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Increase Metropolitan Police Department Presence in the Shaw Neighborhood, Washington, DC USA
See: www.washingtonpost.com/local/crime/shooting-on-east-capit...
Increases in temperature and precipitation can affect Reindeer pastures in a variety of ways that may influence conditions for reindeer. For instance, increased temperature in autumn can delay both the arrival of snow, as a result of which the reindeer tend to disperse and the herds become less easy to control, and also the formation of thick, safe ice over rivers and lakes, consequently impeding the movement of herds inland. Increased precipitation in winter can result in greater accumulation of snow on winter pastures resulting in a general reduction in the availability of forage.
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This photo has been graciously provided to be used in the GRID-Arendal resources library by: Lawrence Hislop
Increased groundnut (peanut, Arachis hypogaea) seed weight in inter-specific cross derivative line (middle - average nut weight (1.39 g/nut) resulting from crossing cultivated groundnut parent TMV 2 (left - average seed weight 0.30 g) with an amphidiploid produced from a wild species (0.08 g). The amphidiploid parent is TxAG 6 [Arachis batizocoi x (A. cardenasii x A. diogoi)]
Farmers and communities in the Fraser Valley, particularly those most affected by the 2021 atmospheric river, will receive support to increase their resiliency to floods and restore local ecosystems. Learn more: news.gov.bc.ca/29040
Orange Avenue Historic District Boundary Increase
Pascagoula, Mississippi
Listed 09/18/2013
Reference Number: 13000739
The Orange Avenue Historic District Boundary Extension No. 1 is significant under Criterion C for Architecture. The historic district contains locally significant examples of Folk Victorian and Colonial Revival style houses. The buildings reflect regional trends in architectural development extending from the late-nineteenth century to 1945.
National Register of Historic Places Homepage
Orange Avenue Historic District Boundary Increase, Pascagoula, Mississippi, Summary Page
If you want to get lust spells to increase attraction then consult with our spell casting expert and get voodoon sex spells to attract someone. Lust spells and sex magic shows amazing result. You can always seek spell casting advice through our expert and can ask him to cast Lust Spells to Increase Attraction on your behalf. For more information visit us @ www.chantlovespells.com/lust-spells-to-increase-attraction/
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Breast implants to increase bust size are very popular among women of all ages. But did you know that women can also undergo surgery in order to reduce their breast size? There are a few reasons why a woman would want to do this, and below we outline the major ones. In Phoenix, AZ, Dr. Meger offers breast reduction to women looking to go down a few cup sizes in order to improve their quality of life. Dr. Meger is able to remove any excess skin, fat, and skin to sculpt the breasts into what the patient desires. Contrary to popular belief, there is such as thing as breasts that are too big.
1. Relieve Back and Neck Pain
The main reasons why women undergo breast reduction is to relieve back and neck pain. Having large breasts can pull the entire body forward, which causes pain overtime. A good supportive bra can relieve some of this, but the only way to truly experience pain relief is to undergo surgery with Dr. Meger in Arizona.
2. Soothe Skin Irritation
If you have larger-than-average breasts, you know that wearing a bra is a must. Just to lessen the back and neck pain, a bra must be worn at all times. The straps can often cause skin irritation, especially on sensitive areas like near the underarms. Some women even develop a rash on the site where the straps rub the most often. A breast reduction will allow this skin irritation to disappear.
3. Improve Posture
Because large breasts cause you to be pulled forward due to their weight, this can cause you to also have bad posture. It may be painful to stand up straight all the time, as it put unnecessary stress on your back muscles. Smaller breasts are also lighter, which means you will be able to stand up straight and enjoy perfect posture without pain.
Who Is a Candidate?
If you desire a breast reduction for any reason you may be a good candidate for this procedure. You are especially likely to qualify if your quality of life is impacted due to the size of your breasts. At your personalized consultation, Dr. Meger will go over all the pros and cons associated with this procedure to help you make the best decision. He will also discuss the aftercare so you are fully aware of all a breast reduction surgery in Phoenix entails. If you live in Phoenix or Scottsdale, contact the office of Dr. Meger today to schedule your consultation!
The post 3 Ways Breast Reduction Surgery Can Benefit You appeared first on Dr. Robert Meger Board Certified Plastic Surgeon - Phoenix, AZ.
source drmeger.com/breast-reduction-surgery-phoenix/ drmegermdpc.blogspot.com/2018/12/3-ways-breast-reduction-...
Governor Murphy, Senator Bramnick, and Acting Department of Education Commissioner Angelica Allen-McMillan tour Chatham High School and highlight Increased funding for legislative district 21 at Chatham High School on Friday March 25, 2022(Edwin J. Torres/NJ Governor’s Office).
Reims (Gueux) altered the circuit layout to increase top speeds, bought several house around the circuit, knocked them down and changed the circuit to make it faster. Not safer, but faster. Safety simply wasn’t an issue. There was one especially feared corner, the ‘Courbe Gueux’, unofficially known as the ‘Courbe du Calvaire’ or simply ‘Calvary.’ Why? You entered it at over 160mph even during the 1950’s, it had drainage ditches running either side of it, a concrete marshal’s post on the outside of the fastest part and was a death-trap. Make a mistake - you're crucified - you’d almost certainly die. Hence the name. This structure is newly placed here -- because it doesn't show up on the Sept 2013 Google Steet view. So, clearly it has been refurbished and relocated from it's original position further down the track.
