History of Geophysical Research in The Netherlands ... - DWC - KNAW
History of Geophysical Research in The Netherlands ... - DWC - KNAW
History of Geophysical Research in The Netherlands ... - DWC - KNAW
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on the formation <strong>of</strong> the ionized layers, on the propagation <strong>of</strong> radio waves <strong>in</strong><br />
the ionosphere, and on prediction and selection <strong>of</strong> the most suitable frequencies<br />
for cover<strong>in</strong>g a certa<strong>in</strong> distance by radio. In a further paper (Groenewold,<br />
1949) he discussed temporary variations <strong>in</strong> the ionization and the <strong>in</strong>fluence on<br />
the ionosphere <strong>of</strong> outbursts on the sun. He published also a theoretical study<br />
on the triple magnetic splitt<strong>in</strong>g <strong>of</strong> radio waves reflected <strong>in</strong> the F2-1ayer (Groenewold,1950).<br />
Veldkamp and Scholte (1954a) also studied the magnetic double refraction <strong>of</strong><br />
electromagnetic waves <strong>in</strong> the ionosphere. <strong>The</strong>y <strong>in</strong>vestigated the equatorial<br />
electrojet <strong>in</strong> the ionosphere, as revealed by the analysis <strong>of</strong> solar flare effects ,<br />
and expla<strong>in</strong>ed some properties <strong>of</strong> the electrojet by the non-co<strong>in</strong>cidence <strong>of</strong> the<br />
geomagnetic and geographic equators (Veldkamp and Scholte, 1954). H.J.A.<br />
Vesseur (1970) succeeded <strong>in</strong> <strong>in</strong>ferr<strong>in</strong>g from the fad<strong>in</strong>g pattern <strong>of</strong> radio waves<br />
reflected <strong>in</strong> the ionosphere the rhythmic tidal movements <strong>of</strong> air <strong>in</strong> the ionosphere,<br />
which are responsible for the diurnal geomagnetic variation. <strong>The</strong> w<strong>in</strong>d<br />
movements <strong>in</strong> the E-layer are recorded almost cont<strong>in</strong>uously by an automatic<br />
apparatus developed by Vesseur. He could determ<strong>in</strong>e the diurnal and the semidiurnal<br />
period <strong>of</strong> the tidal movements <strong>in</strong> the E-layer above the <strong>Netherlands</strong><br />
over a period <strong>of</strong> years (Vesseur, 1972). A similar apparatus was set up near<br />
Paramaribo (Sur<strong>in</strong>ame); it was <strong>in</strong> operation from January 1971 until September<br />
1972.<br />
H. Kelder (1975) <strong>in</strong>vestigated the <strong>in</strong>fluence <strong>of</strong> acoustic gravity waves on ion<br />
density <strong>in</strong> the E-layer. <strong>The</strong> tidal movements are <strong>in</strong> fact strongly disturbed by<br />
acoustic waves with a very long wavelength , which travel through the ionosphere<br />
and the thermosphere (Kelder, 1976).<br />
Temporary disturbances <strong>in</strong> the geomagnetic field, which are caused by "disturbed"<br />
solar radiation - corpuscular as weIl as electromagnetic - penetrat<strong>in</strong>g<br />
the outer layers <strong>of</strong> the atmosphere, are important for chang<strong>in</strong>g the reflect<strong>in</strong>g<br />
power <strong>of</strong> the ionosphere. For this reason study <strong>of</strong> the ionosphere is <strong>of</strong> practical<br />
importance for radio propagation through the ionosphere (Vesseur, 1974).<br />
<strong>The</strong> results <strong>of</strong> this research are published each month by the KNMI <strong>in</strong> an "Ionospheric<br />
Bullet<strong>in</strong>". In this monthly publication are given, not only heights and<br />
plasma freq uencies <strong>of</strong> the ionospheric layers, but also factors for calculat<strong>in</strong>g the<br />
radio frequencies for cover<strong>in</strong>g a certa<strong>in</strong> distance and further the ionospheric<br />
and geomagnetic disturbance-<strong>in</strong>dices, disturbances <strong>in</strong> the <strong>in</strong>tensity <strong>of</strong> cosmic<br />
radiation , <strong>in</strong>tensity <strong>of</strong> radio radiation from the sun and summaries <strong>of</strong> special<br />
phenomena <strong>of</strong> the solar radiation (KNMI, 1949 up to the present).<br />
<strong>The</strong> monthly publication <strong>of</strong> the "Ionospheric Bullet<strong>in</strong>" by the KNMI gives<br />
evidence <strong>of</strong> the close relation exist<strong>in</strong>g between the ionosphere, the earth's<br />
magnetic field, cosmic radiation and phenomena on the sun.<br />
1.5. GEOMAGNETISM AND COSMIC RAYS<br />
About 1930 J. Clay (pr<strong>of</strong>essor at the Technical University <strong>of</strong> Bandoeng from<br />
1920 to 1929, and pr<strong>of</strong>essor at the Municipal University <strong>of</strong> Amsterdam from 1929<br />
to 1952) discovered that the geomagnetic field exerts an <strong>in</strong>fluence on cosmic<br />
rays. Dur<strong>in</strong>g his voyages bet ween the <strong>Netherlands</strong> and the <strong>Netherlands</strong> East<br />
Indies, Clay studied the <strong>in</strong>tensity <strong>of</strong> cosmic radiation (at that time called ultraradiation)<br />
. lt appeared that this very penetrat<strong>in</strong>g radiation depended on the<br />
geomagnetic latitude. <strong>The</strong> <strong>in</strong>tensity was m<strong>in</strong>imal <strong>in</strong> the Gulf <strong>of</strong> Aden, which is<br />
<strong>in</strong> the neighbourhood <strong>of</strong> the geomagnetic equator (Clay, 1932). From this the<br />
corpuscular character <strong>of</strong> cosmic rays became evident; only electrically charged<br />
particles can be <strong>in</strong>fluenced by the magnetic field <strong>of</strong> the earth. <strong>The</strong> latitude<br />
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