PPT-Processes underlying the variation of the magnetic field spectral index in the inner solar

J R McIntyre C H K Chen Turbulence process by which energy injected at large scales in a system is transported to small scales where it can be dissipated The solar wind known to contain a turbulent cascade proposed that it plays a role in the heating and acceleration of the wind. 09:50, Friday November 21 . auditorium . Reine. Elisabeth. Session: 14 Space Climate . Time allowed 20 min. Mike . Lockwood. , . L. Barnard. , C.J. . Scott, & M.J. Owens. (Department . of Meteorology, University of Reading, . How to snag that DX!. Michael Smith, N5TGL. Agenda. Purpose. Three Magic words. Understanding . Propagation. Propagation modes. How . solar activity impacts the ionosphere. Learning . the numbers. A and K index, SFI, 304A, . Solar Prominence. Sun Fact Sheet. The Sun is a normal G2 star, one of more than 100 billion stars in our galaxy.. . Diameter: . 1,390,000 km. (Earth 12,742 km or nearly 100 times smaller). Mass: . 1.1989 x 10. Chapter 8:. Outflow and Accretion. Yosuke Mizuno. Institute of Astronomy. National . Tsing-Hua. University. Outflow and Accretion. In the universe, . outflow. and . accretion. are common feature.. N. U. Crooker, S. W. . Antiochos. ,. . X. Zhao, Yi-M. Wang, and . M. . . Neugebauer. Source of solar wind. Coronal holes (Open field regions) . . Egidio Landi Degl’Innocenti. Dipartimento di Fisica e Astronomia. Università di Firenze, Italia. Banja Koviljaca, May 13-17, 2013. 9th Serbian Conference on Spectral Line Shapes in Astrophysics. Line shapes I. P. ropagation . T. ool. Chihiro Tao. 1,2. ,. . Nicolas Andre. 1. , Vincent Génot. 1. , Alexis P. Rouillard. 1. , Elena Budnik. 1. , Arnaud Biegun. 1. , Andrei Fedorov. 1. 1. IRAP, Univ. de Toulouse/UPS-OMP/CNRS. Dr. Phillip C. Anderson. W. B. Hanson Center for Space Sciences. University of Texas at Dallas. What is Space Weather?. The conditions and processes occurring in space which have the potential to affect the near Earth environment. . basic concepts and magnetic topology . Anna (. Ania. ) . Malanushenko. Plasma. Is matter…. Mass is conserved. Momentum is conserved. Energy is conserved. …ionized and in magnetic field. Obeys Maxwell’s equations. Mathew Owens. 1. Space and Atmospheric Electricity group. Department of Meteorology. HMF: big Questions . (that I probably won’t answer today). What are the physical processes by which the the heliospheric magnetic field (HMF) evolve?. Substorms. 2. 5-29 September 2017. Portsmouth, New Hampshire, USA. . Double Magnetic Reconnection Driven by Kelvin-Helmholtz . Vortices. W. . Horton. 1. , M. Faganello. 2. , F. . Pegoraro. 2. F.Califano. the Heliosphere. Riaan Steenkamp. University of Namibia. . 5. . July . 2018. History and Discovery. A short history of the discovery of Cosmic Rays. At beginning of 20. th. Century:. Hypothesis: . Introduction. Solar flares occur when energy is converted into x-rays ,heat & supersonic fluid motion.. Energy is stored in magnetic filed lines.. Electric field changes connectivity of magnetic field lines and the energy is released.. Open: Venus – solar wind. Closed: Venus – Venus. Draped: solar wind – solar wind. Magnetic fields guide ion and electron motions. The connectivity (topology) of these field lines helps us to understand how the upper atmosphere interacts with the solar wind..