Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>Chapman's theories werre prefered over Birkeland's theories until the mid 70s. Who know why the mainstream prefers their theories? It certainly isn't based on emprical physics.<br />Posted by michaelmozina</DIV><br /><br />HISTORY OF PRE-SPACE AGE MAGNETOSPHERE - David P. Stern<br /><br />
http://www.agu.org/journals/rg/v027/i001/RG027i001p00103/RG027i001p00103.pdf<br /><br />I hand typed some relevant material from the article, so any typos are mine and any bolded emphasis is mine and any reformatting paragraphs for ease of reading are mine<br />. <br /><br />From the article contained in the above link:<br /><br />Abstract<br /><br />This review traces early research on the Earth's magnetic environment, covering the period when only ground-based observations were possible. Observations of magnetic storms (1724) and of perturbations associated with the aurora (1741) suggested that those phenomena originated outside the Earth; correlation of the solar cycle (1851) with magnetic activity (1852) pointed to the Sun's involvement. The discovery of solar flares (1859) and growing evidence for their association with large storms led Birkeland (1900) to propose solar electron streams as the cause. <br /><br />Though laboratory experiments provided some support, the idea ran into theoretical difficulties and was replaced by Chapman and Ferraro's notion of solar plasma clouds. Magnetic storms were first attributed (Stoermer 1911) to a "ring current" of high-energy particles circling the Earth, but later work recognized that low energy particles undergoing guiding center drifts could have the same effect. To produce the ring current and aurora, plasma cloud particles required some way of penetrating The "Chapman-Ferraro cavity": Alfvén (1939) invoked an electric field, but his ideas met resistance. <br /><br />The picture grew more complicated with observations of comets (1943, 1951) which suggested a fast "solar wind" emanating from The Sun's corona at all times. This flow was explained by Parker's Theory (1958), and the permanent cavity which it produced around the Earth was later named the "magnetosphere" (1959). As early as 1905, Birkeland had proposed that the large magnetic perturbations of the polar aurora reflected a "polar" type of magnetic storm whose electric currents descended into the upper atmosphere; that idea, however, was resisted for more than 50 years. By the time of the International Geophysical Year (1957-1958), when the first artificial satellites were launched, most of the important features of the magnetosphere had been glimpsed, but detailed understanding had to wait for in situ observations.<br /><br /><br /><br />INTRODUCTION: {snip}<br /><br />EARLY WORK ON GEOMAGNETISM: {snip}<br /><br />THE SUNSPOT CYCLE: {snip}<br /><br />SOLAR FLARES: {snip}<br /><br /><br /><br />ELECTRON BEAMS FROM THE SUN?<br /><br />{snip}<br /><br />In 1896 Birkeland aimed cathod rays at a magnet and found that the magnet apparently "sucked in" cathode rays: he suggested that the Earth's field did the same to beams from the Sun. He comunicated his findings to his former teacher, the French mathematical physicist Henri Poincare, who showed that rather than being attracted, charged particles were guided by magnetic field lines (Poincare, 1896). Poincare calculated the motion of an electron in the field of a magnetic monopole, a completely soluble problem, and found that the electron spiraled around a cone bounded by field lines, gradually losing headway until at a certain distance it was reflected backward.<br /><br />{snip}<br /><br />Birkeland certainly did his best to promote the notion of solar electron streams. He also asked a colleague, the young mathematician Carl Stoermer, to calculate the motion of electrons in a dipole field, and Stoermer spent a large part of his career attacking that problem [Stoermer, 1955; Nutting, 1908]. Unfortunately, motion in a dipole field (unlike the monopole problem) has no analytical solution but is beset by pathologies resembling those of teh notorious three-body problem of celestial mechanics [Dragt and Finn, 1976], so that Stoermer never achieved what he had sought, though he did integrate many orbits numerically.<br /><br />{snip}<br /><br />The theory of solar electron streams soon hit another snag: Arthur Schuster [schuster, 1911; Chapman, 1934; Bartels, 1934b] showed that electrostatic repulsion would quickly disperse any stream of solar elelctrons.