A new method for reconstructing type III trajectories

Details A new method for reconstructing type III trajectories A new method for reconstructing type III trajectories

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..106..397r&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 106, Aug. 1986, p. 397-401.

Astronomy and Astrophysics

Astronomy

8

Approximation, Electron Density (Concentration), Electron Trajectories, Interplanetary Medium, Type 3 Bursts, Drift Rate, Frequency Shift, Radio Sources (Astronomy), Reconstruction, Spaceborne Astronomy

Scientific paper

A local density approximation (LDA) method is developed for reconstructing the trajectories of type III radio bursts through the interplanetary medium. The method uses the measured source directions and the measured frequency drift rates of the type III burst to determine the locations of the radio source in the interplanetary medium at consecutive frequency levels. The technique is used to reconstruct the trajectory of an actual type III burst and the results are compared to the trajectory obtained from the global density law method. The LDA method represents an improvement in that it utilizes more observed data on the type III burst and that it takes full account of the local density variations at the source locations.

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