And here, when magnetized bubble piles up at the boundary of the two layers, a sufficiently strong vert. grad. of B may satisfy criteria for magnetic buoyancy instabilities, and let the top part of the bubble to erupt into the stably stratified layer. http
RT @markcheung: Just had to search for some #solar #MHD refs and found this to be helpful https://t.co/78WgRyLNhz Disclosure: by yours trul…
RT @markcheung: Just had to search for some #solar #MHD refs and found this to be helpful https://t.co/78WgRyLNhz Disclosure: by yours trul…
これが出版されたの2014年かあ。ずいぶん時間が経ったな
Just had to search for some #solar #MHD refs and found this to be helpful https://t.co/78WgRyLNhz Disclosure: by yours truly 🤗 and @isobehiroaki
Flux Emergence (Theory) http://t.co/pzeMtaDyce solar activity and different physical effects e.g., magnetic buoyancy, magnetoconvection ...
"Flux Emergence (Theory)" by Mark C. M. Cheung and Hiroaki Isobe http://t.co/sAf7RI6xUo #SolarPhysics @isobehiroaki http://t.co/47HZhSKgq4
"Flux Emergence (Theory)" by Mark C. M. Cheung and Hiroaki Isobe http://t.co/sAf7RI6xUo #SolarPhysics @isobehiroaki http://t.co/47HZhSKgq4
"Flux Emergence (Theory)" by Mark C. M. Cheung and Hiroaki Isobe http://t.co/sAf7RI6xUo #SolarPhysics @isobehiroaki http://t.co/47HZhSKgq4