Abstract
A statistical analysis is used to determine the properties of metre-wavelength events which are associated with interplanetary type II bursts. It is found that the likelihood of an interplanetary type II burst is greatly increased if: (a) an associated metre-wavelength type II has a starting frequency less than 45 MHz; (b) a strong metre-wavelength continuum is present; (c) the type II contains herringbone fine structure; and (d) the metre-wavelength activity is accompanied by strong, long-lasting Hα and soft X-ray events.
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Visiting scientist at Division of Radiophysics, January 1983; previous address - NASA/Goddard Space Flight Center, Greenbelt, Maryland.
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Robinson, R.D., Stewart, R.T. & Cane, H.V. Properties of metre-wavelength solar bursts associated with interplanetary type II emission. Sol Phys 91, 159–168 (1984). https://doi.org/10.1007/BF00213621
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DOI: https://doi.org/10.1007/BF00213621