Samir Mandal Indian Institute of Space Science & Technology IISER, 18th November 2011 Accretion and Radiative Processes Around Black Hole Candidates.
Locarno, 8 June 2005Peter Gallagher (UCD) Chromospheric Evaporation Peter Gallagher University College Dublin Ryan Milligan Queens University Belfast.
Lyndsay Fletcher, University of Glasgow Ramaty High Energy Solar Spectroscopic Imager Fast Particles in Solar Flares The view from RHESSI (and TRACE) MRT.
Connecting Simulations with Observations of the Galactic Center Black Hole
The Frequency Agile Solar Radiotelecope
On the Sources Above the Neutral Line of Radial Magnetic Fields in Solar Active Regions
Inversions of Flaring Radio Emissions
Microwave Observations of Compact Radio Sources During Solar Eclipses and Ballooning
Main-Cluster XIS0XIS1XIS3 Weighted mean Chandra Figure 2 : XIS spectra of the main-cluster XIS0 0.4-10keV Main-Cluster Sub-Cluster Search for Bulk Motion.
Small scale energy release can play an important role in many phenomena: solar flares, coronal heating, fast solar wind etc. However, microwave observations.
Lyndsay Fletcher, University of Glasgow
Simulation of relativistic shocks and associated radiation from turbulent magnetic fields