MHD simulations of coronal heating
The problem of heating the solar corona requires the conversion of magnetic energy into thermal energy. Presently, there are two promising mechanisms for heating the solar corona: wave heating and nanoflare heating.
Tam, Kuan V.
core
Helioseismic evidence that the solar dynamo originates near the tachocline. [PDF]
Mandal K, Kosovichev AG.
europepmc +1 more source
A Fuzzy Fishier Mantis Optimizer method for MPPT in PV solar system. [PDF]
Elwaer HE, Avci SA, Rahebi J.
europepmc +1 more source
Nonlinear stability and vibration of flexible spacecraft solar arrays under thermally induced flutter during the penumbra phase. [PDF]
Motaharifard O +2 more
europepmc +1 more source
Regression and statistical analysis of heat transfer enhancement in water/ethylene glycol (40/60) base molybdenum carbide (Mo<sub>2</sub>C) MXene nanofluid using a transient fractional model. [PDF]
Sheikh NA +4 more
europepmc +1 more source
Resilient virtual inertia strategy for frequency support of renewable-based microgrids using a variable structure fuzzy PID controller. [PDF]
Abdelghany MA +3 more
europepmc +1 more source
High-efficiency predictive torque control of induction motors in PV water pumping using GTO-optimized PI controller. [PDF]
Kechida R +7 more
europepmc +1 more source
Development and application of a global magnetic field evolution model for the solar corona
Magnetic fields are fundamental to the structure and dynamics of the Sun’s corona. Observations show them to be locally complex, with highly sheared and twisted fields visible in solar filaments/prominences.
Yeates, Anthony Robinson
core
Impact of metal filings and acoustic waves on solar still performance. [PDF]
Elwekeel FNM +3 more
europepmc +1 more source
Numerical Modeling of Prominences and Coronal Rain with the MPI-AMRVAC Code. [PDF]
Liakh V, Jenkins J.
europepmc +1 more source

