Layers of Atmosphere:Ionosphere

The ionosphere is a name for the layer of the earth’s atmosphere that is ionized by solar  wind. Even though many believe the space around earth is a vacuum, it is not completely empty. The sun’s upper atmosphere (the corona) is very hot and some of its hydrogen and helium are able to escape the sun’s gravity. Because the gas is hot and is in a constant stream of solar energy it becomes a fully ionized plasma. This streaming plasma is the solar wind, and it flows out past the earth affecting the earth’s magnetic field, the magnetosphere and ionosphere(read here about Anatomy of Sun). The Earth receives a lot of energy from the sun in the form of radiation- about 1370 Watts per square meter.The ionosphere is the uppermost part of the atmosphere, distinguished because it is ionized by solar radiation. It plays an important part in atmospheric electricity and forms the inner edge of the magnetosphere. It has practical importance because, among other functions, it influences radio propagation to distant places on the Earth.

The ionosphere is a shell of electrons and electrically charged atoms and molecules that surrounds the Earth, stretching from a height of about 50 km to more than 1000 km. It owes its existence primarily to ultraviolet radiation from the sun.

The lowest part of the Earth’s atmosphere, the troposphere extends from the surface to about 10 km. Above 10 km is the stratosphere, followed by the mesosphere. In the stratosphere incoming solar radiation creates the ozone layer. At heights of above 80 km (50 miles), in the thermosphere, the atmosphere is so thin that free electrons can exist for short periods of time before they are captured by a nearby positive ion. The number of these free electrons is sufficient to affect radio propagation. This portion of the atmosphere is ionized and contains a plasma which is referred to as the ionosphere. In a plasma, the negative free electrons and the positive ions are attracted to each other by the electromagnetic force, but they are too energetic to stay fixed together in an electrically neutral molecule.

Ionization depends primarily on the Sun and its activity. The amount of ionization in the ionosphere varies greatly with the amount of radiation received from the sun. Thus there is a diurnal (time of day) effect and a seasonal effect. The local winter hemisphere is tipped away from the Sun, thus there is less received solar radiation. The activity of the sun is associated with the sunspot cycle, with more radiation occurring with more sunspots. Radiation received also varies with geographical location (polar, auroral zones, mid-latitudes, and equatorial regions). There are also mechanisms that disturb the ionosphere and decrease the ionization. There are disturbances such as solar flares and the associated release of charged particles into the solar wind which reaches the Earth and interacts with its geomagnetic field.

Sources:

Wikipedia

The Ionosphere Explained

About the Ionosphere

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IIT-Kanpur of India sets up base station for its nano Jugnu satellite

The Indian Institute of Technology-Kanpur has set up a base station within its premises for nano-satellite Jugnu, which will be launched in a polar orbit by the Indian Space Research Organisation (ISRO) early next year. The nano-satellite, designed and developed by the IIT was  handed over to the ISRO .

The data packets will include transmission of images, health status of the satellite and commands related to the details of locations of which the images will be taken. “We are through with the setting up of the transmission device and antenna, and are confident of completing all the related tests in the next few weeks,” Agarwal said. The satellite, which will be placed in an orbit around 700 kms from the Earth, will remain in space for one year. The nano satellite will encircle the earth 15 times in a day.

Sources:

GIS Development

Indian Express

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Turning Energy Waste to Into Hydrogen Fuel

Materials scientists at the University of Wisconsin-Madison have designed a way to harvest small amounts of waste energy and harness them to turn water into usable hydrogen fuel.

READ HERE

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Magnetopause

The magnetic boundary between the Earth’s field and the solar wind, named the magnetopause, has a bullet-shaped front, gradually changing into a cylinder. Its cross-section is approximately circular.Distances in the magnetosphere are often measured in Earth radii (RE), with one Earth radius amounting to 6371 km or 3960 miles. In these units, the distance from the Earth’s center to the “nose” of the magnetosphere is about 10.5 RE and to the flanks abreast of the Earth about 15 RE, while the radius of the distant tail is 25-30 RE. By way of comparison, the moon’s average distance is about 60 RE.

When solar wind flows past the Earth, it applies pressure to the magnetic field of the earth. The brunt of the solar wind pressure is exerted on the  field, compressing it. Only the restorative pressure of the magnetic field pushes against the solar wind, and a rough balance of these pressures occurs. Like imaginary football scrimage line, this balance moves towards the earth when the solar wind pressure  increases, and it moves outwards toward the sun as the solar wind pressure . This scrimage line is called the magnetopause boundary.

Distances in the magnetosphere are often measured in Earth radii (RE), with one Earth radius amounting to 6371 km or 3960 miles. In these units, the distance from the Earth’s center to the “nose” of the magnetosphere is about 10.5 RE and to the flanks abreast of the Earth about 15 RE, while the radius of the distant tail is 25-30 RE. By way of comparison, the moon’s average distance is about 60 RE.

Links and Sources:

The Magnetopause

Nasa

Wikipedia

UCLA

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