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researcher

S. O'Sullivan

4 papers hereh-index 12626 citations43 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author1
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4

identity via Semantic Scholar / OpenAlex

activity
20052008
most citedThe transport of cosmic rays in self-excited magnetic turbulence

91 citations · 182 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph2008★ 21 cited

Environmental limits on the non-resonant cosmic-ray current-driven instability

B. Reville, J. G. Kirk, P. Duffy +1

We investigate the so-called non-resonant cosmic-ray streaming instability, first discussed by Bell (2004). The extent to which thermal damping and ion-neutral collisions reduce th…

astro-ph2008★ 91 cited

The transport of cosmic rays in self-excited magnetic turbulence

B. Reville, S. O'Sullivan, P. Duffy +1

The process of diffusive shock acceleration relies on the efficacy with which hydromagnetic waves can scatter charged particles in the precursor of a shock. The growth of self-gene…

astro-ph2007★ 70 cited

A cosmic ray current driven instability in partially ionised media

B. Reville, J. G. Kirk, P. Duffy +1

We investigate the growth of hydromagnetic waves driven by streaming cosmic rays in the precursor environment of a supernova remnant shock. It is known that transverse waves propag…

astro-ph2005

An explicit scheme for multifluid magnetohydrodynamics

Stephen O'Sullivan, Turlough P. Downes

When modeling astrophysical fluid flows, it is often appropriate to discard the canonical magnetohydrodynamic approximation thereby freeing the magnetic field to diffuse with respe…

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