How Can Press Release Increase Web Traffic?
Publicity is crucial when running a business, whether your business is located offline or on the Internet. When a business has little or even no budget to promote, "Press Releases" are the most advantageous method to promote your...
blogs.freeinboundmarketingtools.com/uncategorized/how-can...
The Northern Lights are an atmospheric light phenomenon consisting of colorful, dancing and changing patterns in the northern and southern night sky. The northern lights are mostly green, but sometimes red, purple or blue.
The northern lights are caused by charged particles brought by the solar wind hitting the Earth's atmosphere at an altitude of about 80-250 kilometers. When a particle collides with oxygen atoms and nitrogen molecules in the Earth's ionosphere , it gives them additional energy, and the atoms are momentarily excited to a higher energy state. When a particle's excited state is released, the excited energy is released as photons , which is visible as light .
Designation
In the northern hemisphere, the aurora borealis is also internationally called by the Latin name Aurora borealis , or northern fire, in the southern hemisphere, Aurora australis , or southern fire. In most other languages as well, the name of the phenomenon refers to the northern lights or northern brown. Only in Finnish is the phenomenon called "aurora borealis". The name is said to come from the fact that the aurora borealis is believed to have been caused by the fur of the Fire Fox rubbing against the trees. According to another theory, "repo" means the spells of the forest Finns , i.e. the northern lights are the spell fires of the sky.
Occurrence
The source of the aurora's energy is the Sun and the solar wind emanating from it , which continuously blows electrically charged particles towards the Earth. The aurora borealis is caused by the interaction of high-energy, charged particles of the solar wind with molecules in the Earth's atmosphere at an altitude of about 80–600 kilometers. Most aurora borealis occur between 80 and 250 km altitude. Their lower edge is usually sharp, but the upper edge gradually fades into invisibility.
Upon arriving in the Earth's magnetic field , the charged particle that arrived from the Sun begins to bounce, guided by the magnetic field, between the Earth's north and south polar regions along the magnetic path, i.e. the field line. When the particle stops bouncing under the influence of an external force, it plunges down in the direction of the Earth's magnetic field. When a particle collides with oxygen atoms and nitrogen molecules in the Earth's ionosphere , it gives them additional energy, and the atoms are momentarily excited to a higher energy state. When the excited state of the particle is released, the excited energy is released as photons, which is visible as a flash of light. Up to thousands of such can occur simultaneously in an area of a cubic centimeter. Together, all the flashes produce a vast aurora borealis.
Occurrence
The aurora borealis occurs mainly in ring-like areas surrounding the Earth's geomagnetic north and south poles, called aurora borealis. They are located at a distance of about 20 degrees of latitude from the poles. The northern aurora oval runs along the width of the northern part of Fennoscandia , the Svalbards , Iceland , southern Greenland , northern Canada, Alaska and the northern coast of Siberia . The southern aurora borealis is located in an uninhabited area around Antarctica, far from, for example, Australia and New Zealand.
The diameter of the aurora oval increases from time to time, when the aurora borealis moves further from the poles and can be seen further away. An aurora substorm is an event where the point of the aurora oval brightens, the oval becomes wider, and the bright area spreads west and east.
On Karhusaari in the Arctic Ocean, halfway between Fennoscandia and Väippuvuorti, the probability of aurora borealis is at its highest, and they occur there every night. In Finland's Kilpisjärvi, the northern lights occur three nights out of four, at the height of Oulu every fourth night, and in the capital region once a month. In the south, the aurora borealis are usually only visible in the northern sky, but sometimes the aurora borealis can also be seen in southern Finland directly above at the zenith .
Sometimes, during periods of strong solar activity, the northern lights can also be seen in Central and Southern Europe, for example in Vienna on average once a year and in Istanbul about every ten years. At low latitudes, the northern lights can sometimes very rarely be observed during strong solar storms in the sky. The northern lights were observed in 1859 in Hawaii at 21 degrees north latitude and in 1872 in Mumbai , India at 19 degrees north latitude, when they were at their zenith in Istanbul and Athens . The southern northern lights have possibly been observed in 1921 in Samoa 13 degrees south latitude and in 1909 in Singapore just one degree north of the equator .
Because the magnetic poles wander on the Earth's surface, the aurora borealis also moves to different places over the centuries. For example, in 1700 the aurora borealis extended to Oulu and Scotland , as a result of which Europe saw ten times more northern lights than today. In the 11th century, however, the aurora borealis reached deep into the southern parts of Siberia, and the aurora borealis was seen significantly more in China than now, but only a little in Western Europe.
Occurrence periods
The frequency of northern lights varies in several cycles – daily, 27-day cycle, seasonal and 11-year cycle.
Since the aurora oval is asymmetric with respect to the magnetic pole and remains stationary with respect to the Sun, as the Earth rotates, it moves during the day relative to the Earth's surface. In the afternoons, the northern lights are far to the north of Finland, but in the course of the evening they move towards the south and are over northern Finland at 22–23. Towards morning, the northern lights retreat to the north again.
