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The energy budget for X-ray to infrared reprocessing in Compton-thin and Compton-thick active galaxies
The energy budget X-ray Compton-thin
2011/1/13
Heavily obscured active galactic nuclei (AGNs) play an important role in contributing to the cosmic X-ray background (CXRB). However, the AGNs found in deep X-ray surveys are often too weak to allow d...
UV Diagnostics for the Energy Budget of Flares and CMEs
Sun corona flares coronal mass ejections
2010/9/16
Solar flares and coronal mass ejections convert large amounts of magnetic free energy into thermal, kinetic and potential energies, and into energy of non-thermal particles. The partitioning among the...
UV Diagnostics for the Energy Budget of Flares and CMEs
Sun: corona flares coronal mass ejections
2009/5/6
Solar flares and coronal mass ejections convert large amounts
of magnetic free energy into thermal, kinetic and potential energies, and
into energy of non-thermal particles. The partitioning among t...