Why three planets radio the sun.Why three planets radio the sun When the solar wind solar wind, stream of ionized hydrogen—protons and electrons—with an 8% component of helium ions and trace amounts of heavier ions that radiates outward from the sun at high speeds. , a continuous outpouring of electrically charged particles from the sun, collides at supersonic speed supersonic speed: see aerodynamics. with the magnetic field of a planet, it creates a shock wave on the sunward side. This in turn triggers the emission of radio waves Radio waves Electromagnetic energy of the frequency range corresponding to that used in radio communications, usually 10,000 cycles per second to 300 billion cycles per second. that radiate ra·di·ate v. 1. To spread out in all directions from a center. 2. To emit or be emitted as radiation. ra back toward the sun. The widths of the arc-shaped shock waves responsible for the radio signals from the solar system's inner three planets -- Mercury, Venus and Earth -- vary widely. The signals themselves, however, are quite similar, according to a new analysis of spacecraft data more than 10 years old. Earth and Mercury owe their shock waves to magnetic fields magnetic fields, n.pl the spaces in which magnetic forces are detectable; created by magnetostrictive ultrasonic scalers to cause the tips of instruments such as ultrasonic scalers to vibrate. generated by the dynamo at each planet's spinning core, says Chris T. Russell of the University of California, Los Angeles UCLA comprises the College of Letters and Science (the primary undergraduate college), seven professional schools, and five professional Health Science schools. Since 2001, UCLA has enrolled over 33,000 total students, and that number is steadily rising. . He and two graduate students coauthored the analysis, which appears in the December GEOPHYSICAL RESEARCH LETTERS Geophysical Research Letters is a publication of the American Geophysical Union. GRL is the organization's only letters journal. Since its introduction in 1974, GRL has published only short research letters, typically 3-5 pages long, which focus on a specific discipline or . The width of Earth's shock wave is about 10 times the planet's diameter. Owing to Mercury's roughly 50 percent smaller size and weaker magnetic field, its shock wave is only 5 percent as big as Earth's. Venus, nearly Earth's twin in size, derives its weak magnetic field from a far different mechanism: the collision of the solar wind and that planet's upper atmosphere. The resulting shock wave is only about 10 percent as wide as Earth's. Sunward-radiating radio waves spawned by these vastly different-sized shock waves share a number of common properties, the space physicists found. For instance, all radiate at extremely low frequencies -- about 1 to 3 cycles per second. They also leave the shock wave around each planet at approximately the same range of angles. And the amplitudes or strengths of the radio signals -- which naturally decrease with distance -- appear comparable when measured at about the same distance from their source. The new analysis also appears to have answered a long-standing question about which type of solar wind particles trigger the radio waves: negatively charged electrons or positively charged particles such as protons (ionized i·on·ize tr. & intr.v. i·on·ized, i·on·iz·ing, i·on·iz·es To convert or be converted totally or partially into ions. i hydrogen atoms). Previous studies, including one by Russell himself, had suggested that the solar wind ions took a "left-handed" spiral around the planetary magnetic field lines that captured them -- a sign that the ions were positively charged. But in the new report, Russell's team concludes that the spiraling only appeared left-handed owing to the spacecrafts' motion relative to the solar wind. By analyzing the spiral's direction with respect to the flowing solar wind, they have now determined that it's actually right-handed, Russell says. This indicates the radio waves are really spawned by electrons, his team now reports. |
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