U.S. researchers discover mystery about solar wind
As a result of the discovery, spacecraft, power grids and other modern facets of life could be made safer, according to researchers at the University of California in Los Angeles (UCLA).
The mystery about how the solar wind interacts with earth's atmosphere had puzzled scientists for half century.
The rate at which the solar wind transfers energy to the magnetosphere -- a highly magnetized region which surrounds and protects the Earth -- can vary widely, but what determines the rate of energy transfer was unclear, according to UCLA atmospheric scientists.
"We thought it was unknown, but we came up with a major surprise," UCLA professor Larry Lyons said in a press release available here on Monday.
Lyons said Heejong Kim, an assistant UCLA researcher and their colleagues analyzed radar data that measure the strength of the interaction by measuring flows in the ionosphere, the part of the Earth's upper atmosphere ionized by solar radiation. The results surprised them.
Charged particles carry currents, which cause significant modifications in the Earth's magnetosphere. This region is where communications spacecraft operate and where the energy releases in space known as substorms wreak havoc on satellites, power grids and communication systems.
"Any space physicist, including me, would have said a year ago there could not be substorms when the interplanetary magnetic field was staying northward, but that is wrong," Lyon said. "Generally, it's correct, but when you have a fluctuating interplanetary magnetic field, you can have substorms going off once per hour."
The magnetosphere was discovered in 1957. By the late 1960s, it had become accepted among scientists that the energy transfer rate was controlled predominately by the interplanetary magnetic field, the Sun's solar wind which carries the particles from the Sun's magnetic field to the Earth, taking about three or fours to reach the planet; Kazinform cites Xinhua.
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