Evolution of the magnetic fields of solar flare active regions from the geometry and topology of HMI/SDO magnetograms

ISSN： 1063-7729

Source： Astronomy Reports, Vol.58, Iss.3, 2014-03, pp. : 145-155

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

Fractal and Multifractal Properties of Active Regions as Flare Precursors: A Case Study Based on SOHO/MDI and SDO/HMI Observations

By Ermolli I. Giorgi F. Romano P. Zuccarello F. Criscuoli S. Stangalini M.

Solar Physics, Vol. 289, Iss. 7, 2014-07 ,pp. : 2525-2545

Springer Publishing Company

Access to resources Recommend Favorite

The Topology of Background Magnetic Fields and Solar Flare Activity

By Mordvinov A.V. Salakhutdinova I.I. Plyusnina L.A. Makarenko N.G. Karimova L.M.

Solar Physics, Vol. 211, Iss. 1-2, 2002-12 ,pp. : 241-253

Springer Publishing Company

Access to resources Recommend Favorite

Determination of magnetic helicity content of solar active regions from SOHO/MDI magnetograms

By Chae Jongchul Moon Yong-Jae Park Young-Deuk

Solar Physics, Vol. 223, Iss. 1-2, 2004-09 ,pp. : 39-55

Springer Publishing Company

Access to resources Recommend Favorite

Analyses of Vector Magnetograms in Flare-Productive Active Regions

By Wang H.

Solar Physics, Vol. 174, Iss. 1-2, 1997-08 ,pp. : 163-173

Springer Publishing Company

Access to resources Recommend Favorite

Integral properties of the magnetic fields of solar active regions under quiet and flare activity conditions

By Chumak O. Zhang H. Gou J.

Astronomical and Astrophysical Transactions, Vol. 23, Iss. 6, 2004-12 ,pp. : 525-531

Taylor & Francis Ltd

Access to resources Recommend Favorite