  We present the results from observing nine Galactic novae in eruption with
the Solar Mass Ejection Imager (SMEI) between 2004 and 2009. While many of
these novae reached peak magnitudes that were either at or approaching the
detection limits of SMEI, we were still able to produce light curves that in
many cases contained more data at and around the initial rise, peak, and
decline than those found in other variable star catalogs. For each nova, we
obtained a peak time, maximum magnitude, and for several an estimate of the
decline time (t2). Interestingly, although of lower quality than those found in
Hounsell et al. (2010a), two of the light curves may indicate the presence of a
pre-maximum halt. In addition the high cadence of the SMEI instrument has
allowed the detection of low amplitude variations in at least one of the nova
light curves.
