Abstract
Whistlers observed on the ground with frequency cutoffs greater than one‐half the equatorial electron gyrofrequency along their field‐aligned propagation paths have been termed super whistlers. The rarity of the super whistler is a consequence of the relatively small number of ducts which allow their propagation. The upper cutoff frequency of the super whistler is directly related to the physical structure of the duct. In addition to the path location and equatorial electron density that can be deduced from ordinary whistlers, super whistlers also provide information on density gradients along the magnetic field lines near the equator. Analysis of one set of super whistlers shows that immediately after a magnetic disturbance the equatorial plasma near L=4.5 is in an intermediate state between the collisionless and diffusive equilibrium distributions. The plasma distribution approaches that of diffusive equilibrium after a period of low geomagnetic activity.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