When an area of the Sun is activated, it produces not only a lot of sunspots , but also a lot of charged particles that cause the aurora borealis. Such an active region is turned towards the Earth every 27 days, because in that time the Sun rotates once around its axis. An active northern lights period is often followed by a new active period after 27 days. This usually lasts for a few revolutions of the Sun, until the active point of the Sun fades and the aurora borealis decreases.
The most active time of the northern lights is called the northern lights maximum and the smallest is called the northern lights minimum. During the year, the northern lights have their maxima at the vernal equinox and autumn equinox . The minima, on the other hand, are at the summer solstice and winter solstice . However, their differences are not great, and in the northern lights event, the northern lights are observed every night of the year.
Over a period of several years, the northern lights occur most often when the Sun's magnetic activity is at its highest during its 11-year sunspot period , more precisely in the early years of the waning season.
Longer-lasting or irregular fluctuations have also been observed in the number of sunspots and, at the same time, auroras. Around the years 1640–1715 there was the so-called Maunder minimum , during which there were exceptionally few sunspots and the aurora borealis was hardly visible.
Detection
Place and time of sighting
One of the best places to observe and study the aurora borealis is northern Fennoscandia , as it is more populated and has better transport links than the rest of the aurora borealis area.
The aurora borealis is best observed in clear and dark conditions, when the Sun has set behind the horizon . The air temperature is not important in itself, although in freezing weather the air is often clear and therefore good for spotting the northern lights. The aurora borealis occurs as much during the day as at night, but daylight prevents them from being seen just as well as the aurora borealis at night. In Finland, the best time to observe the northern lights is in the northern sky between 21 and 24, far from the light pollution of urban areas .
Northern Lights substorm
The aurora borealis occurs during the night as regular aurora borealis substorms, or "aurora borealis shows". On a calm night, one occurs only once a night, but sometimes 3 to 5 of them are seen during the night. In the north, the aurora borealis can sometimes be seen from directly below, but in the south it is usually only visible from the side.
An aurora substorm starts early in the evening, when one or more peaceful greenish aurora arcs appear on the northern horizon. The arches stretch across the horizon in the east-west direction, but in the north-south direction their width is only a couple of kilometers. The arcs remain unchanged or drift slowly towards the south. The arc brightens an hour or two after it appears, and red may be visible above it. The previously flat light splits into vertical rays, and the arc often begins to ripple. During half an hour, the arc moves south to the middle sky.
The third act of the northern lights play lasts only 10 minutes, but during that time the northern lights substorm is at its fiercest. In the sky, you can see wide aurora bands and curtains that fold and rotate and move rapidly north and south. In addition to green and red, you can also see blue and violet, sometimes even purple. The climax of the northern lights show is sometimes formed by the so-called aurora corona, which is directly above the viewer and spreads to both the northern and southern sky.
In the fourth act, the northern lights diminish in brightness and calm down, and the sky is covered by a gray-green diffuse mantle or pulsating northern lights. This takes about an hour, after which the whole show can start over, when a new aurora arc appears in the northern sky.
Already after the aurora shows have ended in the morning, there are gauzy aurora surfaces that shine with a steady intensity. During the night, so-called false starts can also occur, where the arc does not develop into a substorm.
Colors
The color of the light of the northern lights depends on the quality of the excited particle and the energy it receives in the collision. The excited states of oxygen atoms make the northern lights green and red, and nitrogen molecules bluish.
Green is the most common color of the northern lights. It is born at an altitude of about 100–300 kilometers. The green forms of aurora borealis are usually clearly distinct and sharp, because the state of excitation that releases the green color is maintained for only a second between the impact and the release of the light. Green auroras sometimes also show yellow, which is due to the mixing effect of other colors or the atmosphere. If the sky is not completely dark, green can appear white because the human eye cannot distinguish color from low brightness.
It takes a good minute for the red state of excitation to be discharged. Because the object of impact moves long distances in that time, the red auroras are softer in shape than the green ones. Red light is also weaker than green. The red auroras are mainly created at an altitude of more than 300 kilometers, because the particles have more room to move there than lower down, and because the low-energy and slow particles that cause the red light collide with oxygen even before they have penetrated lower in the atmosphere. At southern latitudes, the aurora borealis almost always appears as intense red, and not green, as in the north.
Purple or mauve color usually occurs below green. It is caused by very high-energy and fast particles that collide with nitrogen molecules only late, at an altitude of about 80–100 kilometers. This color occurs in strong and fast-moving aurora borealis, and the excited state of the particle only lasts for a fraction of a second. The purple aurora borealis are indeed very strong and sharp.
Blue light from ionized nitrogen molecules can sometimes be seen at the top of the aurora borealis. It is very common in conjunction with all other colors, but is often overshadowed by other, stronger colors. The blue color is best seen in the early evening or late morning, and early fall or late spring.
A single aurora form can change color. At first it may be completely green, but after a while the green color will be replaced by a red and softer form.
Formats
Northern lights come in many different forms. The same Northern Lights can look different depending on whether it is viewed directly from below or from the side. During large eruptions, auroras change rapidly and take many forms.
