Sustaining enterprise education
This presentation examines the impact of enterprise education on the career aspiration, decisions and intentions of HE students
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The Holloway Series in Poetry: Aaron Kunin
A rising star in the poetry world, Kunin is also a literary critic and a novelist. His formally innovative work has been described as "tragicomic," and it is with a certain thrill that one realizes his poems have managed to bundle shame with hilarity, high tension with the highly ridiculous, sharp wit with ominous portents. His first book, Folding Ruler Star (Fence Books, 2005), was devised as a "value-neutral Paradise Lost" in which the structures of belief, shame, and hierarchy are explored b
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Minerals, Crystals, and Gems: Stepping Stones to Inquiry
This site introduces students to mineral science and the scientific process -- observing things, forming hypotheses, and drawing conclusions. Students watch crystals grow, go on a scavenger hunt for minerals, and create a classroom exhibit of rocks and minerals (for Grades 3-8).
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Geologic Time: The Story of a Changing Earth
This site examines the history of Earth. Learn about the formation of Earth, dating the age of rocks, geologic time, plate tectonics, climate change, ocean circulation, evolution, extinction, ecology, and topics related to paleobiology.
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The Star-Spangled Banner
Students will be able to cite the origins and outcome of the War of 1812 and be able to place the creation of the Star-Spangled Banner in a chronological framework.
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The Home Energy Saver
The Home Energy Saver is designed to help consumers identify the best ways to save energy in their homes, and find the resources to make the savings happen. The Home Energy Saver was the first Internet-based tool for calculating energy use in residential buildings. The project is sponsored by the U.S. Department of Energy (DOE), as part of the national ENERGY STAR Program for improving energy efficiency in homes, with previous support from the U.S. Environmental Protection Agency (EPA), the US D
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Stratigraphic Framework of Lower and Upper Cretaceous Rocks in Central and Eastern Montana
This USGS report focuses on Cretaceous rocks in Montana with respect to natural gas and coalbed methane. The study includes the stratigraphy from the top of the Mowry Shale to the base of the Judith River Formation. The project integrates geologic, structural, hydrologic and engineering studies with known and new geochemical data on the gas and co-produced water. The report also facilitates an understanding of the controls on the spatial distribution of potential gas accumulations. Figures, tabl
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002 - regula 7 - Latinae Grammatices Syntaxis
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Exploring Earth: Investigations
This site provides more than 75 earth science investigations. Each presents photos and text (and sometimes video) that help students understand key earth science concepts. Among the topics: earth's layers, rocks, volcanoes and plate tectonics, earthquakes and mountains, surface and ground water, wind and currents, atmosphere and weather, climate change, oceans, our moon and solar system, and earth's history.
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Analogue Microstructural Modeling at the University at Albany, SUNY
This site contains 15 time-lapse QuickTime movies that show the experimental deformation behavior of octachloropropane. This compound shows similar microstructures to those found in quartzite, and thus is a nice analog for the deformation of rocks. The movies illustrate cataclastic deformation, grain boundary opening, formation of subgrains, subgrain boundary formation and grain boundary migration, ribbon formation, grain growth at zero strain rate, and grain boundary migration during high tempe
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The Image Gallery: Rocks
This website offers an extensive, annotated list of photographs of rock types. Some of the photographs are of hand samples, others are of rocks in the field. Users can also follow links to image galleries of fossils, landforms, minerals, geologic features and processes, and geology and cultures.
Author(s): Andrew Aldren

