GALILEO:European Satellite Navigation System

A permanent reference in time and space.

Galileo is Europe’s contribution to a global navigation satellite infrastructure (GNSS).

More and more often, it will become necessary to ascertain one’s precise position in space and time in a reliable manner. This will be possible with the GALILEO satellite radio navigation system, an initiative launched by the European Union and the European Space Agency. This worldwide system will ensure complementarity with the current GPS system.

Satellite radio navigation is an advanced technology. It is based on the emission from satellites of signals indicating the time extremely precisely. This enables any individual to determine his or her position or the location of any moving or stationary object (e.g. a vehicle, a ship, or a herd of cattle, etc.) to within one metre thanks to a small cheap individual receiver.

GALILEO is based on a constellation of 30 satellites and ground stations providing information concerning the positioning of users in many sectors such as transport (vehicle location, route searching, speed control, guidance systems, etc.), social services (e.g. aid for the disabled or elderly), the justice system and customs services (location of suspects, border controls), public works (geographical information systems), search and rescue systems, or leisure (direction-finding at sea or in the mountains, etc.).

Satellite navigation – How does it work ?

Since time immemorial, people have looked to the heavens to find their way. Today, satellite navigation is continuing this tradition, while offering, thanks to leading-edge technology, an accuracy far beyond that possible by simply observing the sun and the stars. This technology, which has been developed over the last thirty years or so, essentially for military purposes originally, enables anyone with a receiver capable of picking up signals emitted by a constellation of satellites to instantly determine their position in time and space very accurately.

The operating principle is simple: the satellites in the constellation are fitted with an atomic clock measuring time very accurately. The satellites emit personalised signals indicating the precise time the signal leaves the satellite. The ground receiver, incorporated for example into a mobile phone, has in its memory the precise details of the orbits of all the satellites in the constellation. By reading the incoming signal, it can thus recognise the particular satellite, determine the time taken by the signal to arrive and calculate the distance from the satellite. Once the ground receiver receives the signals from at least four satellites simultaneously, it can calculate the exact position.

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Mohd Shafi

Born: 1st August 1924, Jaunpur (UP) India.
Died: 9th December, 2007, Aligarh (UP) India.
Father: Husain Ali
Children: Prof. Mohd. Jamil (Civil Engg., AMU Aligarh), Dr. Bilquees Bano

Education: 1945: B.A. Allahabad University
1947: M.A. (Geography), AMU Aligarh
1956: Ph.D. from London School of Economics with Prof. Dudley Stamp

Career: 1948: Lecturer, Department of Geography, AMU Aligarh
1956: Reader, Department of Geography, AMU Aligarh
1962: Professor, Department of Geography, AMU Aligarh
1962-84: Chairman, Department of Geography, AMU Aligarh
1966-68: Dean, Faculty of Science
1959-62: Provost, Sir Shah Sulaiman Hall
1984: Professor Emeritus in Dept. of Geography AMU Aligarh
1972-74: Director Academic Program (DAP)
1979-80: Pro-Vice Chancellor of Aligarh Muslim University

1985-1993: Vice-President, International Geographical Union
http://www.igu-net.org/

1987: Member, Royal geographical Society of London.
1992-95: Pro-Chancellor of Aligarh Muslim University

2001: Padama Shri by the Government of India
2001: Bhoogol Ratna Award by Bhoovigyan Vikas Foundation, New Delhi.
2002: “Saraswati Award” in Environmental Science and Ecology by the UGC

Member: The Scientific Committee of the International Social Science Council

“Laureate d’ honneur” by the International Geographical union at Glasgow,
UK. ‘Academician’ by the Russian Academy of Sciences.

Member : Bureau for Promotion of Urdu

President : Indian Geographical Union, Indian Geographical Council.

Mohd. Shafi was born on 1st June, 1924 in historical city of Jaunpur in eastern Uttar Pardesh. In 1945, after completing his graduation from Allahabad University, he joined Aligarh Muslim University in M.A. in Geography.

