1. General Tours Its Time To Go Thailand - Bangkok And Phuket Name Email Home General Tours The Orient Its Time to Go Thailand Bangkok and Phuket. Its Time to Go Thailand - Bangkok and Phuket http://tmsyn.wc.ask.com/r?t=an&s=hb&uid=24312681243126812&sid=343126

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11. Mole Salamander general information about this salamander that spends much of its time underground. http://www.npwrc.usgs.gov/narcam/idguide/ambytalp.htm

Northern Prairie Wildlife Research Center Home Site Map About ... Web Help Mole Salamander, Ambystoma talpoideum Return to checklist: family/species species only The Mole Salamander is one of the smaller members of the family Ambystomatidae, attaining lengths around 4 inches. The general coloration varies from a dark brown to black background color with white, gray, or silver flecking. They are a burrowing salamander and are found primarily in lowlands and valleys lowland areas where the ground is moist making it suitable for burrowing. Because of their burrowing habits they are rarely seen outside of the breeding season. They breed from Dec. to Feb.(during the winter along the coastal plain, late winter/early spring in the colder areas of their range), in shallow ponds and flooded depressions, usually after heavy rains. Females can lay a few hundred eggs, but they are laid in small clusters of about 20. Neoteny, when larvae become sexually mature but do not metamorphose and leave the pond, is not uncommon in this species. Return to checklist: family/species species only U.S. Department of the Interior

12. Orbits In Strongly Curved Spacetime In strong gravitational fields, general Relativity predicts orbits will lingernear the energy peak for an increasingly long time, while its continued http://www.fourmilab.ch/gravitation/orbits/

Orbits in Strongly Curved Spacetime Sorryit appears your browser doesn't understand Java applets. Introduction The display above shows, from three different physical perspectives, the orbit of a low-mass test particle , the small red circle, around a non-rotating black hole (represented by a grey circle in the panel at the right, where the radius of the circle is the black hole's gravitational radius , or event horizon . Kepler's laws of planetary motion, grounded in Newton's theory of gravity, state that the orbit of a test particle around a massive object is an ellipse with one focus at the centre of the massive object. But when gravitational fields are strong, as is the case for collapsed objects like neutron stars and black holes, Newton's theory is inaccurate; calculations must be done using Einstein's theory of General Relativity. In Newtonian gravitation, an orbit is always an ellipse. As the gravitating body becomes more massive and the test particle orbits it more closely, the speed of the particle in its orbit increases without bound, always balancing the gravitational force. For a black hole, Newton's theory predicts orbital velocities greater than the speed of light, but according to Einstein's Special Theory of Relativity, no material object can achieve or exceed the speed of light. In strong gravitational fields, General Relativity predicts orbits drastically different from the ellipses of Kepler's laws. This page allows you to explore them. The Orbit Plot The panel at the right of the applet shows the test mass orbiting the black hole, viewed perpendicular to the plane of its orbit. The path of the orbit is traced by the green line. After a large number of orbits the display will get cluttered and may start to flash; just click the mouse anywhere in the right panel to erase the path and start over. When the test mass reaches its greatest distance from the black hole, a yellow line is plotted from the centre of the black hole to that point, the

13. Springer - Your Publishers Of Books, Journals, And Electronic Media An international journal concerned with the broadest range of dynamical astronomy and its applications, as well as with peripheral fields. The papers published include treatments of the mathematical, physical and computational aspects of planetory theory, lunar theory, general and special perturbation theory, ephemerides, resonance theory, geodesy of the Earth and the planets, dynamics, the 3body problem, the N-body problem, space mechanics, ring systems, galactic dynamics, reference frames, time, relativity, nongravitational forces, computer methods, computer languages for analytical developments, and database management. http://www.wkap.nl/journalhome.htm/0923-2958

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14. Arnold Arboretum - Bonsai - Introduction Housed at the Arnold Arboretum of Harvard University. An illustrated history of the collection, its founder, the principal type of Hinoki in the collection, and the general care given to the trees at the current time. http://www.arboretum.harvard.edu/plants/bonsai/intro.html

