16.11.2012 Views

Antigen Biotinylated Anti-Rabbit lgs Rabbit Primary Antiserum AB ...

Antigen Biotinylated Anti-Rabbit lgs Rabbit Primary Antiserum AB ...

Antigen Biotinylated Anti-Rabbit lgs Rabbit Primary Antiserum AB ...

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

Magnetoreception - Introduction<br />

1.2 The Earth’s Magnetic Field<br />

At the end of the 16th century, William Gilbert determined that the Earth is a big magnet,<br />

implying that it has a magnetic field (cf., Lanza & Meloni 2006). The Earth’s magnetic field<br />

(fig. B1) is a dipole field, i.e. a system comprising two magnetic charges (or masses) of equal<br />

intensity and opposite signs (cf., Skiles 1985; Lanza & Meloni 2006). These magnetic field’s<br />

measurements are based on superimposed contributions from different sources.<br />

Corresponding to these different origins, the Earth’s magnetic field of force can be<br />

separated into: the main field, generated in the fluid core by a geodynamo mechanism; the crustal<br />

field, generated by magnetized rocks in the Earth’s crust; the external field, generated by electric<br />

currents flowing in both ionosphere and magnetosphere through interactions of the solar<br />

electromagnetic radiation and the solar wind<br />

with the Earth’s magnetic field; and the<br />

magnetic field resulting from an electromagnetic<br />

induction process generated by electric<br />

currents induced in the crust and the upper<br />

mantle by external magnetic field time<br />

variations – the Earth is partly an electric<br />

conductor, and currents can be induced in its<br />

conducting parts by external time variations.<br />

The most stable parts of the Earth’s magnetic<br />

field are the main and the crustal field, which<br />

mainly determine its spatial structure. The<br />

Fig. B1 Schematical view of the Earth’s<br />

magnetic field lines. The Earth is<br />

represented by a sphere, N and S are the ideal<br />

magnetic pole positions (from Lanza &<br />

Meloni 2006).<br />

field is also subject to time variations. These can be divided into long-term variation due to<br />

changes within the Earth, and short-term variation of external origin (see external field above)<br />

(cf., Lanza & Meloni 2006). The Earth’s magnetic field behaves like a small, very strong bar<br />

magnet close to the Earth’s centre that is tilted against the rotation axis by about 11° (cf.,<br />

Press & Siever 2003).<br />

Determining exact geomagnetic coordinates, i.e. identifying exact positions of points<br />

on the Earth’s surface with respect to a geomagnetic reference (similar to geographic<br />

coordinates), is enabled by use of colatitudes and longitudes in the geomagnetic dipole frame.<br />

This coordinate system also enables the identification of north and south geomagnetic poles<br />

as those points on the Earth where the ideal central dipole axis intersects the surface.<br />

Accordingly, the geomagnetic equator is the ideal line on the surface representing the<br />

intersection of the plane passing through the Earth’s centre orthogonal to the central dipole<br />

(Lanza & Meloni 2006).<br />

41

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!