Statistics
Scientific paper
Feb 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988georl..15..168k&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 15, Feb. 1988, p. 168-171.
Statistics
12
Auroras, Cosmic Noise, Geomagnetic Micropulsations, Magnetospheric Instability, Propagation Velocity, Riometers, Kelvin-Helmholtz Instability, Morning
Scientific paper
A new type of cosmic noise absorption (CNA) pulsation observed with a scanning beam riometer with a spatial resolution of 10 km at Syowa Station in Antarctica is reported. The scanning beam riometer system is described, and an example and some statistics for the new type of CNA pulsation are presented. The pulsation has a short azimuthal wavelength corresponding to a large azimuthal m-number. Most of the CNA pulsations propagate eastward in the morning sector. A possible cause of the new type of pulsation is discussed in relation to the drift motion of pulsating auroras.
Kikuchi Takashi
Sato Natsuo
Yamagishi Hisao
No associations
LandOfFree
Eastward propagation of PC4-5 range CNA pulsations in the morning sector observed with scanning narrow beam riometer at L = 6.1 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 Eastward propagation of PC4-5 range CNA pulsations in the morning sector observed with scanning narrow beam riometer at L = 6.1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Eastward propagation of PC4-5 range CNA pulsations in the morning sector observed with scanning narrow beam riometer at L = 6.1 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1225836