The structure of the global solar magnetic field excited by the turbulent dynamo mechanism

ISSN： 1063-7729

Source： Astronomy Reports, Vol.45, Iss.9, 2001-09, pp. : 738-745

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Related content

Simple Model of a Stochastically Excited Solar Dynamo

By Mininni Pablo Gomez Daniel Mindlin Gabriel

Solar Physics, Vol. 201, Iss. 2, 2001-07 ,pp. : 203-223

Springer Publishing Company

Access to resources Recommend Favorite

Statistical analysis of the mass-to-flux ratio in turbulent cores: effects of magnetic field reversals and dynamo amplification

By Bertram E. Federrath C. Banerjee R. Klessen R. S.

Monthly Notices of the Royal Astronomical Society, Vol. 420, Iss. 4, 2012-03 ,pp. : 3163-3173

Oxford University Press

Access to resources Recommend Favorite

The solar cycle from data on the large-scale surface magnetic field and solar-dynamo theory

By Popova E. Sokoloff D.

Astronomy Reports, Vol. 54, Iss. 11, 2010-11 ,pp. : 1042-1046

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite

Fluctuations of the Solar Dynamo Observed in the Solar Wind and Interplanetary Magnetic Field at 1 AU and in the Outer Heliosphere

By Mursula K. Vilppola J.H.

Solar Physics, Vol. 221, Iss. 2, 2004-06 ,pp. : 337-349

Springer Publishing Company

Access to resources Recommend Favorite

Quasi-biennial oscillations of the global solar magnetic field

By Obridko V. Shelting B.

Astronomy Reports, Vol. 45, Iss. 12, 2001-12 ,pp. : 1012-1017

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite