loose ends and magnetic fields in astronomy
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Loose ends and Magnetic Fields in Astronomy. Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter - astronomical applications. Energy Density in EM Waves. The energy density, u , is the energy per unit volume

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loose ends and magnetic fields in astronomy
Loose ends and Magnetic Fields in Astronomy
  • Exam tips – come to class!- Course Evaluations – come to class!- energy in fields- magnetism in matter
  • - astronomical applications
energy density in em waves
Energy Density in EM Waves
  • The energy density, u, is the energy per unit volume
  • For the electric field, uE= ½ εoE2
  • For the magnetic field, uB = ½ μoB2
  • Since B = E/c and
energy density
Energy Density
  • The instantaneous energy density associated with the magnetic field of an EM wave equals the instantaneous energy density associated with the electric field
    • In a given volume, the energy is shared equally by the two fields
energy density1
Energy Density
  • The total instantaneous energy density is the sum of the energy densities associated with each field
    • u =uE + uB = εoE2 = B2 / μo
  • When this is averaged over one or more cycles, the total average becomes
    • uav = εo(E2)av = ½ εoE2max = B2max / 2μo
slide5

Where does magnetism come from ????

Recall these equations:I=Q/t

T=2πr/vL=mvrμ=IA (sub in the above, and A=πr2)Imagine a little circuit with an electron moving at a distance

r from the nucleus of an atom. Combining these, we can

show that:

This is the magnetic moment of anelectron

slide6

Where does magnetism come from ????

Now, because the angular momentum L for electrons isquantized, L=The smallest possible non-zero value of the magnetic

moment is :

Q: So, if all electrons have this unit of magnetic moment,

why are not all substances magnetic ???

slide8

Magnetic fields ‘rotate’ an electromagnetic wave. This is called Faraday Rotation, and it allows us to measure the magnetic field of interstellar space.

slide9
This is the spiral

galaxy M51 and its

magnetic field.

Studying the fields

helps us understand

how galaxies form and

evolve.

slide10
This is the jet of M87,

evidence for a super

massive black hole at

the center of this

galaxy.

slide11
Sunspots are caused by

strong magnetic fields on

the surface of the sun.

We can detect them on other

stars currently!

slide12
A supercomputer

simulation of the

reversal of earth’s

magnetic field

The earth’s magnetic field.

slide13
Planetary formation needs to incorporate magnetic fields in the ‘protoplanetary’ disc.

These are called MHD (magneto-hydro-dynamics simulations.

slide17

Large Scale Galaxy

Distribution

slide19

HDF and early

galaxy formation

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