Abstract Incoherent scatter observations of the ionosphere have been used to monitor the passage of atmospheric gravity waves. The period of a wave and its vertical wavelength can be derived from profiles of electron concentration or field-aligned plasma velocity, and measurements of this kind have been used to confirm the Hines' dispersion equation. On occasions waves have been observed which maintain a regular periodicity over many cycles. Incoherent scatter can also be used to study the source region of large-scale atmospheric gravity waves in the auroral zone. Such observations have identified Joule heating and Lorentz forcing in the auroral electrojet as the main mechanisms for generating large-scale waves which are later observed at mid-latitude propagating equatorwards. The observations often reveal a quasi-periodicity in the substorm electric field which largely determines the periodicity of the wave launched by the electrojet, although this may be modified in the far-field by filtering and dispersion.
Observations of atmospheric gravity waves with incoherent scatter radar
Advances in Space Research ; 9 , 5 ; 65-72
01.01.1989
8 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Incoherent Scatter Radar Observations Related to Magnetospheric Dynamics
British Library Conference Proceedings | 1997
|Incoherent scatter radar contributions
Elsevier | 1989
|Incoherent Scatter Radar Observations Related to Magnetospheric Dynamics
Online Contents | 1997
|