
A glowing 3D butterfly curve is traced by the Lorenz equations. Students change sigma, rho and beta and compare two nearly identical starts to see how fast they diverge.
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Edward Lorenz found these three equations in 1963 while cutting a weather model down to its bones. Nothing in them is random, and nothing is approximate: give the same three starting numbers twice and you get the same path twice, forever. Yet change the eighth decimal place of one of them and within about twenty time units the two paths are on opposite wings of the butterfly. That is sensitive dependence on initial conditions, and it is a property of the equations, not a flaw in the computer. It also has an off switch: the wing centres sit at ±sqrt(beta(rho - 1)) and stay stable until rho passes sigma(sigma + beta + 3)/(sigma - beta - 1), which for Lorenz's own numbers is 470/19, about 24.74. Below that, both twins settle on the same point and the future is perfectly predictable. Above it there is nowhere left to settle. (Strictly, a strange attractor already coexists with those stable points from about rho = 24.06, so in the narrow window between the two values the ending depends on where you start.) Students can change how fast x chases y and how hard it is driven and compare what happens. Use it for math inquiry with High School on a projector or student device.
ស្តង់ដារ៖ Common Core CCSS.MATH.CONTENT.HSF.IF.B.4
Yes. Open the Lorenz Attractor simulation in a modern browser with no download or sign-up required.
The simulation includes learning-level presets spanning High School. Choose the level that matches your class, then use it on a projector or student devices.
ដាក់វាចូលទៅក្នុង LMS ប្លក់ ឬគេហទំព័រថ្នាក់រៀនរបស់អ្នក — ឥតគិតថ្លៃ។
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A glowing 3D butterfly curve is traced by the Lorenz equations. Students change sigma, rho and beta and compare two nearly identical starts to see how fast they diverge.
Type any function and see its shape straight away. Plot up to three at once in three colours to compare them, drag the trace point to read a value off a curve, and see where each one crosses zero.
Spin a spinner, flip a coin or roll a die and watch two sets of bars: the chances the shapes predict, and the results you actually got. Ten spins prove nothing; a few hundred and the two are hard to tell apart.
Move m and watch the line tilt; move b and watch it slide. Or drag the two points on the line and read the equation it writes back. A rise-over-run staircase climbs the line so slope becomes something you can count.
Compare a two-body orbit with three-body figure-eight motion, then add up to twelve bodies. Change initial masses, velocities and positions; watch orbit trails and numerical energy error.
ទីតាំងការងារសម្រាប់គ្រូដោយឥតគិតថ្លៃ KiwiBee នាំមកនូវការរៀបចំមេរៀន សន្លឹកកិច្ចការ ឧបករណ៍ក្នុងថ្នាក់ និងសៀវភៅពិន្ទុ ទាំងអស់នៅកន្លែងតែមួយ។
ចាប់ផ្តើមឥតគិតថ្លៃ និងបង្កើតថ្នាក់ដំបូងរបស់អ្នក