|Office:||107 Peter Engel Science Center|
|Office Hour:||1 pm odd days (or by appointment or just stop by)|
|Lecture:||8:00–9:10 am Days 135 (Mods C+D)|
|Room:||319 Peter Engel Science Center|
|Textbook:||Physics of Space Plasmas by Parks|
Space Physics is the study of what goes on in the solar systems between the Sun and its satellites — the planets, moons, comets, asteroids, etc. In elementary science classes this region is often described as vacuum that contains no matter. This is an exaggeration — even though the number density of particles in most regions of the solar system is small enough to be considered a vacuum by earthbound standards, matter still exists in all regions. This matter usually exists as a plasma. Along with the plasma, many different types of waves exist in space. Much of this course will deal with the plasma and waves in space and their interactions with each other.
In some ways, Space Physics is one of the oldest branches of physics. Since before recorded history, people have been fascinated by the night sky. Much of what interested ancient people involved the stars, which would now be classified as astronomy, but some of the most striking phenomena, including most importantly the aurora borealis and australis, have their roots in Space Physics. Though Space Physics has its roots in the distant past, it did not really come into its own as a field of study until after man-made satellites were first launched into space. In-situ measurements are key to understanding the space environment and in this course we will often look at spacecraft data.
Homework will be assigned roughly once a cycle and be due roughly a cycle later.
The grade in this class will be 35 % from the total homework grade, 15 % from quizzes/participation, 17.5 % from the first test grade, and 32.5 % from the final test.
|7-1||T||3/13||1.1–1.10||Introduction||Particles, fields and structures in space|
|7-3||F||3/16||2.1–5, 2.8–9||Basic Plasma Physics||Fields and statistical mechanics|
|7-5||T||3/20||3.1–6||Fields 1||Magnetic fields in space|
|8-1||R||3/22||3.7–10||Fields 2||Electric fields in space|
|8-3||M||3/26||4.1–10||Particles 1||Equations of motion and drifts|
|8-5||W||3/28||4.11–16||Particles 2||Adiabatic invariants and trapped particles|
|9-1||F||3/30||5.1–3, 5.5–6||MHD 1||Fluids; single particle and ideal|
|9-3||T||4/03||5.9–11||MHD 2||Maxwellian MHD|
|9-5||T||4/10||1–5||Review||Review for Test 1|
|10-3||M||4/16||6.1–2, supplemental||Atmospheres||Earth’s and Sun’s atmospheres|
|10-5||W||4/18||6.4–10||Solar wind||Causes and models of the solar wind|
|11-1||F||4/20||8.1 – 5||Boundaries 1||Basic types and models|
|11-3||T||4/24||8.6–9||Boundaries 2||Applied boundaries and boundary layers|
|11-5||R||4/26||7.1–2, 7.7||Currents||Currents in space, field-aligned currents|
|12-1||M||4/30||supplemental||Aurora||Causes and structure of aurora|
|12-3||W||5/02||11.1–4, 11.6–9||Instabiliies||Instabilities in space and Space Weather|
|12-5||F||5/04||21–33.7||Review||Review for Final|