The structure of our Milky Way galaxy: a container of gas and stars arranged in various components with various properties.. Gaseous halo? ~ 6 x 10 10.
Turbulence and Wave Dissipation in the Chromosphere, Corona, and Solar Wind Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics.
Turbulent Heating of Protons, Electrons, & Heavy Ions in the Tangled & Twisted Solar Corona Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics.
Turbulence in the Solar Corona Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics.
Incorporating Kinetic Effects into Global Models of the Solar Wind Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics.
