magnetosphere oor Viëtnamees
magnetosphere
en
(physics) The comet-shaped region around Earth or another planet in which charged particles are trapped or deflected. Shaped by the solar wind and the planet's magnetic field.
Vertalings in die woordeboek Engels - Viëtnamees
quyển từ
en
region around a planet
Từ quyển
en
area of space near an astronomical object
Mars lost its magnetosphere,
sao Hỏa bị mất từ quyển,
từ quyển
Mars lost its magnetosphere,
sao Hỏa bị mất từ quyển,
Geskatte vertalings
Vertoon algoritmies gegenereerde vertalings
Prenteboek
voorbeelde
Advanced filtering
Voorbeelde moet herlaai word.
Many types of waves in the ULF frequency band can be observed in the magnetosphere and on the ground.
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In front of the magnetopause (at a distance from 80 to 130 RJ from the planet's center) lies the bow shock, a wake-like disturbance in the solar wind caused by its collision with the magnetosphere.
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In the case of the Sun, even this criterion fails (because its magnetosphere is very complex and does not really rotate in a steady fashion), and an agreed-upon value for the rotation of its equator is used instead.
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The load of plasma from Io greatly expands the size of the Jovian magnetosphere, because the magnetodisk creates an additional internal pressure which balances the pressure of the solar wind.
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Which, what we do, we soften... we soften... the Plasmatic Magnetic Field, or magnetosphere around the Plasma.
Dù sao cũng phải để ýQED QED
The Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission began in February 2007 as a constellation of five NASA satellites (THEMIS A through THEMIS E) to study energy releases from Earth's magnetosphere known as substorms, magnetic phenomena that intensify auroras near Earth's poles.
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Observations taken by the Mariner 10 spacecraft detected this low energy plasma in the magnetosphere of the planet's nightside.
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Neptune's bow shock, where the magnetosphere begins to slow the solar wind, occurs at a distance of 34.9 times the radius of the planet.
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Alfvén made many contributions to plasma physics, including theories describing the behavior of aurorae, the Van Allen radiation belts, the effect of magnetic storms on the Earth's magnetic field, the terrestrial magnetosphere, and the dynamics of plasmas in the Milky Way galaxy.
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As cold, dense plasma moves outward, it is replaced by hot, low-density plasma (temperature 20 keV (200 million K) or higher) moving from the outer magnetosphere.
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Wider and flatter than the Earth's magnetosphere, Jupiter's is stronger by an order of magnitude, while its magnetic moment is roughly 18,000 times larger.
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The plasma in this doughnut-shaped ring of ionized sulfur, oxygen, sodium, and chlorine originates when neutral atoms in the "cloud" surrounding Io are ionized and carried along by the Jovian magnetosphere.
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From its distant orbit, the spacecraft produced a wealth of images of the previously invisible region of space in the inner magnetosphere, exceeded all its scientific goals.
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As a by-product of this activity, sulfur, sulfur dioxide gas and silicate pyroclastic material (like ash) are blown up to 200 km (120 mi) into space, producing large, umbrella-shaped plumes, painting the surrounding terrain in red, black, and white, and providing material for Io's patchy atmosphere and Jupiter's extensive magnetosphere.
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The brightest spot belongs to Io, which is the main source of the plasma in the magnetosphere (see above).
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And that's because the magnetosphere magnetic field of the Earth, euh, Matter, comes in touch with the magnetosphere of the Antimatter, and when two Plasmas come together, the field interaction creates what we know as light... different wavelengths.
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For example, in the solar wind they interact with the Earth's magnetosphere giving rise to Birkeland currents and the aurora.
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The auroral radio, optical and X-ray emissions, as well as synchrotron emissions from the radiation belts all show correlations with solar wind pressure, indicating that the solar wind may drive plasma circulation or modulate internal processes in the magnetosphere.
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IMAGE (Imager for Magnetopause-to-Aurora Global Exploration) is a NASA Medium Explorers mission that studied the global response of the Earth's magnetosphere to changes in the solar wind.
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However, during unusually strong flares, protons can be produced with sufficient energies to reach the Earth's magnetosphere and ionosphere around the north pole and south pole.
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When flux tubes loaded with the cold Ionian plasma reach the outer magnetosphere, they go through a reconnection process, which separates the magnetic field from the plasma.
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When solar protons enter the Earth's magnetosphere where the magnetic fields are stronger than solar magnetic fields, they are guided by the Earth's magnetic field into the polar regions where the majority of the Earth's magnetic field lines enter and exit.
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In the middle (between 10 and 40 RJ) and outer (further than 40 RJ) magnetospheres, the magnetic field is not a dipole, and is seriously disturbed by its interaction with the plasma sheet (see magnetodisk below).
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Luckily, here on Earth, we are protected by our planet's natural shield, a magnetic bubble that we call the magnetosphere and that you can see here on the right side.
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Inside the magnetosphere is the plasmasphere, a donut-shaped region containing low-energy charged particles, or plasma.
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67 sinne gevind in 4 ms. Hulle kom uit baie bronne en word nie nagegaan nie.