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Physical Geography
Physical geography is the study of the earth's dynamic systems -- its air, water, weather climate, landforms, rocks, soils, plants, ecosystems and biomes -- and how humans interact with the earth's systems. Physical geography is the study of the world around you. Everyone, every day, interacts with the earth's dynamic systems. I challenge you to join me on an exploration of the complex, and exciting world in which you live! This is a freshman level college course in physical geography. It requir
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Introduction to Psychology
What do your dreams mean? Do men and women differ in the nature and intensity of their sexual desires? Can apes learn sign language? Why can’t we tickle ourselves? This course tries to answer these questions and many others, providing a comprehensive overview of the scientific study of thought and behavior. It explores topics such as perception, communication, learning, memory, decision-making, religion, persuasion, love, lust, hunger, art, fiction, and dreams. We will look at how these aspect
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All You Need Is (the Summer of) Love - Creating an Exhibit that Compares 1960s and Contemporary Cult
In this lesson, students explore various aspects of the 1960s, including the 1967 "Summer of Love," and compare them with contemporary times to ascertain cultural influences.
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Rayleigh-Taylor Instabilities in Supernovae Explosions: Hydrogen Mass Fraction
The following calculation shows the development and evolution of Rayleigh-Taylor instabilities which develop behind the supernova blast wave on a time scale of a few hours. The initial model was chosen to provide a good representation for the progenitor star for Supernova 1987A. The calculation was performed using the Piecewise-Parabolic Method for hydrodynamics on a two-dimensional spherical grid with rotational symmetry about the vertical axis and equatorial symmetry about the horizontal axis.
Author(s): Bruce Fryxell,Dave Arnett,Ewald Muller,Pamela ONei

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Rayleigh-Taylor Instabilities in Supernovae Explosions: Oxygen Mass Fraction
The following calculation shows the development and evolution of Rayleigh-Taylor instabilities which develop behind the supernova blast wave on a time scale of a few hours. The initial model was chosen to provide a good representation for the progenitor star for Supernova 1987A. The calculation was performed using the Piecewise-Parabolic Method for hydrodynamics on a two-dimensional spherical grid with rotational symmetry about the vertical axis and equatorial symmetry about the horizontal axis.
Author(s): Bruce Fryxell,Dave Arnett,Ewald Muller,Pamela ONei

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Rayleigh-Taylor Instabilities in Supernovae Explosions: Partial Density of Helium
The following calculation shows the development and evolution of Rayleigh-Taylor instabilities which develop behind the supernova blast wave on a time scale of a few hours. The initial model was chosen to provide a good representation for the progenitor star for Supernova 1987A. The calculation was ...
Author(s): Pamela ONeil,Bruce Fryxell,Ewald Muller,Dave Arnet

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Stellar Wind Disruption by an Orbiting Neutron Star: High X-Ray Luminosity
A tiny neutron star orbits incessantly around a massive star with a diameter a million times larger than its own. The high luminosity of the massive star drives a strong wind from its surface. The neutron star crashes through this wind at over 300 kilometers per second. The gravity and X-ray luminosity of the neutron star act to disrupt the wind, producing an extended wake of dense gas trailing behind the neutron star. This simulation, in the reference frame of the neutron star, shows conditions
Author(s): Alan McConnell,Bruce Fryxell,Ian Stevens,John Blon

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Stellar Wind Disruption by an Orbiting Neutron Star: Low X-Ray Luminosity
A tiny neutron star orbits incessantly around a massive star with a diameter a million times larger than its own. The high luminosity of the massive star drives a strong wind from its surface. The neutron star crashes through this wind at over 300 kilometers per second. The gravity and X-ray luminosity of the neutron star act to disrupt the wind, producing an extended wake of dense gas trailing behind the neutron star. This simulation, in the reference frame of the neutron star, shows conditions
Author(s): Alan McConnell,Bruce Fryxell,Ian Stevens,John Blon

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Stellar Wind Disruption by an Orbiting Neutron Star: Neutron Star Close-up
A tiny neutron star orbits incessantly around a massive star with a diameter a million times larger than its own. The high luminosity of the massive star drives a strong wind from its surface. The neutron star crashes through this wind at over 300 kilometers per second. The gravity and X-ray luminosity ...
Author(s): Alan McConnell,John Blondin,Ian Stevens,Tim Kallma

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