![Kinematics: Advection, Diffusion and Intensification of Magnetic Fields (Chapter 5) - Introduction to Magnetohydrodynamics Kinematics: Advection, Diffusion and Intensification of Magnetic Fields (Chapter 5) - Introduction to Magnetohydrodynamics](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20171227025936286-0437:9781316672853:16016fig5_1.png?pub-status=live)
Kinematics: Advection, Diffusion and Intensification of Magnetic Fields (Chapter 5) - Introduction to Magnetohydrodynamics
![The Origin of Major Solar Activity: Collisional Shearing between Nonconjugated Polarities of Multiple Bipoles Emerging within Active Regions | HMI Science Nuggets The Origin of Major Solar Activity: Collisional Shearing between Nonconjugated Polarities of Multiple Bipoles Emerging within Active Regions | HMI Science Nuggets](http://hmi.stanford.edu/hminuggets/wp-content/uploads/2019/02/f3_Georgios.png)
The Origin of Major Solar Activity: Collisional Shearing between Nonconjugated Polarities of Multiple Bipoles Emerging within Active Regions | HMI Science Nuggets
![Validation of the PDFI SS method for electric field inversions using magnetic flux emergence simulations | High Altitude Observatory Validation of the PDFI SS method for electric field inversions using magnetic flux emergence simulations | High Altitude Observatory](https://www2.hao.ucar.edu/sites/default/files/styles/extra_large/public/2022-10/Fang_3D-MHD-simulationEmergenceTwistedMagneticFluxTube.png?itok=zsUfAohe)
Validation of the PDFI SS method for electric field inversions using magnetic flux emergence simulations | High Altitude Observatory
![Direct evidence that twisted flux tube emergence creates solar active regions | Nature Communications Direct evidence that twisted flux tube emergence creates solar active regions | Nature Communications](https://media.springernature.com/full/springer-static/image/art%3A10.1038%2Fs41467-021-26981-7/MediaObjects/41467_2021_26981_Fig1_HTML.png)
Direct evidence that twisted flux tube emergence creates solar active regions | Nature Communications
![Sensors | Free Full-Text | Simulations of Switchback, Fragmentation and Sunspot Pair in δ-Sunspots during Magnetic Flux Emergence Sensors | Free Full-Text | Simulations of Switchback, Fragmentation and Sunspot Pair in δ-Sunspots during Magnetic Flux Emergence](https://www.mdpi.com/sensors/sensors-21-00586/article_deploy/html/images/sensors-21-00586-g001.png)
Sensors | Free Full-Text | Simulations of Switchback, Fragmentation and Sunspot Pair in δ-Sunspots during Magnetic Flux Emergence
![The equilibrium configuration. The uniformly twisted magnetic flux tube... | Download Scientific Diagram The equilibrium configuration. The uniformly twisted magnetic flux tube... | Download Scientific Diagram](https://www.researchgate.net/publication/232244450/figure/fig10/AS:300528320958481@1448662943371/The-equilibrium-configuration-The-uniformly-twisted-magnetic-flux-tube-is-in-an-ambient.png)
The equilibrium configuration. The uniformly twisted magnetic flux tube... | Download Scientific Diagram
![Basic concepts on the physics of the magnetic flux tubes formation near the Earth | Pedro P. Ferreira Basic concepts on the physics of the magnetic flux tubes formation near the Earth | Pedro P. Ferreira](https://pedropferreira.org/publication/ferreira2017/featured.png)
Basic concepts on the physics of the magnetic flux tubes formation near the Earth | Pedro P. Ferreira
![Magnetic flux tubes in the penumbra. For a given heliocentric angle θ,... | Download Scientific Diagram Magnetic flux tubes in the penumbra. For a given heliocentric angle θ,... | Download Scientific Diagram](https://www.researchgate.net/publication/233341425/figure/fig2/AS:668925180268559@1536495599739/Magnetic-flux-tubes-in-the-penumbra-For-a-given-heliocentric-angle-th-the-azimuth-ph-and.png)