Read the passage below:
For decades, solar astrophysicists have sought to explain why the Sun's corona reaches temperatures exceeding a million kelvins, far hotter than the underlying photosphere. Early theoretical models postulated that acoustic waves generated in the convective zone carry thermal energy upward, yet spectroscopic observations subsequently demonstrated that these waves dissipate long before reaching the upper atmosphere. Current debate primarily divides researchers between proponents of magnetohydrodynamic wave dissipation and those advocating for the nanoflare model, which posits that millions of tiny, continuous magnetic reconnection events release stored magnetic energy into the coronal plasma. High-resolution observations from recent orbital observatories have provided empirical support for the nanoflare hypothesis by detecting transient, localized temperature spikes in coronal loops that correlate precisely with predicted magnetic field stress thresholds. Consequently, while wave-based heating may still contribute peripherally to coronal energetics, localized magnetic reconnection is increasingly regarded as the primary mechanism sustaining extreme coronal temperatures.
Which sentence in the passage provides specific observational evidence supporting a particular proposed mechanism for coronal heating?
- High-resolution observations from recent orbital observatories have provided empirical support for the nanoflare hypothesis by detecting transient, localized temperature spikes in coronal loops that correlate precisely with predicted magnetic field stress thresholds.Answer
- BEarly theoretical models postulated that acoustic waves generated in the convective zone carry thermal energy upward, yet spectroscopic observations subsequently demonstrated that these waves dissipate long before reaching the upper atmosphere.
- CCurrent debate primarily divides researchers between proponents of magnetohydrodynamic wave dissipation and those advocating for the nanoflare model, which posits that millions of tiny, continuous magnetic reconnection events release stored magnetic energy into the coronal plasma.
- DConsequently, while wave-based heating may still contribute peripherally to coronal energetics, localized magnetic reconnection is increasingly regarded as the primary mechanism sustaining extreme coronal temperatures.
- EFor decades, solar astrophysicists have sought to explain why the Sun's corona reaches temperatures exceeding a million kelvins, far hotter than the underlying photosphere.