Larz Anderson Bonsai Introduction Beginnings Japanese Connection The Bonsai Hinoki Cypress ... Visitor's Information See also Map of the Grounds The Larz Anderson Bonsai Collection The long history of growing plants in containers is documented in the writing and painting of various ancient civilizations, including the Egyptian, the Hindu, the Greek, and the Roman. But it appears that the ancient Chinese were the first to miniaturize trees for ornamental purposes, around A.D. 200. From China, the practice spread to Japan, probably during the Heian period (782-1185). During the peaceful and prosperous Tokugawa period of Japanese history (1603-1867), landscape gardening attained new importance. Many of the great Japanese gardens that exist today were established then, when the cultivation of native Japanese plants such as azaleas and maples was a pastime of the wealthy. Growing dwarf plants in containers was also popular, but by modern bonsai standards the container plants of the Tokugawa period were too large and their containers too deep. In this period, the term used for dwarf potted trees was hachi-no-ki , meaning "a tree in a pot." The term

15. Daylight Saving Time Daylight Saving Time, Its History And Why We Use It Daylight Saving time, for the US and its territories, is NOT observed in Hawaii,American Samoa, Guam, Puerto Rico, the Virgin Islands, the Eastern time http://tf.nist.gov/general/daylightsavingtime.html

Adapted with permission from an online article by Bob Aldrich, California Energy Commission Introduction Daylight Saving Time begins for most of the United States at 2 a.m. on the first Sunday of April. Time reverts to standard time at 2 a.m. on the last Sunday of October. (Note that it is Daylight Saving (singular) Time, NOT Daylight Saving S Time. We are saving daylight, so it is singular and not plural.) Year DST Begins 2 a.m. DST Ends 2 a.m. April 2 October 29 April 7 October 27 April 6 October 26 April 5 October 25 April 4 October 31 April 2 October 29 April 1 October 28 April 7 October 27 April 6 October 26 April 4 October 31 Daylight Saving Time, for the U.S. and its territories, is NOT observed in Hawaii, American Samoa, Guam, Puerto Rico, the Virgin Islands, the Eastern Time Zone portion of the State of Indiana, and by most of Arizona (with the exception of the Navajo Indian Reservation in Arizona). Other parts of the world observe Daylight Saving Time as well. While European nations have been taking advantage of the time change for decades, in 1996 the European Union (EU) standardized a EU-wide "summertime period." The EU version of Daylight Saving Time runs from the last Sunday in March through the last Sunday in October. During the summer, Russia's clocks are two hours ahead of standard time. During the winter, all 11 of the Russian time zones are an hour ahead of standard time. During the summer months, Russian clocks are advanced another hour ahead. With their high latitude, the two hours of Daylight Saving Time really helps to save daylight. In the southern hemisphere where summer comes in December, Daylight Saving Time is observed from October to March. Equatorial and tropical countries (lower latitudes) don't observe Daylight Saving Time since the daylight hours are similar during every season, so there's no advantage to moving clocks forward during the summer.

16. About Thailand general information for those who want to visit Thailand for the first time or just want to know its most important features. http://thai95e.tripod.com

setAdGroup('67.18.104.18'); var cm_role = "live" var cm_host = "tripod.lycos.com" var cm_taxid = "/memberembedded" Search: Lycos Tripod Aeon Flux Share This Page Report Abuse Edit your Site ... Next "The real voyage of discovery consists not in seeking new landscapes but in having new eyes". Welcome to Thailand, the land of smiles click here for the Italian version This website has two purposes. But it is mainly meant to pay homage to Thailand and to the Thai people. And it is also meant to be a reference for all those who are planning to organize a trip to Thailand to let them have the basic information, and maybe even an "invitation" to visit and discover this beautiful country. Bangkok Rome How is the weather in Thailand now? email me for comments and suggestions visit my personal website this page has been visited times Directory of fine websites on Thailand [ Home ] why to Thailand before leaving meteo the first time ... on the net

17. Publishers Of Time And Frequency Software The time and frequency software from each publisher have been categorized as follows Company, ACTS, its, Platform. 1 Ace Software, X, Windows http://tf.nist.gov/general/softwarelist.htm