The different forms of northern lights are divided into belt-like, diffuse (blurry) and radiated. In structure, aurora borealis are homogeneous (even), circular or radial. The state of the aurora borealis can be calm, active (moving or changing), or pulsating.
The most common, longest-lived and first visible form of the Northern Lights is the Northern Lights Arc. It stretches from the eastern horizon to the western horizon, and has a flat lower edge. It is usually green and moves calmly and steadily. It can gradually rise higher. As the aurora activity intensifies, several adjacent arcs can be seen in the sky, and the aurora zone expands at the same time. There may be brightenings in the arc that go east or west. The arcs may also start flashing.
Northern Lights Belt.
The aurora belt is created when the aurora arc begins to activate. The aurora borealis has various folds and other structures, and the lower edge of the shape becomes folded and multi-layered.
Northern Lights Veil.
The aurora borealis is a radial arc or belt when viewed from the side. The rays are streaks of light up to several hundreds of kilometers high that may move along the veil.
The aurora corona or aurora crown is visible directly above the observer. It can sometimes cover the entire sky. The corona is usually green, but sometimes it can be completely red.
Aurora spiral.
The aurora spiral is a twisted belt-like structure. The rotation of the magnetic field is caused by the increased upward electric currents, which twist the field line of the magnetic field. A spiral chain has several simultaneous and adjacent spirals.
A westward advancing attack is not as strongly twisted as a spiral. It heralds the strengthening of the northern lights within half an hour.
A place where there is no aurora light is called a black aurora, because the particles travel back into near space. The black aurora borealis form streaks against the bright green aurora borealis.
North–south arcs occur as magnetic activity increases. [39]
Pulsating northern lights occur when the most powerful phase of the eruption begins to pass. They do not move, but their brightness varies greatly, i.e. they pulse or flash. They can appear as patches or long streaks, and are most common in the early morning hours.
The Omega belt resembles the letter omega of the Greek alphabet. It is often seen in the early hours of the morning. It forms a wide and long arc-shaped circle from north to south, and moves towards the eastern horizon.
The aurora pillars can be seen during calm times of the aurora night. They appear on their own and may remain completely in place for a long time. They can show all the colors of the northern lights, but they are quite dim.
Diffuse Northern lights are a flat and dim blanket of northern lights that often appear in the early hours of the night.
Sounds
It has been claimed that a sound is sometimes produced from the aurora borealis. Sounds are not believed to be produced high in the atmosphere, but according to some researchers, it is possible that some kind of sound is produced in the lower atmosphere in connection with the northern lights.
One possibility is that electromagnetic waves are converted into sound waves in objects located near the viewer. Such objects could be, for example, the listener's hair or clothes, or even some parts of the hearing organs. A recent Finnish study suggests that voices can actually be heard. However, their physical basis is still not completely known.
According to the latest measurement results, the sounds associated with the northern lights are produced only at a height of 70 meters and are audible to the human ear. Unto K. Laine and other researchers from Aalto University recorded the sounds of the aurora borealis with three microphones placed apart from each other and were able to locate their place of origin by comparing the delays caused by the passage of the sounds. The sounds are not created in the northern lights, but the same solar particle eruptions that cause the northern lights can also create sound sources near the earth's surface. The details of how the sounds are made are still a mystery, and they do not occur regularly during the northern lights. The sounds are quiet and barely stand out from the surrounding noise. Those who have heard the sounds have often described them as a distant noise and crackling. Because of this, the researchers consider it possible that there are several ways of generating sounds and that the distances of the sound sources from the surface of the earth can vary.
In Culture and Research
Concepts and beliefs related to the northern lights are abundant in the traditions of the peoples who lived in the regions of the Arctic Circle. According to Finnish folk belief, the northern lights were caused by fire foxes running around in Lapland , when their flanks hit trees or their tails hit the snow. Native Americans in Canada had a similar belief, featuring a caribou deer instead of a fire fox . According to an Inger and Karelian folklore, the aurora borealis is caused by the sunlight-reflecting scales of the Leviathan whale swimming in the Arctic Ocean . In the Kalevala, the aurora borealis is referred to, among other things, as the Gates of the North.
The gates of Pohjola are visible,
The evil guards are shining,
The roofs are colorful
from the man-eating village,
from the sinker of Uroho.
( Old poems of the Finnish people : VII1,679)
The pale green color of the northern lights is often associated with the dead in northern folklore, and for example the Eskimos of Greenland considered the northern lights to be the souls of dead children. The red glow of the northern lights has sometimes been seen as soldiers who died in battle struggle with giants. In central and southern Europe, rare and usually blood-red aurora borealis were seen as heavenly signs of wars, plagues and other upheavals. The Norsemen of the time of the Edda poems also associated the northern lights with battles and the dead in battles, and the Canadian Eskimos in Hudson Bay saw the northern lights as guiding lights to heaven for the souls of those who had died violently. In Finland, the northern lights are also widely believed to predict weather changes, although in different ways in different regions.
