Moyo Vol. I N 1

JDB, Greek to Me . 1. Hood, Richard. Hood Advocates Off-Campus Living . 3. Rinehart, Dawn. Beta Press Biggio on Plan B . 10. Boyden, Ode on a Grecian Turn: An Interview with President Michele T. Myers . 6. Rogers, Kirstin. The Social Auction . 11. Bosari, David. Bosari on Brotherhood . 13. Mason, Amy. A Pledge in a Sea of Screaming Girls . 13. Kruse, Kristina. Kruse, Urges Thinking Hard . 14. O\u27Hare, Kimberly. Never Uncertain . 15. Howard, Tressie. D.U.\u27s New Face from Bucknell . 15. Pryor, Derrick. AΦA: A Fraternity of a Different Color . 16. Norpell, Bradley F. The Year of 1950: Looking Back on Fraternity Life . 18. Rogers, Kirstin. Freshman Lambert Co-Authors Book . 19. Bergstrom, Ida. Defending the System . 20. Bristow, Vernall. Meding D.U.\u27s Broken Reputation . 20

Exoplanet Diversity in the Era of Space-based Direct Imaging Missions

This whitepaper discusses the diversity of exoplanets that could be detected by future observations, so that comparative exoplanetology can be performed in the upcoming era of large space-based flagship missions. The primary focus will be on characterizing Earth-like worlds around Sun-like stars. However, we will also be able to characterize companion planets in the system simultaneously. This will not only provide a contextual picture with regards to our Solar system, but also presents a unique opportunity to observe size dependent planetary atmospheres at different orbital distances. We propose a preliminary scheme based on chemical behavior of gases and condensates in a planet's atmosphere that classifies them with respect to planetary radius and incident stellar flux.Comment: A white paper submitted to the National Academy of Sciences Exoplanet Science Strateg

Chief PooPaw\u27s Teepee

This is a color image of Chief Poopaw\u27s Teepee. This image is part of the Maine Folklife Center Collection of the University of Maine.https://digitalcommons.library.umaine.edu/penobscotimages/1009/thumbnail.jp

Bank of Indian Island with Teepees

This is a black and white image of the bank of Indian Island with teepees and buildings in the background. This image is part of the Maine Folklife Center Collection of the University of Maine.https://digitalcommons.library.umaine.edu/penobscotimages/1010/thumbnail.jp

Chief Poolaw Statue with Totems

This is a color image of an Indian statue with totem poles and a sign that reads Chief Poolaw\u27s Teepee--1959 . This image is part of the Maine Folklife Center Collection of the University of Maine.https://digitalcommons.library.umaine.edu/penobscotimages/1008/thumbnail.jp

A Benthic Terrain Classification Scheme for American Samoa

Coral reef ecosystems, the most varied on earth, continually face destruction from anthropogenic and natural threats. The U.S. Coral Reef Task Force seeks to characterize and map priority coral reef ecosystems in the U.S./Trust Territories by 2009. Building upon NOAA Biogeography shallow-water classifications based on Ikonos imagery, presented here are new methods, based on acoustic data, for classifying benthic terrain below 30 m, around Tutuila, American Samoa. The result is a new classification scheme for American Samoa that extends and improves the NOAA Biogeography scheme, which, although developed for Pacific island nations and territories, is only applicable to a maximum depth of 30 m, due to the limitations of satellite imagery. The scheme may be suitable for developing habitat maps pinpointing high biodiversity around coral reefs throughout the western Pacific

Exoplanet Diversity in the Era of Space-based Direct Imaging Missions

This whitepaper discusses the diversity of exoplanets that could be detected by future observations, so that comparative exoplanetology can be performed in the upcoming era of large space-based flagship missions. The primary focus will be on characterizing Earth-like worlds around Sun-like stars. However, we will also be able to characterize companion planets in the system simultaneously. This will not only provide a contextual picture with regards to our Solar system, but also presents a unique opportunity to observe size dependent planetary atmospheres at different orbital distances. We propose a preliminary scheme based on chemical behavior of gases and condensates in a planet's atmosphere that classifies them with respect to planetary radius and incident stellar flux