<br /><br />THE CHAPMAN-FERRARO CAVITY<br /><br />Sidney Chapman, a relative newcomer to the field of geomangentism who was apparently unaware of Schuster's work, again raised the idea of solar eelectron streams in a 1918 paper on magnetic storms [chapman, 1918; Akasofu et al., 1969]. He was pounced upon by Frederick Lindemann {snip}. Lindemann then suggested that any cloud or stream expelled from the Sun would have to be electically neutral, containing equal charge from ions and electrons.<br /><br />It took more than 10 years before Chapman figured out how a neutral beam could cause magnetic disturbances. In 1927 he was joined in his quest by Vincent C. A. Ferraro, newly graduated [Cowling, 1975].<br /><br />The two had realized that an electrically neutral mixture of ions and electrons - what would nowadays be called a plasma - would be a very good conductor of electricity.<br /><br />{snip}<br /><br />The Earth's magnetic field also exerts a force on the induced currents, and that force grows stronger as the cloud draws nearer. Ultimately, Chapman and Ferraro argued, it became strong enough to stop any further frontal advance of the cloud toward Earth; however, the flanks continued to advance, so that soon a cavity was formed, enveloping the Earth. That was known for many years as the "Chapman-Ferraro cavity, the region from which the plasma of the cloud was excluded by the action of the Earth's magnetic field.<br /><br />{snip}<br /><br />THE RING CURRENT {snip}<br /><br />ALFVEN'S THEORY AND ELECTRIC FIELD<br /><br />{snip}<br /><br />Alfven did not believe in the Chapman-Ferraro theory, which treated the cloud as a continuous fluid [Alfven, 1951] but rather viewed the cloud as a collection of individually moving particles.<br /><br />{snip}<br /><br />INTERPLANETARY PLASMA<br /><br />{snip}<br /><br />It then became clear that the Chapman-Ferraro cavity was not a temporary feature but existed at all times, and it received the name "magnetosphere" coined by Gold [1959]. Rapidly spreading plasma clouds produced by solar flares, like those envisioned by Chapman and Ferraro, are sometimes superposed on the solar wind flow. We now know that when the expansion velocity of such clouds greatly exceeds that of the solar wind, they are indeed preceded by collision-free shocks.<br /><br />POLAR MAGNETIC STORMS<br /><br />{snipped Chapman's work on distinguishing between magnetic storms and Birkeland's polar storms (now know as substorms.)}<br /><br />Contrary to Birkeland's interpretation, much of the horizontal part of their circuit, in the ionosphere, flows not along auroral arcs but perpendicular to them, for by a quirk of electrodynamics [fukushima, 1969, 1976] the main circuit produces only a weak magnetic signature on the ground. What Birkeland observed was mostly the signature of an associated Hall current, the "auroral electrojet" which parallels auroral arcs.<br /><br />ASSESSMENT<br /><br />{snip}<br /><br />Many important magnetospheric features had indeed been inferred before spacecraft were available, but in almost every case some important detail was missing or wrong. The Chapman-Ferraro cavity was predicted as a temporary rather than permanent feature, and the same was true for the radiation belt. Alfven's convection contained a nucleus of truth, but electric field effect supplemented rather than supplanted the Chapman-Ferraro picture, and the convection which they produced was found to flow from the tail sunward, opposite to its direction in Alfven's theory. Birkeland's auroral currents did exist, but their configuration was not the one predicted. The existence and importance of the magnetospheric tail generally went unsuspected, and so did the existence of parallel electric fields along auroral arcs, although Alfven later developed the theory of quasi-neutral equilibria, relevant to such fields. All this underscores the essential role of in situ observations: one can only speculate how much of this might be paralleled in astrophysics.<br /><br />END OF ARTICLE<br /><br />to be continued...<br /><br /> <div class="Discussion_UserSignature"> <div> </div><br /><div><span style="color:#0000ff" class="Apple-style-span">"If something's hard to do, then it's not worth doing." - Homer Simpson</span></div> </div>