Slide 1 Magnetic fields in the photosphere and heliosphere: structure, statistical parameters, turbulent state Valentyna I. Abramenko Big Bear Solar Observatory of NJIT Email:…
Slide 1 Can the coronal field’s susceptibility to emergence-induced eruption be estimated? SSPVSE Discussion Group B, Wed., 19 Oct. 2005 B. Welsch, Space Sciences Lab,…
Calculating Magnetic Energy in Active Regions Using Coronal Loops for AR 11092 and AR 11112 Presentation by, Joseph B. Jensen Magnetic energy equation Non-linear force-free…
Spatio-Temporal Dynamics of Magnetic Fields and Flaring Productivity of Active Regions Valentina I. Abramenko Big Bear Solar Observatory of NJIT Email: [email protected]…