements, provides a key step in unraveling the space-time structure of interplanetary turbulence. Simultaneous magnetic field data from the Wind, ACE, and Cluster spacecraft are analyzed to determine the correlation (outer) scale, and the Taylor microscale near Earth’s orbit.

Affiliated with

Also associated with

No associations

Rating

Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spatial Correlation of Solar-Wind Turbulence from Two-Point Measurements will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1467985