  The presence of aerosols in an exoplanet atmosphere can veil the underlying
material and can lead to a flat transmission spectrum during primary transit
observations. In this work, we explore forward scattering effects from
super-micron sized aerosol particles present in the atmosphere of a transiting
exoplanet. We find that the impacts of forward scattering from larger aerosols
can significantly impact exoplanet transits and the strength of these effects
can be dependent on wavelength. In certain cloud configurations, the
forward-scattered light can effectively pass through the clouds unhindered,
thus rendering the clouds transparent. The dependence of the aerosol scattering
properties on wavelength can then lead to a positive slope in the transit
spectrum. These slopes are characteristically different from both Rayleigh and
aerosol absorption slopes. As examples, we demonstrate scattering effects for
both a rocky world and a hot Jupiter. In these models, the predicted spectral
slopes due to forward scattering effects can manifest in the transit spectrum
at the level of $\sim$10s to $\sim$100s of parts per million and, hence, could
be observable with NASA's James Webb Space Telescope.