Earliest written references
Northern lights are rarely seen in Mediterranean countries, but when they are, they can be very spectacular and can be seen over large areas. They are mentioned in several ancient Greek literary sources. Thale is known for example around 600 BC. having paid attention to them and tried to come up with an explanation for them. It has been speculated that at that time Thales saw the same aurora borealis that was also noticed by the prophet Ezekiel who lived at the same time , whose description of the extraordinary phenomena seen in the sky at the beginning of the book has been explained as referring to the aurora borealis.
History of Scientific Theories
The Greek Aristotle proposed in the 3rd century BC that the aurora borealis would be vapors evaporating from the underground layers that ignite from the heat of the Sun. Even at the beginning of the modern era until the 18th century, the northern lights were explained as reflections of sunlight either from ice crystals in the air in the polar regions or from the waves or salt sprays of the Arctic Ocean. Another popular explanation was the glowing smoke from volcanic eruptions in Iceland .
Swedish physics professor Anders Celsius noticed in 1741 that the compass needle vibrated more than usual during the occurrence of strong aurora borealis. This is how the aurora borealis was first connected to Earth's magnetism. Later in the same century, more evidence was found of connections between the aurora borealis and magnetism. In the 19th century, the aurora borealis began to be considered an electromagnetic phenomenon produced by the atmosphere. For example, Selim Lemström , professor of physics at the University of Helsinki , developed the aurora theory at the end of the 19th century, according to which the aurora borealis is a slow discharge of electric charge accumulations in the atmosphere, while lightning is their rapid discharge.
When the electron was discovered at the end of the 19th century, the Norwegians Carl Strömer and Kristian Birkeland proposed that the aurora borealis is caused by electrons thrown into space by the Sun, which somehow generate a glow of light in the upper layers of the atmosphere. Finally, in the 1920s, it was discovered that the northern lights are created by the impact of the Sun's particles on atmospheric oxygen and nitrogen, which release the energy they receive as light.
In popular culture
The northern lights appear, among others, in Philip Pullman's fantasy novel Kultainen Kompassi , in the films Kätketty kullan maa (1996), Insomnia (2002) and Aurora Borealis (2005) and in the television series Villi Pohjola
The Pakistan Strategy Support Program (PSSP) held the conference, “Increasing Productivity and Unleashing Growth” at the Serena Hotel in Islamabad on May 26-27th, 2012. This conference also marked the final round of the Competitive Grants Program that was launched by PSSP in January 2012 for Pakistani PhD and graduate students studying locally and abroad on economic development issues of Pakistan. The finalists presented in front of the Research Advisory Committee, donor heads, professors and students from local universities. The event also consisted of plenary sessions on Pakistan’s various economic growth issues by renowned academics from all over the world, such as Dr. Jock Anderson, Dr. Regina Birner and Dr. David Spielman.
Increasing female labor participation not only economically and politically empowers women, it also has the potential to substantially increase economic productivity. This is an especially critical issue in Japan where getting more women into the workforce could result in GDP gains of up to 13 percent and help to offset losses caused by the country’s demographic decline. Cooperation and coordination between Japan and the United States could also help to economically empower women elsewhere around the world, especially in developing countries where the potential economic gains are most significant. While increased female labor participation presents a significant opportunity, the structural and social hurdles are enormous – and it is not clear that policy initiatives currently underway in Japan and elsewhere can surmount them. Join the CSIS Simon Chair for a major event on this important topic featuring government officials, NGOs, private sector representatives.
By 2030, water security problems are projected to intensify in southern and eastern Australia, and in Northland and some eastern regions of New Zealand. By 2030, production from agriculture and forestry is projected to decline over much of southern and eastern Australia and over parts of eastern New Zealand, due to increased drought and fire. By 2050, ongoing coastal development and population growth in some areas of Australia and New Zealand are projected to exacerbate risks from sea level rise. Increases in the severity and frequency of storms and coastal flooding are also expected. When parts of Brisbane, Australia, flooded in early 2011, train lines and roads were washed out, leaving many communities isolated, making evacuations extremely difficult and resulting in enormous economic losses.
Photo by Martin Howard / UNISDR Visualizing DRR Group
* New Urus S delivers power increased to 666 CV, matching output of new high performance-oriented Urus Performante
* 4.0 liter V8 twin-turbo engine producing 850 Nm of torque
* Improved acceleration of 0-100 km/h in 3.5 seconds and top speed of 305 km/h
* Six drive modes plus EGO mode for the most versatile, comfortable and sporty Super SUV experience in every environment
* Specific design modifications on the Urus S for a high-performance but sophisticated, lifestyle Lamborghini Super SUV: the most successful model in Lamborghini history
* Urus S and Urus Performante: new two-model line-up for the Lamborghini Super SUV
Waiting for customers. There is an increasing number of small- to medium-scale businesses, largely family owned, helping to nudge Cambodia's economic growth. With investment in the textile and apparel sectors, the country is looking to attract more.
The use of this image is restricted by the ILO and subject to authorization. If you wish to use this photo, please send a request to multimedia@ilo.org specifying the reference number, its intended use, the media you represent, your postal address, email and phone number.
