1. Wave-Induced Transport

2. Example: Acoustic Streaming

3. Acoustic Streaming (Quartz Wind) I (Lenoir & Botton 2007)

4. Acoustic Streaming (Quartz Wind) II (Lenoir & Botton 2007)

5. Physics of Acoustic Streaming (Eckart 1948; Lighthill 1978)

6. Solar Atmospheric & Internal Structure (NASA/ESA 2006)

7. Surface & Internal Rotation (Thompson et al. 2003)

8. Solar Magnetism (Arlt 2003) (Dikpati 2010)

9. The Sun (7/2/10)

10. Ideal Magnetohydrodynamics I

11. Ideal Magnetohydrodynamics II

12. Alfvén Waves I

13. Alfvén Waves II

14. Solar Coronal Temperature & Density (Meyer-Vernet 2007)

15. Necessity of Coronal Expansion

16. Observed Solar Wind Speed Ulysses (1992-2009) (McComas et al. 2003)

17. Solar Wind Properties (Hansteen 2009)

18. Constraints on Acceleration Mechanisms (Leer & Holzer 1980)

19. Alfvén Waves in the Solar Wind Mariner 5 (Venus 1967) (Belcher & Davis 1971)

20. Alfvén Waves in the Solar Corona (Tomczyk et al. 2007)

21. Alfvén Waves in the Chromosphere Solar Optical Telescope – Hinode (McIntosh et al. 2010) Spicules

22. Alfvén Wave-Driven Wind Model

23. Wave Amplitudes in a Steady Flow

24. Wave-Modified Thermally Driven Wind

25. Wave Amplitudes

26. Wave Energy Flux

27. Wind Force Balance

28. Winds with Non-WKB Alfvén Waves I

29. Winds with Non-WKB Alfvén Waves II

30. Winds with Non-WKB Alfvén Waves III

31. Gravity Waves I

32. Gravity Waves II

33. Gravity Wave Propagation I

34. Gravity Wave Propagation II (Mowbray & Rarity 1967)

35. Gravity Wave Excitation I Ice-Water Convection Experiment (Malkus 1960; Townsend 1964; Adrian 1975) (M. MacGregor 2004)

36. Gravity Wave Excitation II (Townsend 1964)

37. Gravity Wave Excitation III (Ansong & Sutherland 2010)

38. Gravity Wave Excitation IV (Rogers & Glatzmaier 2005; Rempel 2004)

39. Gravity Wave - Shear Flow Interaction

40. The Quasi-Biennial Oscillation (Baldwin et al. 2001)

41. The Plumb-McEwan Experiment (1978)

42. Gravity Wave-Driven Flows Wave Interactions with Tachocline Rotational Shear

43. Oscillatory Flow Properties

44. Origin of Oscillatory Behavior

45. Time-Dependent Flow Properties (Thompson et al. 2003)

46. Gravity Waves & Internal Solar Rotation I Interaction of Waves with Non-uniform Rotation

47. Gravity Waves & Internal Solar Rotation II (Talon, Kumar, & Zahn 2002)

48. Conclusion/Extensions Interactions between small-scale waves and the media through which they propagate can have large-scale dynamical consequences in a variety of astrophysical systems Wave-dominated flows – winds from cool evolved stars Radiative amplification of acoustic/Alfvén waves in hot star winds Accretion-generated Alfvén/gravity waves in pre-MS objects Internal excitation of gravity modes by planetary companions Alfvén waves from satellite-planet, planet-star interactions Some examples/possibilities: