'Serpentine Emission' at the high latitude Antarctic station, Davis

Details 'Serpentine Emission' at the high latitude Antarctic station, Davis 'Serpentine Emission' at the high latitude Antarctic station, Davis

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987p%26ss...35..313m&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 35, March 1987, p. 313-328. Research supported by the Department of Science a

Mathematics

Logic

5

Antarctic Regions, Auroral Arcs, Extremely Low Radio Frequencies, Oscillations, Radio Emission, Amplitudes, Frequency Modulation, Polarization Characteristics, Power Spectra, Time Response

Scientific paper

New observational and dynamical morphological results on the Serpentine Emission (SE) phenomenon observed at Davis, Antarctica during 1981 are discussed. Included are analyses of the amplitude-time structure, the maximum entropy power spectra, digital sonograms, and SE polarizations. Data revealed 0.8-10 sec individual oscillation periods, amplitude peaks at 0.4 nT, a carrier-frequency range between 0.05 and 0.4 Hz, and durations of several minutes to days. The Davis SEs were found to occur during magnetic quiescence and to exhibit left-handed polarization.

Affiliated with

Also associated with

No associations

Rating

'Serpentine Emission' at the high latitude Antarctic station, Davis 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 'Serpentine Emission' at the high latitude Antarctic station, Davis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 'Serpentine Emission' at the high latitude Antarctic station, Davis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1598881