RT @KoderaSoftware @lougrims VASIMR is the nearest real-world approximation of rockets I have in game- a reference point. The in-game rocket you see is a NTRL (NTR/MHD hybrid) - with hydrogen/oxygen plasma initially heated by nuclear reactor and further a…
RT @SIRISYSPrime Almost no part of that entry point seems like a good idea. . . You basically are starting here: "Magnetic helicity, K (self linkage of magnetic field lines), Where A = the vector potential, B = the magnetic field … buff.ly/2yb5yz4
RT @Un1v3rs0Z3r0 Determining the Transport of Magnetic Helicity and Free Energy in the Sun's Atmosphere [SSA] buff.ly/2K3zpPs
RT @arXiver Determining the Transport of Magnetic Helicity and Free Energy in the Sun's Atmosphere [SSA] buff.ly/2K3zpPs buff.ly/2K27XSs
RT @mathAPb Rajendra Beekie, Tristan Buckmaster, Vlad Vicol : Weak solutions of ideal MHD which do not conserve magnetic helicity buff.ly/2Y45ErO buff.ly/2Y45FvS
RT @livrev_lrsp New book: Bernard Roberts "MHD Waves in the Solar Atmosphere" (CUP 2019) buff.ly/2O6rJ4B
RT @FalseWiki Andrew Parkinson is a technique of studying the plasma of the Sun's corona with the use of magnetohydrodynamic (MHD) waves and oscillations.
RT @Un1v3rs0Z3r0 Magnetic helicity and eruptivity in active region 12673 [SSA] buff.ly/2jYZMNT
RT @arXiver Magnetic helicity and eruptivity in active region 12673 [SSA] buff.ly/2jYZMNT buff.ly/2jYX374
RT @DVerscharen Our HolmMHD code is now publicly available for download under buff.ly/2Xwi1HS. It solves the polytropic, isotropic MHD equations. The paper that describe the code will come out shortly. #numerical #plasma #… buff.ly/2XtNGtD
RT @HirokiAkamatsu Allard Jan van Marle will talk about "Numerical models of particle acceleration in astrophysical shocks: the influence of the Mach number and plasma-beta on the acceleration process" Nice introduction of particles in MHD cells. Keppens+…
RT @HirokiAkamatsu David Ball will talk about "Electron Acceleration in Magnetic Reconnection: Dependence on Magnetization and Plasma-Beta" X-ray flares from SGR A* . Several flares but no flares in MHD models (e.g., Chan+15). need nonthermal electrons. P…
RT @spheromak : @corbinbleeuu 10 + (8-(10-6)) Longer form: 10-6 =4 8-4=4 10+4 = 14 I am thinking how much of 8 do I need to add to 6 to get to ten. Fun to break down how we think abt math.
RT @X_DenJP ITER la fusion test. Il faudra contrôler le plasma MHD en boucle vers une sortie et récupérer l'énergie au passage avec l'aide d'une mèche ou d'un filin adéquat ou le déplacer en rythme mesuré vers des matériaux de la … buff.ly/2EYY4Vm
RT @alexgagliano : Day 2 : A tour of the Swarthmore Spheromak Experiment (SSX)! The lab studies magnetic reconnection using rings of plasma called spheromaks, in the hopes of better understanding solar flares and coronal mass ejec… buff.ly/2ZzYGak
RT @astrotweeps Alemayehu Cherkos - Effect of viscosity on propagation of MHD waves in astrophysical plasma #FSTPII buff.ly/2RroH8N
RT @spheromak : @fujin_ @dysinger Basically everything should have these. I want to C-r in slack every day.
RT @alexgagliano Day 1 of GPAP2019 done. Topics covered: Introduction to plasma physics, turbulence, hydro, and MHD...we'll see if there's anything left for day two! buff.ly/31Kfygj