Home Welcome Current Time Exhibits ... Opportunities Radio Stations WWV WWVH WWVB Services Computer Time Telephone Time Calibrations Seminars ... Survey Results Standards NIST-F1 Space Clock History Time Transfer GPS Digital Time Two Way Metrology Phase Noise Tutorial Research Ion Storage Optical Chip-Scale Atomic Clocks Data Time Scale GPS LORAN-C WWVB Publishers of Time and Frequency Software The following list of links to publishers of time and frequency software may be incomplete, and inclusion on the list does not imply endorsement by NIST. The publishers are listed alphabetically. Send corrections or additions to: timeinfo@boulder.nist.gov The time and frequency software from each publisher have been categorized as follows: ACTS Automated Computer Time Service (via analog modem) ITS Internet Time Service Company ACTS ITS Platform #1 Ace Software X Windows 40Tude Software X Windows 4D Keeper Group X Windows Acrovista X Windows Apple Computer X Macintosh Atom Time X Windows Beagle Software X X Windows Bytefusion Ltd. X Windows Dillobits X Windows Thinking Man Software X Windows eXport Ventures Corp X OS/400 Express Computing X Windows Getware X Windows Green Parrots Software X Windows Gregory Braun X Windows Greyware Automation Products X Windows, Linux, UNIX, FreeBSD

18. General Relativity In The Global Positioning System Also, because the earth and its satellites are in free fall, gravitational frequency In general Relativity (GR), coordinate time, such as is expressed http://www.phys.lsu.edu/mog/mog9/node9.html

General relativity in the global positioning system Neil Ashby University of Colorado n_ashby@mobek.colorado.edu The Global Position System (GPS) consists of 24 earth-orbiting satellites, each carrying accurate, stable atomic clocks. Four satellites are in each of six different orbital planes, of inclination 55 degrees with respect to earth's equator. Orbital periods are 12 hours (sidereal), so that the apparent position of a satellite against the background of stars repeats in 12 hours. Clock-driven transmitters send out synchronous time signals, tagged with the position and time of the transmission event, so that a receiver near the earth can determine its position and time by decoding navigation messages from four satellites to find the transmission event coordinates, and then solving four simultaneous one-way signal propagation equations. Conversely, gamma-ray detectors on the satellites could determine the space-time coordinates of a nuclear event by measuring signal arrival times and solving four one-way propagation delay equations. Apart possibly from high-energy accelerators, there are no other engineering systems in existence today in which both special and general relativity have so many applications. The system is based on the principle of the constancy of c in a local inertial frame: the Earth-Centered Inertial or ECI frame. Time dilation of moving clocks is significant for clocks in the satellites as well as clocks at rest on earth. The weak principle of equivalence finds expression in the presence of several sources of large gravitational frequency shifts. Also, because the earth and its satellites are in free fall, gravitational frequency shifts arising from the tidal potentials of the moon and sun are only a few parts in

19. Touché Fencing Club Club meeting regularly on Wednesdays. Details about the club and its equipment, about fencing in general along with meeting times and contact details. http://mysite.wanadoo-members.co.uk/touchefencingclubmk/

20. MAGIC Throught Two MILLENNIA time Dilation or the Gravitational Redshift. Both Special and general If the other clock is placed in a plane flying Eastwards, its speed will add to http://www.upscale.utoronto.ca/GeneralInterest/Key/relgen.htm

To the MAGIC Homepage MAGIC through two MILLENNIA GENERAL RELATIVITY - a primer Gravity and Time Gravity and Space Bending of Light in a Gravitational Field Experimental Verification Gravity and Time. Consider three clocks. Clocks 1 and 2 are mounted on a rotating disk, with clock 1 exactly at the centre, and clock 2 fixed on the rim, and clock 3 is sitting at rest with respect to the centre of the disk. Note that the disk exerts a force on clock 2 which forces it to follow a circular path; since, without this force, clock 2 would move in a straight line, it is clear that the force and the resultant acceleration are both directed towards the centre of the disk. Clocks 1 and 3 are not moving relative to one another (there is some rotation involved, but their relative position in space does not change with time); thus, as far as Special Relativity is concerned, they keep the same time. However, clock 2 is moving with respect to clock 3; thus clock 2 is running slow as seen by clock 3. Since clocks 1 and 3 keep the same time, this means that clock 2 runs slow compared to clock 1, even though clocks 1 and 2 have no relative translatory motion. (Note that, since clock 2 is not in an inertial frame, Special Relativity does not make any statement about its timekeeping - this is a new effect) . Finally, consider a clock situated on the disk somewhere between clocks 1 and 2; the acceleration of such a clock is less than that of clock 2, and since it is also moving more slowly than clock 2, it is running less slowly.

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