Red-violet asymmetry in Pearl satellites' birth

Details Red-violet asymmetry in Pearl satellites' birth Red-violet asymmetry in Pearl satellites' birth

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985p%26ss...33..271f&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 33, March 1985, p. 271-273.

Physics

4

Geomagnetic Pulsations, Plasma Spectra, Red Shift, Sonograms, Spectrum Analysis, Amplitude Distribution Analysis, Frequency Shift, Resonance Lines, Space Plasmas

Scientific paper

The present frequency-time analysis of the Pc-1 geomagnetic pulsations obtained by a high resolution numerical sonogram has confirmed that the dynamics of their spectra are characterized by a step-by-step energy transfer between the lines of a quasi-discreted set. During this process, the preferential birth of the spectrum lines that were shifted toward lower frequencies with respect to the parent lines occurs. The fate of the parent line after the birth depends on its amplitude; while high amplitude lines disappear at once, moderate amplitude lines can linger for many bounce times.

Affiliated with

Also associated with

No associations

Rating

Red-violet asymmetry in Pearl satellites' birth 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 Red-violet asymmetry in Pearl satellites' birth, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Red-violet asymmetry in Pearl satellites' birth will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-826074