Solar physics meeting at IIA, Bangalore
Solar physics meeting at IIA, Bangalore Solar physics meeting at IIA, Bangalore
Are we entering another grand minimum right now? Publication date of our paper: August, 2009 Choudhuri & Karak (2009)
Are we entering another grand minimum right now? No! The polar field diminution factor γ at the end of 23 th cycle is 0.6 (Svalgaard, Cliver & Kamide 2000; Choudhuri, Chatterjee & Jiang 2007) which is not sufficient to trigger a Maunder minimum. Choudhuri & Karak (2009)
- 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 and 8: Dynamo Model: Parker (1955) Axisymm
- Page 9 and 10: Poloidal Field Generation:- The Mea
- 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: Dynamo growth rate is determined by
- Page 30: Path between D to A can be advectio
Are we entering another grand<br />
minimum right now?<br />
Public<strong>at</strong>ion d<strong>at</strong>e of our paper:<br />
August, 2009<br />
Choudhuri & Karak (2009)
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