We report here preliminary results of a mission analysis fur a space weathe
r monitoring system that provides continuous transmission of solar wind con
ditions 0.10 A.U. upstream from Earth. The system is based on four platform
s that are phased into eccentric heliocentric orbits but, from the perspect
ive of a fixed Sun-Earth line, the spacecraft appear to orbit Earth. This s
ystem offers a 10x improvement in reporting solar wind plasma and magnetic
field characteristics beyond similar platforms located at the Lagrangian L-
1 point. We describe launch and energy considerations, along with a prelimi
nary analysis of communication requirements. The Space Weather Diamond offe
rs significant potential for scientific insight into problems requiring coo
rdinated observations from multiple vantage points by providing the ability
to separate spatial from temporal variations. We discuss examples for payl
oads including both in situ and remote sensing instrumentation. (C) 2000 El
sevier Science Ltd. All rights reserved.