Publication Date:
2019-07-27
Description:
The LF radio emission of the heliospheric cavity is discussed, summarizing Voyager measurement data. The solar wind is considered to be the outer layer of the solar atmosphere, and its interaction with the interstellar medium is examined in detail. Typical data are presented graphically, and theoretical models proposed to explain the emission are reviewed. It is suggested that the emission may originate at the terminal shock or heliopause, thus providing a means of estimating its location.
Keywords:
ASTROPHYSICS
Type:
COSPAR Colloquium; Sept. 19-22, 1989; Warsaw; Poland
Format:
text