Credit: Cassidy K. / ILO
Date: 2004-05-25
Country : Cambodia
ILO PHOTO reference ILO photo cn1904
Country : Cambodia
Date : 25/05/2004
Copyright : Cassidy K. / ILO
The Pakistan Strategy Support Program (PSSP) held the conference, “Increasing Productivity and Unleashing Growth” at the Serena Hotel in Islamabad on May 26-27th, 2012. This conference also marked the final round of the Competitive Grants Program that was launched by PSSP in January 2012 for Pakistani PhD and graduate students studying locally and abroad on economic development issues of Pakistan. The finalists presented in front of the Research Advisory Committee, donor heads, professors and students from local universities. The event also consisted of plenary sessions on Pakistan’s various economic growth issues by renowned academics from all over the world, such as Dr. Jock Anderson, Dr. Regina Birner and Dr. David Spielman.
The Pakistan Strategy Support Program (PSSP) held the conference, “Increasing Productivity and Unleashing Growth” at the Serena Hotel in Islamabad on May 26-27th, 2012. This conference also marked the final round of the Competitive Grants Program that was launched by PSSP in January 2012 for Pakistani PhD and graduate students studying locally and abroad on economic development issues of Pakistan. The finalists presented in front of the Research Advisory Committee, donor heads, professors and students from local universities. The event also consisted of plenary sessions on Pakistan’s various economic growth issues by renowned academics from all over the world, such as Dr. Jock Anderson, Dr. Regina Birner and Dr. David Spielman.
www.youtube.com/watch?v=f42MLoLbnnQ&feature=related
Killing Joke are an English post-punk band formed in October 1978 in Notting Hill, London, England; other sources report the band formed in early 1979. Founding members Jaz Coleman (vocals, keyboards) and Geordie Walker (guitars) have been the only constant members.
A key influence on industrial rock, their early music was described by critics Stephen Thomas Erlewine and John Dougan as "quasi-metal ... dancing to a tune of doom and gloom," which gradually evolved over the years, incorporating elements of electronic music, synth-pop, gothic rock, and alternative rock,though always emphasising Coleman's "savagely strident vocals."
Finding modest commercial success, Killing Joke have influenced many later bands, such as Nirvana, Ministry, Amen, Lamb of God, Nine Inch Nails, Porcupine Tree, Napalm Death, Behemoth, Amebix, Big Black, Opeth, Murderdolls, Godflesh, Dead by April, Tool, Prong, Metallica, Franz Ferdinand, Primus, Jane's Addiction, Soundgarden, Foo Fighters, Faith No More, Blacklist, Shihad, Pitchshifter, Das Oath, Rammstein and Korn, all of whom have at some point cited some debt of gratitude to Killing Joke
The Sonisphere Festival is a touring music festival which takes place across Europe between June and August. The festival is owned and promoted by Kilimanjaro Live with financial backing from AEG. It has hosted heavy metal bands such as Iron Maiden, Metallica, Mötley Crüe, and Slayer.
The idea for Sonisphere was first conceived when Stuart Galbraith was working for Live Nation, the organisers of Download Festival. The plan was to hold a series of events that would "translate into other territories". The event did not begin to materialize, however, until Galbraith left Live Nation for the events company Kilimanjaro Live.
Galbraith gained the support of the metal band Metallica, who were claimed to have helped curate the festival for later years; however, rumours were denied of Metallica signing a multi-million pound deal promising the band to headlining the festival for three years. The first run of festivals ran throughout the summer of 2009 at six venues, returning in 2010 with 11 venues.
Galbraith's plans for future festivals consist of increasing the number of festivals, making the event global rather than local to Europe, expanding the UK event into a 3-day festival, and increasing the UK capacity from 40,000 to 60,000 attendees
The EU is dedicated to increasing its involvement with young people in the Southern Mediterranean region, as well as assisting partner countries in providing greater possibilities for young people through education, vocational training, job creation, and SME support. It also promotes youth policy exchanges among Southern Mediterranean countries through existing regional cooperation fora.
Senator Nancy Spence speaking to SR11-004 | Opposition to Tax Increases. To read the resolution click below: www.leg.state.co.us/clics/clics2011a/csl.nsf/fsbillcont/6...
For more information visit www.ColoradoSenateNews.com.
Increasing distance is the holy grail of golf training. Nothing increases distance like rotational power.
Increasing the availability of drinking water in the rural areas of Ferghana Valley - educational component "Water Week".
Photos: East European Democratic Centre
Zwiększenie dostępności do wody pitnej na terenie Kotliny Fergańskiej - komponent edukacyjny "Tydzień Wody".
Zdjęcia: Stowarzyszenie Wschodnioeuropejskie Centrum Demokratyczne
Although the engine power had been slightly increased moving from the Mk I to Mk II Spitfire, the first major update of the aircraft to see squadron service - and incidentally become the most produced single variant - was the Spitfire Mark V. This introduced the Rolls Royce Merlin 45 series of engines, optimised for low or high flight hence the LF designation of EE602. The fuselage was strengthened internally and the wing redesigned more than once: production ranged from the original "a" wing with 4 0.303 Browning machine guns on each side through the far more numerous "b" wing designed for a single 20mm cannon and retaining the two outboard Brownings to the universal "c" wing that could hold two 20mm cannon or one plus the Brownings. The stub outboard of the 20mm on this Spitfire shows it to have the last wing design. Spitfire Vs restored equality with the Me109F but proved inferior to the FW190A, requiring further development of the Merlin to again restore the balance. EE602 is shown at the end of its landing roll following participation in the Big Wing finale of Duxford's 2024 Battle of Britain Airshow: the pilot has already retracted the flaps so they don't occlude the airflow through the radiators.
