Abstract
We argue that the solar g-modes are unlikely to have caused the discrete peaks in the power spectrum of the solar wind flux observed by Thomson et al (1995). The lower limit to the energy of individual g-modes, using the amplitudes
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CITATION STYLE
APA
Kumar, P., Quataert, E. J., & Bahcall, J. N. (1996). Observational Searches for Solar [ITAL]g[/ITAL]-Modes: Some Theoretical Considerations. The Astrophysical Journal, 458(2). https://doi.org/10.1086/309926
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