Solar physics meeting at IIA, Bangalore

More documents

Recommendations

Info

Toroidal Field Generation (ω Effect) (Schou et al. 1998; Observationally verified Charbonneau et al. 1999)
Poloidal Field Generation:– The Mean Field α- effect/classical α-effect • Small scale helical convection – Mean-Field α-effect (Parker 1955) • Buoyantly yrising toroidal field is twisted by helical turbulent convection, creating loops in the poloidal plane • The small-scale loops diffuse to generate a large-scale poloidal field
Page 1 and 2: A possible explanation of Maunder m
Page 3 and 4: Maunder minimum: ‣Galileo's s Tel
Page 5 and 6: Usual 11-year period of solar activ
Page 7: Dynamo Model: Parker (1955) Axisymm
Page 11 and 12: In axisymmetry case Velocity field=
Page 13 and 14: Transport mechanisms: 1) meridional
Page 15 and 16: Chatterjee et al. (2004)
Page 17 and 18: 2. Fluctuation in the meridional ci
Page 19 and 20: ∂B 1⎡ ∂ ∂ ⎤ 2 1 + ( rvrB)
Page 21 and 22: How to introduce fluctuation? The s
Page 23 and 24: all Choudhuri & Karak (2009)
Page 25 and 26: Dynamo growth rate is determined by
Page 27 and 28: Are we entering another grand minim
Page 30: Path between D to A can be advectio

Solar physics meeting at IIA, Bangalore

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?