Underlying Processes of the Jovian Decametric Radiation /
Underlying Processes of the Jovian Decametric Radiation /
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Expeifience has shown the third order alias effects are negligibly small and thus they will be ignored, Table 11 shows the expected frequencies for the various satellites. In scanning the table the redundancies become apparent. lo, Europa, and Ganymede all have predicted periods in the range of frequency index 14 to 16, while 119 Europa and Ganymede have components in the 30 to 32 range.
The plots in Figures 30, 31, and 32 depict the frequency spectra of the daily activity index Ag(t) as define...d in Chapter 2 for 1967-68. In principle, this function is free of the observation spectra previously displayed in Figure 29. In these plots the lo effect has deliberately not been removed in order to demonstrate the effect of a periodic exciter on the data. Source B has long been recognized as the prototype for lo related activity. These plots show clearly that this is the case. The lo features in the vicinity of indices 14-16, 30-31 and 47 are the dominant features in the source B spec- trum. All but the strong peak at index 17 can be attributed to the loian, Jovian, and joint interactions outlined in Table 9.
What to read after Underlying Processes of the Jovian Decametric Radiation /?
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To quickly assess the difficulty of the text, read a short excerpt:
Expeifience has shown the third order alias effects are negligibly small and thus they will be ignored, Table 11 shows the expected frequencies for the various satellites. In scanning the table the redundancies become apparent. lo, Europa, and Ganymede all have predicted periods in the range of frequency index 14 to 16, while 119 Europa and Ganymede have components in the 30 to 32 range.
The plots in Figures 30, 31, and 32 depict the frequency spectra of the daily activity index Ag(t) as define...d in Chapter 2 for 1967-68. In principle, this function is free of the observation spectra previously displayed in Figure 29. In these plots the lo effect has deliberately not been removed in order to demonstrate the effect of a periodic exciter on the data. Source B has long been recognized as the prototype for lo related activity. These plots show clearly that this is the case. The lo features in the vicinity of indices 14-16, 30-31 and 47 are the dominant features in the source B spec- trum. All but the strong peak at index 17 can be attributed to the loian, Jovian, and joint interactions outlined in Table 9.
What to read after Underlying Processes of the Jovian Decametric Radiation /?
You can find similar books in the "Read Also" column, or choose other free books by Kennedy, James Richard, 1941- to read onlineMoreLess
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