Helioseismology probes solar interior structure by analyzing oscillation modes of the photosphere.
- True - reveals convection zone depth/radiative zone rotation
- False - only studies surface
- True - but only for flares
- False - requires spacecraft
Answer: True - reveals convection zone depth/radiative zone rotation
p-mode/g-mode frequencies constrain internal sound speed profile, revealing tachocline location and differential rotation; validated solar models.