Space Physics – Physics of the space environment

• estimate the density and pressure in the upper atmosphere from basic principles
• derive basic equations describing formation of the ionosphere
• calculate the motion of charged particles in the Earth’s magnetosphere, including the radiation belts
• perform simple calculations of solar wind and interplanetary magnetic field propagation
• describe and estimate effects of the solar wind on planetary environment
• explain the distribution of plasma and electric currents in the Earth’s environment, the plasmasphere and magnetosphere
• use and exploit wellknown theoretical and empirical models for the space environment
• analyze satellite data of solar winds that interact with the Earth’s magnetosphere.

Single-particle motion in magnetic and electric fields. MHD theory application to space. Structure and dynamics of the upper atmosphere. Ionospheric formation and structure. Wave propagation in plasma. Solar activity and solar wind. Solar wind planetary interactions. Magnetospheric structure and dynamics. Plasmasphere, aurora and radiation belts.

• 36 – 49 (Mon 13-17)

10033/10034/30400/31400/10036/02631/02632/02633

Lectures, exercise calculations, and model and data exercises.

Maximum: 20.

Please be aware that this course has a limited number of seats available. If there are too many applicants, a pool will be created for the remainder of the qualified applicants, and they will be selected at random. You will be informed 8 days before the start of the course, whether you have been allocated a spot.