Groundbased And Spacecraft Studies of Jupiter At Decameter And Hectometer Wavelengths.
Groundbased And Spacecraft Studies of Jupiter At Decameter And Hectometer Wavelengths.
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The same comments apply of course to the emission occurring in the 30 to 40 MHz region.
Whether or not non-Io emission actually takes place above 30 MHz is unknown (see e.g. Goertz and Haschick 1972) . This particular question has been addressed theoretically by Smith (1976) , though, within the framework of the emission mechanism of Wu (1973) . As seen by Smith, the post-Pioneer magnetic-field model of Jupiter (Acuna and Ness 1975) may preclude the possibility of higher frequency (>30 MHz) non...-Io-related activity. Alternate mechanisms operating in a fundamentally different manner, such as those of Goldstein and Eviatar (1972) or Melrose (1976) , do not explicitly rule out the possibility of such emission however.
Observations made at threshold sensitivities as deduced from the extrapolation of the non-Io curve will aid in discriminating between competing mechanisms. We will explore the interesting 166 problem of the frequency limits of the non-Io emission in Chapter VIII.
VII-5. ROTATION- AND lO-PHASE BEHAVIOR AND CURRENT THEORETICAL MODELS In this chapter the pronounced dependence of the lo-effect on flux density has been shown to account very nicely for the apparent decline in lo control observed at frequencies in the 10- to 20-MHz region.
What to read after Groundbased And Spacecraft Studies of Jupiter At Decameter And Hectometer Wavelengths.?
You can find similar books in the "Read Also" column, or choose other free books by Desch, Michael Daniel, 1947- to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
The same comments apply of course to the emission occurring in the 30 to 40 MHz region.
Whether or not non-Io emission actually takes place above 30 MHz is unknown (see e.g. Goertz and Haschick 1972) . This particular question has been addressed theoretically by Smith (1976) , though, within the framework of the emission mechanism of Wu (1973) . As seen by Smith, the post-Pioneer magnetic-field model of Jupiter (Acuna and Ness 1975) may preclude the possibility of higher frequency (>30 MHz) non...-Io-related activity. Alternate mechanisms operating in a fundamentally different manner, such as those of Goldstein and Eviatar (1972) or Melrose (1976) , do not explicitly rule out the possibility of such emission however.
Observations made at threshold sensitivities as deduced from the extrapolation of the non-Io curve will aid in discriminating between competing mechanisms. We will explore the interesting 166 problem of the frequency limits of the non-Io emission in Chapter VIII.
VII-5. ROTATION- AND lO-PHASE BEHAVIOR AND CURRENT THEORETICAL MODELS In this chapter the pronounced dependence of the lo-effect on flux density has been shown to account very nicely for the apparent decline in lo control observed at frequencies in the 10- to 20-MHz region.
What to read after Groundbased And Spacecraft Studies of Jupiter At Decameter And Hectometer Wavelengths.?
You can find similar books in the "Read Also" column, or choose other free books by Desch, Michael Daniel, 1947- to read onlineMoreLess
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