Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations –...

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Loose ends and Loose ends and Magnetic Fields in Astronomy Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter - astronomical applications

Transcript of Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations –...

Page 1: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

Loose ends and Loose ends and Magnetic Fields in AstronomyMagnetic Fields in Astronomy

- Exam tips – come to class!- Course Evaluations – come to class!

- energy in fields- magnetism in matter- astronomical applications

Page 2: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

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 1 o oc μ ε

221

2 2B E oo

Bu u ε E

μ

Page 3: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

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

Page 4: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

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 εoE2

max = B2max / 2μo

Page 5: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

Where does magnetism come from ????

Recall these equations:

I=Q/t

T=2πr/v

L=mvr

μ=IA (sub in the above, and A=πr2)

Imagine a little circuit with an electron moving at a distancer from the nucleus of an atom. Combining these, we can show that: L

m

e

2 This is the magnetic moment of an

electron

Page 6: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

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 :

m

e

2

Q: So, if all electrons have this unit of magnetic moment, why are not all substances magnetic ???

....3,2,,0

Page 7: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

EM in Astronomy

Page 8: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

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

Page 9: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

This is the spiral

galaxy M51 and its

magnetic field.

Studying the fields

helps us understand

how galaxies form and

evolve.

Page 10: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

This is the jet of M87,

evidence for a super

massive black hole at

the center of this

galaxy.

Page 11: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

Sunspots are caused by

strong magnetic fields on

the surface of the sun.

We can detect them on other

stars currently!

Page 12: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

A supercomputer

simulation of the

reversal of earth’s

magnetic field

The earth’s magnetic field.

Page 13: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

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

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

Page 14: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

Redshift of EM waves

Page 15: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

Galaxy distribution

Page 16: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.
Page 17: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

Large Scale GalaxyDistribution

Page 18: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

Computer simulations of large scale structure formation

Page 19: Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.

HDF and earlygalaxy formation