Solar flares, which have significant space weather consequences, are
natural particle accelerators and one of the most spectacular phenomena
of solar activity. RHESSI is the most advanced solar X-ray and gamma-ray
mission ever flown and has opened a new era in solar flare research
following its launch in 2002. This book offers a glimpse of this active
research area from a high-energy perspective and contains a
comprehensive guideline for RHESSI data analysis. Its main theme is the
investigation of particle acceleration and transport in solar flares.
The strength of this book lies in its well-balanced account of the
latest X-ray observations and theoretical models. The observational
focus is on the morphology and spectra of imaged X-ray sources produced
by nonthermal electrons or hot plasma. The modeling takes the novel
approach of combining the Fokker-Planck treatment of the accelerated
particles with the hydro-dynamic treatment of the heated atmosphere.
Applications of this modeling technique reach beyond the Sun to other
exotic environ-ments in the universe, such as extrasolar planetary
auroras, stellar flares, and flares on accretion disks around neutron
stars and black holes.