Observation of Equatorial Electrodynamics in Africa using AMBER Magnetometer Network Endawoke Yizengaw Institute for Scientific Research, Boston College,
Magnetism and Rotation in Herbig Ae/Be stars E. Alecian Laboratoire d’Astrophysique de l’Observatoire de Grenoble In collaboration with G.A. Wade, C. Catala,
Observation of a Non Thermal Continuum radio event during the CLUSTER Tilt campaign 17th CLUSTER Workshop Uppsala, Sweden, 12 – 15 May 2009 Uppsala May.
It can be powered by NUCLEAR ENERGY! Luminosity ~ 10 billion years Nuclear Potential Energy (core) E = mc 2 - Einstein, 1905.
Stellar Spectroscopy during Exoplanet Transits Dissecting fine structure across stellar surfaces Dainis Dravins *, Hans-Günter Ludwig, Erik Dahlén, Hiva.
Auroras Now! Auroral nowcasting service for hotels, amateur astronomers, and general public Kauristie, K.1), Mälkki, A.1), Ketola, A.1), Nevanlinna, H.1),
General Properties Absolute visual magnitude M V = 4.83 Central temperature = 15 million 0 K X = 0.73, Y = 0.25, Z = 0.02 Initial abundances: Age: ~ 4.52.
M D WARF V ARIABILITY & T RANSITS I N T HE N EAR I NFRARED RoPACS Meeting Lisbon 2010 Niall Goudling ([email protected])
Announcements Pick up graded homework Seminar on gravitational waves today, 1:00, SL 240 No class this Friday! Test next week on material through today’s.
The EUV spectral irradiance of the Sun from minimum to maximum Giulio Del Zanna Department of Space and Climate Physics University College London Vincenzo.
Forbes CME Hones TPE 5101520 50 100 150 200 250 300 Distance in Rs Acceleration (m/s 2 ) CME Acceleration 50100150200 400 600 800 1000 1200 Solar Wind.
Understanding the Connection Between Magnetic Fields in the Solar Interior and Magnetic Activity in the Corona W.P. Abbett and G.H. Fisher, B.T. Welsch,