
Announcements l Help room hours (1248 BPS) LON-CAPA #7 due Oct. 25
... l All electromagnetic waves travel through vacuum with a speed c (3 X 108 m/s) l For all EM waves, c=λf (true for any type of wave) l λ = c/f l The visible portion of the spectrum forms a tiny portion of the total EM spectrum ...
... l All electromagnetic waves travel through vacuum with a speed c (3 X 108 m/s) l For all EM waves, c=λf (true for any type of wave) l λ = c/f l The visible portion of the spectrum forms a tiny portion of the total EM spectrum ...
Magnetic Fields
... 1) An alpha particle travels at a velocity v of magnitude 550 m/s through a uniform magnetic field B of magnitude 0.045 T. The angle between v and B is 52°. What are the magnitudes of: a) The force FB acting on the particle due to B b) The acceleration of the particle. c) Does the speed of the parti ...
... 1) An alpha particle travels at a velocity v of magnitude 550 m/s through a uniform magnetic field B of magnitude 0.045 T. The angle between v and B is 52°. What are the magnitudes of: a) The force FB acting on the particle due to B b) The acceleration of the particle. c) Does the speed of the parti ...
N - PembyPhysics
... induced in the metal by the changing magnetic field. These currents produce an undesirable by-product—heat in the iron. Energy loss in a transformer can be reduced by using thinner laminations, very “soft” (low-carbon) iron and wire with a larger cross section, or by winding the primary and secondar ...
... induced in the metal by the changing magnetic field. These currents produce an undesirable by-product—heat in the iron. Energy loss in a transformer can be reduced by using thinner laminations, very “soft” (low-carbon) iron and wire with a larger cross section, or by winding the primary and secondar ...
magnetic - Timber Ridge Elementary
... other. They always need to be opposite poles to be attracted. The magnetic force pulls them together. ...
... other. They always need to be opposite poles to be attracted. The magnetic force pulls them together. ...
Document
... CT –1 Cosmic rays (atomic nuclei stripped bare of their electrons) which come from all directions, would continuously bombard Earth’s surface if most of them were not deflected by Earth’s magnetic field. Given that Earth is, to an excellent approximation, a magnetic dipole, the intensity of cosmic ...
... CT –1 Cosmic rays (atomic nuclei stripped bare of their electrons) which come from all directions, would continuously bombard Earth’s surface if most of them were not deflected by Earth’s magnetic field. Given that Earth is, to an excellent approximation, a magnetic dipole, the intensity of cosmic ...
Master Notes
... Can you come up with some more? We all have some idea of what magnet is; as you can see from the examples, we use them in many different applications. They are useful instruments in our day to day life, but it is one thing to know what a magnet is, it is another to understand how they work. What exa ...
... Can you come up with some more? We all have some idea of what magnet is; as you can see from the examples, we use them in many different applications. They are useful instruments in our day to day life, but it is one thing to know what a magnet is, it is another to understand how they work. What exa ...
Phys2102 Spring 2002
... and Morley looked and looked, and decided it wasn’t there. How do waves travel??? Electricity and magnetism are “relative”: Whether charges move or not depends on which frame we use… This was how Einstein began thinking about his “theory of special relativity”… We’ll leave that theory for later. ...
... and Morley looked and looked, and decided it wasn’t there. How do waves travel??? Electricity and magnetism are “relative”: Whether charges move or not depends on which frame we use… This was how Einstein began thinking about his “theory of special relativity”… We’ll leave that theory for later. ...
The Earth`s Interior
... • S-wave shadow zone: the region on the earth’s surface (at any distance more than 103o from an earthquake epicenter) in which S waves from the earthquake are absent • The S-wave shadow zone seems to indicate that S waves do not travel through the core at all, if this is true, it implies that the co ...
... • S-wave shadow zone: the region on the earth’s surface (at any distance more than 103o from an earthquake epicenter) in which S waves from the earthquake are absent • The S-wave shadow zone seems to indicate that S waves do not travel through the core at all, if this is true, it implies that the co ...
Aurora

An aurora is a natural light display in the sky, predominantly seen in the high latitude (Arctic and Antarctic) regions. Auroras are produced when the magnetosphere is sufficiently disturbed by the solar wind that the trajectories of charged particles in both solar wind and magnetospheric plasma, mainly in the form of electrons and protons, precipitate them into the upper atmosphere (thermosphere/exosphere), where their energy is lost. The resulting ionization and excitation of atmospheric constituents emits light of varying colour and complexity. The form of the aurora, occurring within bands around both polar regions, is also dependent on the amount of acceleration imparted to the precipitating particles. Precipitating protons generally produce optical emissions as incident hydrogen atoms after gaining electrons from the atmosphere. Proton auroras are usually observed at lower latitudes. Different aspects of an aurora are elaborated in various sections below.