This is a photograph from the 3rd annual running of the Trim AC 10 Mile Road Race and Fun Run which was held in Trim, Co. Meath, Ireland on Sunday 5th February 2017 at 12:00. The race attracted over 1,200 participants which shows a 100% increase on last year's participation. The event shows growth year on year mirroring the growing popularity of the race. The race started on the Trim/Athboy road on the town's ring road and proceded to take an anti-clockwise loop out towards the village of Dunderry and townland of Kilbride before returning back to the Trim Industrial Estate for the finish. The route is held on quiet country roads with some hills at 3, 6, 8 mile segments.
Our full set of photos from mile 1 and the finish are at: www.flickr.com/photos/peterm7/albums/72157679859593016
The weather for this year's race was perfect for racing. There was a hard frost overnight but this brought clear bright skies and crisp air. There was no real wind to speak of.
Waterstops were provided at the 4.5 and 7 mile marks on the course. All access roads were well stewarded. The event was sponsored by Bewleys 1840 and many local business establishments. Credit must go to the Trim AC team for their flawless organisation. If the first three years of this year are anything to go on then this race will continue to grow. For runners around the North Leinster area this 10 mile race serves as a perfect training progress stepping stone to the Bohermeen Half Marathon which will take place in March 2016 and is located only 15 minutes drive from Trim.
USEFUL LINKS
Our Flickr photographs from the 2016 race: www.flickr.com/photos/peterm7/sets/72157664217257512
Our Flickr photographs from the 2015 race: www.flickr.com/photos/peterm7/albums/72157650166189770
Boards.ie Discussion Thread on the 2017 race: www.boards.ie/vbulletin/showthread.php?t=2057673405
10 Mile Road Race Timelapse Video of the Route: www.youtube.com/watch?v=4Jp84CrctQM
USING OUR PHOTOGRAPHS - A QUICK GUIDE AND ANSWERS TO YOUR QUESTIONS
Can I use these photographs directly from Flickr on my social media account(s)?
Yes - of course you can! Flickr provides several ways to share this and other photographs in this Flickr set. You can share directly to: email, Facebook, Pinterest, Twitter, Tumblr, LiveJournal, and Wordpress and Blogger blog sites. Your mobile, tablet, or desktop device will also offer you several different options for sharing this photo page on your social media outlets.
BUT..... Wait there a minute....
We take these photographs as a hobby and as a contribution to the running community in Ireland. We do not charge for our photographs. Our only "cost" is that we request that if you are using these images: (1) on social media sites such as Facebook, Tumblr, Pinterest, Instagram, Snapchat, Twitter,LinkedIn, Google+, VK.com, Vine, Meetup, Tagged, Ask.fm,etc or (2) other websites, blogs, web multimedia, commercial/promotional material that you must provide a link back to our Flickr page to attribute us or acknowledge us as the original photographers.
This also extends to the use of these images for Facebook profile pictures. In these cases please make a separate wall or blog post with a link to our Flickr page. If you do not know how this should be done for Facebook or other social media please email us and we will be happy to help suggest how to link to us.
I want to download these pictures to my computer or device?
You can download this photographic image here directly to your computer or device. This version is the low resolution web-quality image. How to download will vary slight from device to device and from browser to browser. Have a look for a down-arrow symbol or the link to 'View/Download' all sizes. When you click on either of these you will be presented with the option to download the image. Remember just doing a right-click and "save target as" will not work on Flickr.
I want get full resolution, print-quality, copies of these photographs?
If you just need these photographs for online usage then they can be used directly once you respect their Creative Commons license and provide a link back to our Flickr set if you use them. For offline usage and printing all of the photographs posted here on this Flickr set are available free, at no cost, at full image resolution.
Please email petermooney78 AT gmail DOT com with the links to the photographs you would like to obtain a full resolution copy of. We also ask race organisers, media, etc to ask for permission before use of our images for flyers, posters, etc. We reserve the right to refuse a request.
In summary please remember when requesting photographs from us - If you are using the photographs online all we ask is for you to provide a link back to our Flickr set or Flickr pages. You will find the link above clearly outlined in the description text which accompanies this photograph. Taking these photographs and preparing them for online posting takes a significant effort and time. We are not posting photographs to Flickr for commercial reasons. If you really like what we do please spread the link around your social media, send us an email, leave a comment beside the photographs, send us a Flickr email, etc. If you are using the photographs in newspapers or magazines we ask that you mention where the original photograph came from.
I would like to contribute something for your photograph(s)?
Many people offer payment for our photographs. As stated above we do not charge for these photographs. We take these photographs as our contribution to the running community in Ireland. If you feel that the photograph(s) you request are good enough that you would consider paying for their purchase from other photographic providers or in other circumstances we would suggest that you can provide a donation to any of the great charities in Ireland who do work for Cancer Care or Cancer Research in Ireland.
