We have investigated the temperature, pressure, and field dependence o
f the spin density wave (SDW) transition in the organic superconductor
(TMTSF)(2)PF6 and derived parameters for this transition. The SDW can
be characterized by the degree to which the two Fermi surfaces couple
or ''nest'' as measured by the imperfect nesting banawidth t'(b). Per
fect nesting (maximum T-SDW) occurs for t'(b) = 0, and increasing pres
sure increases t'(b) and suppresses T-SDW to 0 K at a critical value t
'(b). The increase of T-SDW with field has been shown to be orbitally
driven, and the field dependence is nearly quadratic for fields in th
e c direction. We have made quantitative observations of the field dep
endence of T-SDW at ambient pressure to 29 T and under hydrostatic pre
ssure to 8 T. From our measurements at ambient pressure we are able to
extract t'(b) and t'(b) using mean field theory and observe T-SDW =
12.1+/-0.1 K, t'(b) = 4.5+/-0.3 K, and t'(b) = 11.3+/-0.2 K. Under a
hydrostatic pressure of 5.2+/-0.2 kbar, t'(b) increases to 11.0+/-0.3
K with T-SDW decreasing to 3.3+/-0.1 K. The high pressure results are
consistent with the value of t'(b) from the ambient pressure measurem
ents. We also observe no dependence of T-SDW with field in the a or b
directions, in contrast to previous results.