Electron heat conduction in the solar wind: Transition from spitzer-härm to the collisionless limit

Physics & Astronomy

• solar wind 98%
• conductive heat transfer 96%
• heat flux 88%
• electrons 41%
• mean free path 39%
• collisional plasmas 26%
• wave-particle interactions 26%
• temperature profiles 19%
• temperature gradients 17%
• astrophysics 17%
• electron energy 14%
• saturation 13%
• electric potential 10%

Earth & Environmental Sciences

• solar wind 100%
• heat flux 90%
• electron 68%
• transition 61%
• temperature profile 19%
• temperature gradient 19%
• plasma 15%
• saturation 14%
• regulation 13%
• particle 9%
• effect 4%