![]() Students use two images from the Solar Dynamics Observatory to estimate the speed of the X-class solar flare on March 6, 2012. Problem 467: Estimating Magnetic Field Speeds on the Sun ![]() Sunspot cycle to estimate the time between X-class flares during the current sunspot cycle Students use simple statistics to determine the solar flare frequency during a Problem 468: How Common are X-Class Solar Flares? Students estimate the speed of plasma streamers near the solar surface using images from a Solar Dynamics Observatory. Problem 505: SDO Sees Coronal Rain - Estimating Plasma Speeds ![]() Students work with simple averaging and explore the latest sunspot cycle to find their averages for 20. Problem 514: Solar Flares and the Stormy Sun Students work with simple proportions to estimate the diameter of the sun using the Moon and the Moon's distance. Problem 516: Hinode Observes a Solar Eclipse from Space Students use an image from IRIS to examine the sizes and equivalent energy of bright regions in the solar transition region. Problem 556:IRIS Explores the Solar Transition Region To find the missing words in a short essay about solar storms. Students solve 10 problems using positive and negative numbers, addition, subtraction and multiplication A series of Appendices reveal the imagery and history through news paper articles of the Transits of Venus observed during the 17s. Students explore astronomical eclipses, transits and occultations to learn about their unique geometry, and how modern observations by NASA's Kepler Satellite will use transit math to discover Six appendices and an extensive provide a rich 150-year context for why space whether is an important issue. Students explore the way in which the sun interacts with Earth to produce space weather, and the ways in whichĪstronomers study solar storms to predict when adverse conditions may pose a hazard for satellites and human ![]() The various ways that astronomers image the universe across the electromagnetic spectrum to learn moreĪbout the properties of matter and its movement. Properties of waves, wavelength, frequency, the Doppler shift, and Students explore the simple mathematics behind light and other forms of electromagnetic energy including the To investigating solar magnetism, the sunspot cycle, and solar storms using algebra and geometry. Problems range from calculating the sizes of sunspots from photographs, The activities explore solar storms and solar structure using simple math activities. This book features problems about the sun from many NASA science missions. ![]()
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