Nerds on Wall Street: Math, Machines and Wired Markets
An intriguing look at how technology is changing financial markets, from an innovator on the frontlines of this revolution Nerds on Wall Street tells the tale of the ongoing technological transformation of the world's financial markets. The impact of technology on investing is profound, and author David Leinweber provides readers with an overview of where we were just a few short years ago, and where we are going.
Each unit of the Student's Book is divided into 3 manageable steps with clear aims and outcomes. Students can see quick results through regular 'Use what you know' sections at the end of each step. 'Life and culture' sections provide rich reading material while stimulating students' imaginations. There is a variety of exercises where students can work to their own level, making the course ideal for mixed ability classes.
This is a 6 level series of readers for children learning English, bringing together a variety of enjoyable fiction and non-fiction titles. The series provides reinforcement of the basic structures and vocabulary contained in most major primary courses. Activities and a picture dictionary or wordlist at the back of each reader.
Dear user! Your publication has been rejected as it seems to be a duplicate of another publication that already exists on Englishtips. Please make sure you always check BEFORE submitting your publication. If you only have an alternative link for an existing publication, please add it using the special field for alternative links in that publication.
Thank you!
Oscar Mandel, Professor of literature at the California Institute of Technology, is the author of numerous acclaimed books of poetry, drama, essays, fiction, literary criticism, translation, and art history.
The magnetic field of the Sun is the underlying cause of the many diverse phenomena combined under the heading of solar activity. Here we describe the magnetic field as it threads its way from the bottom of the convection zone, where it is built up by the solar dynamo, to the solar surface, where it manifests itself in the form of sunspots and faculae, and beyond into the outer solar atmosphere and, finally, into the heliosphere.
