## You are here

Home ›Now showing results **1-10** of **12**

This is the first module in the Solar Dynamic Observatory (SDO) Project Suite curriculum. Activities are self-directed by students or student teams using online videos and data from the SDO satellite to explore, research and build knowledge about... (View More) features of the Sun. Students build vocabulary, apply or demonstrate learning through real world connections, and creating resources to use in their investigations. Each activity comes with both a teacher and student guide with sequential instructions and embedded links to the needed videos and internet resources. Activity 1A: Structure of the Earth's Star takes students through the features and function of the Sun's structures using online videos, completing a "Sun Primer" data sheet using information from the videos, and creating a 3D origami model of the Sun. Students use a KWL chart to track what they have learned. Activity 1B: Observing the Sun has students capture real solar images from SDO data to find and record sunspots and track their movement across the surface of the Sun. Activity 1C has students create a pin-hole camera to use in calculating the actual diameter of the Sun, and then calculate scales to create a Earth-Sun scale model. Students reflect on their learning and results at the end of the module. An internet connection and access to computers are needed to complete this module. (View Less)

This is the second module in the Solar Dynamic Observatory (SDO) Project Suite curriculum. Each activity is self-directed by students or student teams and uses online videos, data from the SDO satellite and hands-on activities to explore, research... (View More) and build knowledge about how and why studying the Sun's electromagnetic energy and magnetic fields help scientists better understand the Sun's activity and space weather. Students build knowledge and vocabulary, apply or demonstrate learning through real world connections and create resources to use in investigations. Both a teacher and student guide is included with sequential instructions and embedded links to the needed videos, tutorials and internet resources. In Activity 2A: The Sun and the EM Spectrum students learn how SDO uses key parts of the Sun's electromagnetic spectrum (EMS) to research regions of the Sun, create an interactive foldable to describe the different wavebands of the EMS, then use real-time SDO image data and the Helioviewer online tool to explore the Sun's regional activity. Tutorials for using Helioviewer and making the EMS foldable are included. Activity 2B: Solar activity and Magnetism has students use information in online videos and slide presentations to demonstrate concepts of magnetism and the relationship between the Sun's variable magnetic fields and sunspots. Activity 3B: Solar Research in Action! Build a Spectroscope has students create a spectroscope to observe the different wavebands of visible light, demonstrate how the Sun emits varying EMS energies, and explain how this information helps scientists understand the composition and activity of both our nearest star, and other stars in the universe. A computer for student-teams and a connection to the Internet are needed to complete this module. (View Less)

This is an activity about solar energy. Learners will first use computers to research and learn how solar panels convert sunlight into electricity. Next, they will calculate the surface area of solar panels board a satellite and their total power... (View More) generated in various positions of the satellite, given the dimension of the panels. After, learners will organize and write a report summarizing the information about the MMS mission satellites. This activity requires student access to internet accessible computers. This is lesson four as part of the MMS Mission Educator's Instructional Guide. (View Less)

During the last sunspot cycle between 1996-2008, over 21,000 flares and 13,000 clouds of plasma exploded from the Sun's magnetically active surface. These events create space weather. Students will learn more about space weather and how it affects... (View More) Earth through reading a NASA press release and viewing a NASA eClips video segment. Then students will explore the statistics of various types of space weather storms by determining the mean, median and mode of a sample of storm events. This activity is part of the Space Math multimedia modules that integrate NASA press releases, NASA archival video, and mathematics problems targeted at specific math standards commonly encountered in middle school textbooks. The modules cover specific math topics at multiple levels of difficulty with real-world data and use the 5E instructional sequence. (View Less)

During the last sunspot cycle between 1996-2008, over 21,000 flares and 13,000 clouds of plasma exploded from the Sun's magnetically active surface. Students will learn more about space weather through reading a NASA press release and viewing a NASA... (View More) eClips video segment. Then students will explore the statistics of various types of space weather storms by determining the mean, median and mode of different samples of storm events. This activity is part of the Space Math multimedia modules that integrate NASA press releases, NASA archival video, and mathematics problems targeted at specific math standards commonly encountered in middle school textbooks. The modules cover specific math topics at multiple levels of difficulty with real-world data and use the 5E instructional sequence. (View Less)

Students will learn about the Transit of Venus through reading a NASA press release and viewing a NASA eClips video that describes several ways to observe transits. Then students will study angular measurement by learning about parallax and how... (View More) astronomers use this geometric effect to determine the distance to Venus during a Transit of Venus. This activity is part of the Space Math multimedia modules that integrate NASA press releases, NASA archival video, and mathematics problems targeted at specific math standards commonly encountered in middle school textbooks. The modules cover specific math topics at multiple levels of difficulty with real-world data and use the 5E instructional sequence. (View Less)

This is a lesson about magnetism and solar flares. Learners will evaluate real solar data and images in order to calculate the energy and magnetic strength of a solar flare moving away from the Sun as a coronal mass ejection. This is Activity 3 in... (View More) the Exploring Magnetism in Solar Flares teachers guide. (View Less)

This is an activity about the mathematics of oscillation. Using data obtained in ninth and tenth activities in the Exploring the Earth's Magnetic Field: An IMAGE Satellite Guide to the Magnetosphere educators guide, learners will plot the formula... (View More) X(t)=X(0)cos(ft) or X(t)=X(0)sin(ft), depending on the data obtained during the oscillation experiments. Then, the mathematical model for oscillation is further refined by including damping. This is the eleventh activity in the guide and requires prior use and construction of a soda bottle magnetometer. (View Less)

This is an activity about the magnetic deflection. Learners will observe and measure the deflection that an iron mass causes in a soda bottle magnetometer and plot the data. The data should show the inverse-square cube law of change in the magnetic... (View More) field. This is the twelfth activity in the guide and requires prior use and construction of a soda bottle magnetometer, as well as a six to ten pound container of iron nails (or an equivalent iron mass). (View Less)

This is an activity about satellite size. Learners will calculate the volume of the IMAGE (Imager for Magnetopause-to-Aurora Global Exploration) satellite, the first satellite mission to image the Earth's magnetosphere. They will then determine the... (View More) effect of doubling and tripling the satellite dimensions on the satellite's mass and cost. This is the first activity in the Solar Storms and You: Exploring Satellite Design educator guide. (View Less)