Association with Aligarh :
Mohd. Shafi completed his M.A. in Geography in 1947. Like other part of the country, Aligarh Muslim University campus was also not safe from the socio-political activities of Indian Freedom movement during this time. But this did not affect the studies of young Mohd. Shafi. After completing his M.A., he joined AMU as lecturer in department of Geography. He completed his Ph.D. from London University in 1956 and was appointed as Reader in Geography department of AMU. His Ph.D. work was well recognized at International level. His research area Agricultural Geography got attention in the research community an department of Geography of AMU Aligarh was declared a center of excellence for the subject buy University Grant Commission and Mohd. Shafi was appointed its Coordinator. His research work on the Food System of India has been recognized with high honors in many countries, and by the United Nations.In 1962, he was appointed as Professor in the same department. In the same year he became Chairman, Department of Geography and served on this position till 1984. He has published 11 books and 130 research papers, and has supervised 34 doctoral works. He also served as Provost for 3 years and Dean Faculty of Science. In 1972, Prof. Abdul Aleem, Vice-Chancellor of AMU Aligarh appointed him as Director of Academic Program (DAP). He served as DAP till 1974. His academic excellence and administrative abilities were noticed by AMU Vice Chancellor Prof. Ali Mohammad Khusro and in 1979 he appointed him as Pro-Vice Chancellor of Aligarh Muslim University. He served as Pro Vice-Chancellor for two years. In 1984, he retired from his services but Department of Geography appointed him as Professor Emeritus.

Professor Shafi is the first Indian Geographer in the Indian sub-continent including SAARC countries to receive this prestigious award at the 30th International Geographical Congress held at Glasgow in U.K. More than 1800 geographers from 81 countries participated in the Congress. The Russian Academy of Sciences also conferred on him its highest award ‘Academician’. The Royal Geographers Society, London made him its Honorary Corresponding Member of the Council and the American Geographic Society offered him its Fellowship. In 2002 he has been honored for “Saraswati Award” in Environmental Science and Ecology by the University Grants Commission. On April 22, 2001 at New Delhi Bhoovigyan Vikas Foundation awarded him the maiden Bhoogol Ratna Award, which consists of Rs One lakh and a citation.

In AMU Court meeting on July 5th, 1992, Professor Mohd Shafi was elected as Pro-Chancellor of Aligarh Muslim University for a period of 3 years.

On 9th December 2007, Professor Mohd Shafi died in Aligarh. He was laid to rest in University Graveyard ‘Mintoyee’.
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Climate Forcing

Climate forcing is a term you hear bounced around a lot among academics and politicians. Basically what it means in relation to climate science is the amount of energy that something contributes or takes away from our current energy exchange in the greenhouse effect. It is usually measured in a certain amount of energy (Watts) over a certain amount of area (meters squared). This is really important in determining what effects each thing has on our current global temperatures and how much each thing contributes to climate change. Radiative forcing takes into acct. the change in the amount of a substance and its energy influence. For example, even though we as a society may be spitting out tons of CO2, if CO2 has a small forcing it may not make much of a difference to overall climate. However, if CO2 has a large forcing, then it would make a much bigger difference.

A climate forcing can be positive or negative. Things that contribute to warming (i.e. increasing amount of energy/heat in our atmosphere) have a positive forcing value. Things that contribute to cooling (like pollution that causes clouds to form and reflect sunlight away) have a negative forcing. If we add up all the forcings of all the things that affect climate, then we get the total net forcing on the entire Earth system. The trick here though is to figure out all the things that would have a climate forcing, and then to figure out what that number is and what the uncertainty (possible error) of that number is. If our total net forcing is positive, then we can numerically show how much increased energy is being added into our earth system, and use this number to help develop models to make predictions for the future. If our total net forcing is 0, then it would stand to assume that the things that contribute or take away from global warming have balanced each other out. If our net forcing is less than 0, then it would mean the earth is losing more energy than it is taking in and one would expect a cooling to be occurring. So really, no one knows about the effect and magnitude of anything that could contribute to climate change until they take into acct. how much forcing each thing has.

So what are the climate forcings of various climate affectors and how certain are we to their values? This chart comes from the IPCC 4th Report Summary for Policy Makers (see pg. 4 for better resolution, this pic taken from realclimate.org, but it’s a reprint of the IPCC chart), and shows radiative forcing values of these components since 1750 (start of industrial revolution):

So you can notice a number of things about this chart, there is actually quite a lot of information on it. The RF terms means “Radiative Forcing” terms. Anthropogenic means made by people – things human activity has contributed to the atmosphere. The RF values are the actual forcing values for each term. Spatial scale I think is pretty explanatory, and LOSU stands for “level of scientific understanding” – this term was decided on by the authors of the chapter based on the scientific literature available, and is their assessment of how well we understand the processes and are able to calculate the values of each of these terms.

