This paper presents a comparison between measurements of the spectral radiant intensity of
Magnesium/Teflon®/Viton® (MTV) flares and theoretical estimation using available mathematical models in the range
of 0.6 μm up to 11.5 μm. It is used an indigenous system capable of hold the flare pellets in the same position during the
burning time and reproduce the airflow after an actual air launching at different velocities. Two mathematical models are
studied and adapted to predict MVT flare radiant intensity and average emissivity from visible to long wavelength
infrared. The results indicate that the adapted models can be use to estimate the MTV flare parameters in different
situations with good accuracy.
Access to the requested content is limited to institutions that have purchased or subscribe to SPIE eBooks.
You are receiving this notice because your organization may not have SPIE eBooks access.*
*Shibboleth/Open Athens users─please
sign in
to access your institution's subscriptions.
To obtain this item, you may purchase the complete book in print or electronic format on
SPIE.org.
INSTITUTIONAL Select your institution to access the SPIE Digital Library.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.