Reply to comments of Dikpati et al
arXiv:astro-ph/0505232 · doi:10.1051/0004-6361:20052934
Abstract
We present here our response to Dikpati et al.'s criticism of our recent solar dynamo model.
8 pages, 2 figures
References in corpus (1)
Cited by in corpus (12)
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- A dynamo model of magnetic activity in solar-like stars with different rotational velocities
- Correlation between Decay Rate and Amplitude of Solar Cycles as Revealed from Observations and Dynamo Theory
- Quenching of Meridional Circulation in Flux Transport Dynamo Models
- Development of twist in an emerging magnetic flux tube by poloidal field accretion
- Simulation Study of Hemispheric Phase-Asymmetry in the Solar Cycle
- Supercriticality of the dynamo limits the memory of the polar field to one cycle
- The treatment of magnetic buoyancy in flux transport dynamo models
- A Critical Assessment of the Flux Transport Dynamo
- Astrophysics in 2005