Detecting the Earth's magnetic field

AI Thread Summary
A solar storm detector could effectively capture fluctuations in the Earth's magnetic field caused by solar wind interactions. The Earth's magnetic field experiences compression on the sun-facing side and extension on the opposite side, which can lead to detectable variations. Continuous monitoring over weeks may reveal daily changes in magnetic field strength, influenced by ionospheric currents. Typical daily variations are around 25 nanoteslas, with short-term fluctuations of about 1 nanotesla. This project could yield interesting insights into the dynamic nature of the Earth's magnetic environment.
Steel_Panther
Messages
2
Reaction score
0
Hi guys just a quick question.

I was thinking of building a fairly simple solar storm detector, something similar to this
http://aurorawatch.lancs.ac.uk/detectors/compass

I was just wondering if the effects that the solar wind has on the shape of the Earth's magnetic field, such as the compression it experiences on the side facing the sun and the extension on the opposite side, could be detectable.

I was thinking of running the detector continuously for a couple of weeks to try to detect small fluctuations in the Earth's magnetic field, and then compare the captured data for the day and night.

Thanks a lot
 
Last edited by a moderator:
Physics news on Phys.org
You'd be able to capture these effects I'm sure. The net field is about ~10 uT but variations in the ionosphere and such should cause some noticeable changes. It'd be interesting to see what results you get.
 
Per wiki: http://en.wikipedia.org/wiki/Earth's_magnetic_field#Currents_in_the_ionosphere_and_magnetosphere

Electric currents induced in the ionosphere generate magnetic fields (ionospheric dynamo region). Such a field is always generated near where the atmosphere is closest to the Sun, causing daily alterations that can deflect surface magnetic fields by as much as one degree. Typical daily variations of field strength are about 25 nanoteslas (nT) (one part in 2000), with variations over a few seconds of typically around 1 nT (one part in 50,000).[52]
 
Thread 'Motional EMF in Faraday disc, co-rotating magnet axial mean flux'
So here is the motional EMF formula. Now I understand the standard Faraday paradox that an axis symmetric field source (like a speaker motor ring magnet) has a magnetic field that is frame invariant under rotation around axis of symmetry. The field is static whether you rotate the magnet or not. So far so good. What puzzles me is this , there is a term average magnetic flux or "azimuthal mean" , this term describes the average magnetic field through the area swept by the rotating Faraday...
Back
Top