Related content

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

By Knyazeva I.   Makarenko N.  

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

MAIK Nauka/Interperiodica

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

Investigation of Long-Period Oscillations of Sunspots with Ground-Based (Pulkovo) and SOHO/MDI Data

By Efremov V.   Parfinenko L.   Solov’ev A.  

Solar Physics, Vol. 267, Iss. 2, 2010-12 ,pp. : 279-293

Springer Publishing Company

Access to resources Recommend Favorite

Analysis of Supergranule Sizes and Velocities Using Solar Dynamics Observatory (SDO)/Helioseismic Magnetic Imager (HMI) and Solar and Heliospheric Observatory (SOHO)/Michelson Doppler Imager (MDI) Dopplergrams

By Williams Peter   Pesnell W.   Beck John   Lee Shannon  

Solar Physics, Vol. 289, Iss. 1, 2014-01 ,pp. : 11-25

Springer Publishing Company

Access to resources Recommend Favorite

Are Solar Active Regions with Major Flares More Fractal, Multifractal, or Turbulent Than Others?

By Georgoulis Manolis  

Solar Physics, Vol. 276, Iss. 1-2, 2012-02 ,pp. : 161-181

Springer Publishing Company

Access to resources Recommend Favorite