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Schoolnet
Schoolnet

... 25. During the year, the angle at which the path of the Sun appears in the sky varies. In the Northern Hemisphere, the path of the Sun appears higher on the horizon during the summer and lower on the horizon during the winter. Which factor most contributes to the variation in the path of the Sun acr ...
To, Mr. Prasad Modak We are group of students from Physics
To, Mr. Prasad Modak We are group of students from Physics

... in Africa and passes through Chad, Central African Republic, Democratic Republic of the Congo, Uganda, Kenya, and Somalia. After leaving Africa, the path crosses the Indian Ocean where the maximum duration of annularity reaches 11 min 08 s. The central path then continues into Asia through Banglades ...
The Atmosphere
The Atmosphere

... pressure, relative humidity, and wind speed and direction in the atmosphere is essential for weather forecasting and meteorological research • During the latter part of the 19th century and the first quarter of the 20th century, this information was obtained mainly by meteorographs sent aloft on tet ...
The Sun is our local star.
The Sun is our local star.

... Material in the Sun’s corona is continually streaming out into space. The electrically charged particles that flow out in all directions from the corona are called the solar wind. The solar wind extends throughout our solar system. Most of the solar wind flowing toward Earth is safely guided around ...
space research in slovakia - Astronomical Institute WWW Homepage
space research in slovakia - Astronomical Institute WWW Homepage

... COSPAR, were devoted to the research in solar and stellar physics using satellite observations, mainly in the UV, XUV and X-ray spectral regions. It concerns mainly solar data of the current SOHO mission and TRACE satellite and from previous satellites of the NOAA and GOES series. Stellar data of th ...
AST-2003 Review for Final Exam
AST-2003 Review for Final Exam

... •Main characteristics of Jovian planets. How do they compare with terrestrial planets •Basic differences between terrestrial and Jovian planets •Comparison of mass, diameter, density, number of satellites, distance from the Sun •Satellites (or moons) that are unique in the solar system •The orbits o ...
CGS
CGS

... declination must go to the Chinese. Needham has tabulated eighteen recorded Chinese compass observations of declination covering the period about 720-1829. These are of interest not only to historians but also to geophysicists, for they represent the earliest recorded direct observations of the Eart ...
Like a boiling teakettle atop a COLD stove, the sun`s HOT outer
Like a boiling teakettle atop a COLD stove, the sun`s HOT outer

... perfect conductor cannot sustain an electric field, because charged particles instantaneously reposition themselves to neutralize it. And if a plasma cannot sustain an electric field, it cannot move relative to the magnetic field (or vice versa), because to do so would induce an electric field. This ...
The following slide show is a compilation of slides from... have been produced by different members of the fusion and...
The following slide show is a compilation of slides from... have been produced by different members of the fusion and...

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Planetary interiors and surfaces

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A new picture of Halley`s Comet [Translated and adapted from

... nights. Altogether 81 pictures were taken, each by a single scope, with a total exposure time of 32 284 seconds. The pictures were added together electronically and the images of stars subtracted to give the image above. At the very low brightness of Halley, only one photon every 1⋅6 seconds was rec ...
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Lecture 3: Matter

... Gases: Higher temperature means more average kinetic energy (faster speeds) per atom or molecule. ...
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Worksheet 4.2 (Answer Key)

... 5. Return to your equation for the magnetic field strength in part 1. We are hoping to estimate the strength of the magnetic field that produced the solar flare and CME from this equation. If you use the amount of energy that the NASA scientists found as the total energy released by the flare in Workshe ...
Stellar Winds and Hydrodynamic Atmospheres
Stellar Winds and Hydrodynamic Atmospheres

... Note: if temperature of corona were as cool as photosphere, we would still have a solar wind, but supersonic just at 6 AU in principle, all stars will have a (weak) wind, but the solar wind is strong because of high temperature in corona ...
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... Addressed main questions in this theme: • How does an Earth-sized planet without global magnetic field interact with the solar wind and why and at which rate does it lose its atmosphere? • Does Venus’ atmosphere, ionosphere and solar wind interaction region present an electromagnetic wave activity, ...
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... field revers direction, that is why it is called the neutral sheet. The cross-tail current continues to a current flowing around the tail surface. It is important to note, that the magnetic field lines connect different magnetospheric regions to different latitudes in the ionosphere. At low and midd ...
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... The strength of the earth’s magnetic field had decreased10% over the last 150 years. At this rate, the field will disappear altogether in 1,500 to 2,000 years. ...
Chapter 1
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... C. Lava flows on the seafloor precipitated from seawater. D. all of the above 6) The currently accepted age of Earth is ________ years. A. 4.6 thousand B. 6.4 trillion C. 4.6 billion D. 6.4 million 8) The ________ division of the geologic time scale is an era of the Phanerozoic eon. A. Paleocene B. ...
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... There are three fundamental ways the Earth’s radiation balance can change, thereby causing a climate change: (1) changing the incoming solar radiation (e.g., by changes in the Earth’s orbit or in the Sun itself), (2) changing the fraction of solar radiation that is reflected (this fraction is called ...
Chapter 1
Chapter 1