Let's get a bit technical: We use Creative Commons Licensing for these photographs
We use the Creative Commons Attribution-ShareAlike License for all our photographs here in this photograph set. What does this mean in reality?
The explaination is very simple.
Attribution- anyone using our photographs gives us an appropriate credit for it. This ensures that people aren't taking our photographs and passing them off as their own. This usually just mean putting a link to our photographs somewhere on your website, blog, or Facebook where other people can see it.
ShareAlike – anyone can use these photographs, and make changes if they like, or incorporate them into a bigger project, but they must make those changes available back to the community under the same terms.
Above all what Creative Commons aims to do is to encourage creative sharing. See some examples of Creative Commons photographs on Flickr: www.flickr.com/creativecommons/
I ran in the race - but my photograph doesn't appear here in your Flickr set! What gives?
As mentioned above we take these photographs as a hobby and as a voluntary contribution to the running community in Ireland. Very often we have actually ran in the same race and then switched to photographer mode after we finished the race. Consequently, we feel that we have no obligations to capture a photograph of every participant in the race. However, we do try our very best to capture as many participants as possible. But this is sometimes not possible for a variety of reasons:
►You were hidden behind another participant as you passed our camera
►Weather or lighting conditions meant that we had some photographs with blurry content which we did not upload to our Flickr set
►There were too many people - some races attract thousands of participants and as amateur photographs we cannot hope to capture photographs of everyone
►We simply missed you - sorry about that - we did our best!
You can email us petermooney78 AT gmail DOT com to enquire if we have a photograph of you which didn't make the final Flickr selection for the race. But we cannot promise that there will be photograph there. As alternatives we advise you to contact the race organisers to enquire if there were (1) other photographs taking photographs at the race event or if (2) there were professional commercial sports photographers taking photographs which might have some photographs of you available for purchase. You might find some links for further information above.
Don't like your photograph here?
That's OK! We understand!
If, for any reason, you are not happy or comfortable with your picture appearing here in this photoset on Flickr then please email us at petermooney78 AT gmail DOT com and we will remove it as soon as possible. We give careful consideration to each photograph before uploading.
I want to tell people about these great photographs!
Great! Thank you! The best link to spread the word around is probably http://www.flickr.com/peterm7/sets
The Pakistan Strategy Support Program (PSSP) held the conference, “Increasing Productivity and Unleashing Growth” at the Serena Hotel in Islamabad on May 26-27th, 2012. This conference also marked the final round of the Competitive Grants Program that was launched by PSSP in January 2012 for Pakistani PhD and graduate students studying locally and abroad on economic development issues of Pakistan. The finalists presented in front of the Research Advisory Committee, donor heads, professors and students from local universities. The event also consisted of plenary sessions on Pakistan’s various economic growth issues by renowned academics from all over the world, such as Dr. Jock Anderson, Dr. Regina Birner and Dr. David Spielman.
Holdibona Village, Rajshahi District, Bangladesh
Surovi Mardi (6- right) and Ria Mardi (4) sit during a womens group meeting in Holdibona Village, Bangladesh on January 18, 2013.
"Anheuser-Busch InBev Increases Offer for Rival SABMIller" by CHAD BRAY via NYT t.co/UFKRWlNLIL (via Twitter twitter.com/felipemassone/status/653571340432240641)
Small businesses throughout British Columbia will soon have access to new funding to support increased costs due to crime and vandalism, and to prevent further crime. Learn more: news.gov.bc.ca/29289
The Pakistan Strategy Support Program (PSSP) held the conference, “Increasing Productivity and Unleashing Growth” at the Serena Hotel in Islamabad on May 26-27th, 2012. This conference also marked the final round of the Competitive Grants Program that was launched by PSSP in January 2012 for Pakistani PhD and graduate students studying locally and abroad on economic development issues of Pakistan. The finalists presented in front of the Research Advisory Committee, donor heads, professors and students from local universities. The event also consisted of plenary sessions on Pakistan’s various economic growth issues by renowned academics from all over the world, such as Dr. Jock Anderson, Dr. Regina Birner and Dr. David Spielman.
Impress Your partner- goo.gl/4vlHF7
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Here is what the piece looks like as you finish the last of the rows where the piece is increasing in width.
Photo of a man inflating the tyres on his bicycle using a pump before cycling on the road. This image is licensed under the Attribution Creative Commons License for you to use, though we do ask that you please credit www.tredz.co.uk/
This is how a street scene in bright sunlight would look to someone who has increased light sensitivity.
Photo: ICEH.
Published in: Community Eye Health Journal Vol. 25 No. 77 2012 www.cehjournal.org
Increase C. Bosworth House in the Dundee Township Historic District in West Dundee (c. 1845, remodeled c. 1885). He was one of Dundee's first merchants and land speculators, arriving in 1838. The first Bosworth store was probably built on this site. Bosworth's farm outside of town later became the Country Tea Room. Bosworth was also president of the First National Bank in Elgin. He was on the board of trustees at the University of Chicago and the Northern Hospital for the Insane. He was an Alderman and Supervisor in Elgin.
British Columbia’s Rental Housing Task Force is recommending the provincial government change the annual allowable rent increase formula to ease pressure on renters.
Learn more: news.gov.bc.ca/releases/2018MAH0126-001842