Interplanetary diffusive shock acceleration: Exponential or power-law spectra?

Details Interplanetary diffusive shock acceleration: Exponential or power-law spectra? Interplanetary diffusive shock acceleration: Exponential or power-law spectra?

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..157..349s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 157, no. 1-2, p. 349-366

Computer Science

Numerical Analysis

7

Interplanetary Medium, Particle Acceleration, Particle Diffusion, Shock Fronts, Solar Physics, Sun, Diffusion Coefficient, Diffusion Theory, Exponential Functions, Matrices (Mathematics), Numerical Analysis, Power Series, Solar Wind, Transport Theory

Scientific paper

A new method for solving the transport equation and boundary condition describing diffusive shock acceleration for inter- planetary corotating interaction regions (CIRs) is provided. It involves inverting a quindiagonal matrix. Application of this method to realistic parameters indicates that the parallel diffusion coefficient magnitude is critical in determining whether observed particle distribution functions are exponential or power law.

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