... from the core to the surface in the form of electromagnetic radiation, radiant energy that travels through space and matter. The heat that we feel when when we hold a hand over an electric light bulb or lie on a beach on a hot, sunny day is produced by electromagnetic radiation. In the Sun’s core th ...
zaneposter
zaneposter

... (2002), that most of the magnetars phenomenology can be explained by the onset of a long-lasting magnetospheric twist. Basically, in magnetars the strong toroidal component of the internal magnetic field stresses the star crust inducing a deformation of the surface layers and twisting up the externa ...
The Atmosphere - MIT Haystack Observatory
The Atmosphere - MIT Haystack Observatory

... • The Earth has a magnetic field that reaches into space • The magnetic field of the Earth is surrounded in a region called the magnetosphere. The magnetosphere prevents most of the particles from the sun ( solar wind) from hitting the Earth • Some particles from the solar wind can enter the magneto ...
Atomic Physics Explaining the Universe
Atomic Physics Explaining the Universe

... Hot component has 1% EM of AR component ...
< 1 ... 15 16 17 18 19 20 21 22 23 ... 37 >

Energetic neutral atom



Energetic neutral atom (ENA) imaging, often described as ""seeing with atoms"", is a technology used to create global images of otherwise invisible phenomena in the magnetospheres of planets and throughout the heliosphere, even to its outer boundary.This constitutes the far-flung edge of the solar system.The solar wind consists of ripped-apart atoms (called plasma) flying out of the Sun. This is mostly hydrogen, that is, bare electrons and protons, with a little bit of other kinds of nuclei, mostly helium. The space between solar systems is similar, but they come from other stars in our galaxy. These charged particles can be redirected by magnetic fields; for instance, Earth's magnetic field shields us from these particles. But, every so often, a few of them steal electrons from neutral atoms they run into. At that point, they become neutral, although they're still moving very fast, and they travel in an exact straight line. These are called Energetic Neutral Atoms. ENA images are constructed from the detection of these energetic neutral atoms.Earth's magnetosphere preserves Earth's atmosphere and protects us from cell-damaging radiation. This region of ""space weather"" is the site of geomagnetic storms that disrupt communications systems and pose radiation hazards to humans traveling at high polar altitudes or in orbiting spacecraft. A deeper understanding of this region is vitally important. Geomagnetic weather systems have been late to benefit from the satellite imagery taken for granted in weather forecasting, and space physics because their origins in magnetospheric plasmas present the added problem of invisibility.The heliosphere protects the entire Solar System from the majority of cosmic rays but is so remote that only an imaging technique such as ENA imaging will reveal its properties. The heliosphere's structure is due to the invisible interaction between the solar wind and cold gas from the local interstellar medium.The creation of ENAs by space plasmas was predicted but their discovery was both deliberate and serendipitous. While some early efforts were made at detection, their signatures also explained inconsistent findings by ion detectors in regions of expected low ion populations. Ion detectors were co-opted for further ENA detection experiments in other low-ion regions. However, the development of dedicated ENA detectors entailed overcoming significant obstacles in both skepticism and technology.Although ENAs were observed in space from the 1960s through 1980s, the first dedicated ENA camera was not flown until 1995 on the Swedish Astrid-1 satellite, to study Earth's magnetosphere.Today, dedicated ENA instruments have provided detailed magnetospheric images from Venus, Mars, Jupiter, and Saturn. Cassini's ENA images of Saturn revealed a unique magnetosphere with complex interactions that have yet to be fully explained. The IMAGE mission's three dedicated ENA cameras observed Earth's magnetosphere from 2000–2005 while the TWINS Mission, launched in 2008, provides stereo ENA imaging of Earth's magnetosphere using simultaneous imaging from two satellites.The first ever images of the heliospheric boundary, published in October 2009, were made by the ENA instruments aboard the IBEX and Cassini spacecraft. These images are very exciting because they challenge existing theories about the region.
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