A little bit on each of the terms:

GHGs: One of the most noticeable things on this chart is that CO2 and other greenhouse gases like methane (CH4), nitros oxide (N2O) and hydrocarbons have a very large contribution to net radiative forcing. Different gases are prevalent in different amounts (you can view their concentrations in the air here (IPCC 4th report, Ch.2)- and have differing radiative capacities, often expressed as global warming potential (GWP) in terms of carbon dioxide equivalents. Carbon dioxide equivalents are how much carbon dioxide it would take to have the equivalent heat absorbing capacity as the other greenhouse gas. I’ll try to make a list here to see but my list making skills in wordpress are somewhat limited:

CO2 – current concentration 380 ppm (parts per million), GWP =1
CH4 – current concentration 1775 ppb (parts per billion), GWP = 20
N2O – current concentration 320 ppb, GWP = 310
CFCs – current concentrations very small, but GWPs can be as high as 8,000

So the radiative forcing takes into acct. the change in concentrations as well as their radiative absorbance capacity in order to compute the amount of climate forcing each has had on our atmosphere over the last 250 years.

Aerosols: Also noticeable are the very large error bars on aerosols. Aerosols have shorter lifetimes so are harder to get an average measure of their concentration. Unlike the GHGs, aerosols are not necessarily evenly spread out through the atmosphere, which complicates our ability to understand their exact contribution. Also, aerosols can participate in a number of mechanisms Aerosols can reflect sunlight back to space. They can also can help to seed cloud formation. Clouds have a high albedo (i.e. they are white), and so reflect light back to space as well. There are also a number of various chemistry reactions that aerosols can take place in the atmosphere that can have a number of effects, not just on climate. Aerosols also are not just one specific molecule like CO2, but can be a number of different chemical compounds from a number of different sources. This pic from NASA shows where aerosols come from pretty well:

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Positioning Systems Before GPS

For thousands of years, speed was limited to a walking pace and landmarks were used to find location. At sea, early navigators limited their voyages to coastal routes to avoid becoming lost. New methods for determining position arose as trade between distant ports increased. Polaris, the North Star, was used to determine north-south distance (latitude) in the northern hemisphere. But mariners also had to find latitude when sailing in the southern hemisphere, and they lacked a method for determining east-west position (longitude). The solution, celestial navigation, required accurate time. In the late 18th century this led to the development of the marine chronometer, an accurate sea-going timepiece. Beginning in the 19th century the U.S. Naval Observatory, the nation’s official timekeeper, provided accurate time for navigators from an array of chronometers.

Sextant
A sextant is used to make precise celestial observations of the Sun, stars, and planets. It measures height, in degrees, above the horizon, which is used with the exact time to calculate position. The sextant shown here was made in the first half of the 19th century. “Shooting the stars” remains a basic skill for the sea-going navigator.

Electronic Innovations
Electronic navigation introduced all-weather capability, ease of use, and eventually, increased accuracy. In the 1930’s radio beacons were used to provide bearings from airfields. During World War II radio navigation systems were developed, the best known being LORAN, or Long Range Aid to Navigation. Positions were determined by the timing of signals received from different LORAN transmitter stations. In the 1960s the Omega system provided worldwide electronic navigation coverage for the first time. These land-based electronic navigation systems were accurate to within several miles, equivalent to celestial navigation. In the mid-1960’s the U.S. Navy’s NAVigation SATellite System (NAVSAT), also known as TRANSIT, was developed to provide more accurate positions for ships and submarines.
TRANSIT Satellite
TRANSIT was the first operational satellite positioning system. Six satellites gave worldwide coverage every 90 minutes and provided positions that were accurate to within 200 meters (660 feet). Positions were obtained by measuring the Doppler shift of the satellite signal. TRANSIT was effective, but it was limited by low accuracy and lack of 24-hour availability. The TRANSIT system operated until 1996.

SI Photo #7B-32766
© Smithsonian Institution.

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