Community Continuity and Resilience Manual

The Community Continuity and Resilience Manual can be used by small organizations to make themselves more resilient. The manual provides materials for organizations to give their own continuity and resilience workshops. It includes background on continuity and resilience, a sample presentation, agendas and invites for workshops, as well as a sample continuity plan

Preparing for Storms in Louisiana: Manual for Nonreaders

The Preparing for Storms nonreader manual uses the same curriculum as the Preparing for Storms student manual, but is designed for beginning readers

Preparing for Storms in Louisiana Take Home Guide, 2nd Edition (English)

Louisiana is at risk from natural and man-made disasters. Flooding, tropical storms, and hurricanes happen. To stay safe, sometimes you and your family will need to leave home before a storm comes. People in Louisiana need to be ready for emergencies. This is your take home guide. It helps you prepare for storms

Preparing for Storms in Louisiana Take Home Guide, 2nd Edition (English/Spanish)

Louisiana is at risk from natural and man-made disasters. Flooding, tropical storms, and hurricanes happen. To stay safe, sometimes you and your family will need to leave home before a storm comes. People in Louisiana need to be ready for emergencies. This take home guide will help you get prepared

Preparing for Storms in Louisiana English/Spanish Flashcards

Louisiana is at risk from natural and man-made disasters. Flooding, tropical storms, and hurricanes happen. To stay safe, sometimes you and your family will need to leave home before a storm comes. People in Louisiana need to be ready for emergencies. These flashcards will help you get prepared

Gravity-darkening Analysis of the Misaligned Hot Jupiter MASCARA-4 b

MASCARA-4 b is a hot Jupiter in a highly misaligned orbit around a rapidly rotating A3V star that was observed for 54 days by the Transiting Exoplanet Survey Satellite (TESS). We perform two analyses of MASCARA-4 b using a stellar gravity-darkened model. First, we measure MASCARA-4 b's misaligned orbital configuration by modeling its TESS photometric light curve. We take advantage of the asymmetry in MASCARA-4 b's transit due to its host star's gravity-darkened surface to measure MASCARA-4 b's true spin–orbit angle to be 104°+7°-13°. We also detect a ~4σ secondary eclipse at 0.491 ± 0.007 orbital phase, proving that the orbit is slightly eccentric. Second, we model MASCARA-4 b's insolation including gravity darkening and find that the planet's received X-ray and ultraviolet flux varies by 4% throughout its orbit. MASCARA-4 b's short-period, polar orbit suggests that the planet likely underwent dramatic orbital evolution to end up in its present-day configuration and that it receives a varying stellar irradiance that perpetually forces the planet out of thermal equilibrium. These findings make MASCARA-4 b an excellent target for follow-up characterization to better understand the orbital evolution and present-day environment of planets around high-mass stars