Uniserve Internet, home phone and web products are simple to use, highly reliable, and give you unlimited access. We’re talking no contracts and no monthly caps on usage, with 24-hour support care, 7 days a week.High Frequency Active Auroral Research Program. For the live CD/DVD package by Muse named after the project, see HAARP (album). Southeast Alaska (in 2011, combined into one Alaska stock report): 2009 2007 2006 1998; Harp Seal. Western North Atlantic: 2013. HAMP versus HARP: Which is right for you? The HARP program expires on September 30, 2017. HARP Mortgage Program Overview: A HARP refinance only applies to Fannie Mae or Freddie Mac mortgage. The homeowner must be able to afford the new lower. HARP Loan Limits Alabama Alaska Arizona Arkansas California Colorado. View and map all Fayetteville, GA schools. Before school program After school program Dress code. Sara Harp Minter Elementary School. 1650 Hwy 85 South, Fayetteville. Harpsicle Harp Company; STRINGS; ACCESSORIES; BOOKS & PDFs. Harp Essentials Program. Metal Adjustable Floor Stand for Harpsicle and Grand Harpsicle Harps. The Home Affordable Refinance Program (HARP) is a government program that helps homeowners who are unable to refinance due to a decline in their home’s value. The Home Affordable Refinance Program (HARP). Here are some of the most important changes to HARP since the program began: (Image: HSH.com) Am I eligible for HARP 2.0 despite my recent bankruptcy? According to Fannie Mae. The Home Affordable Refinance Program (HARP). THE HARP CONNECTION NATIONAL TEACHER DIRECTORY. ALASKA: ALASKA: No information available ARIZONA. Program Director, Harp Department, Bob Jones University. The High Frequency Active Auroral Research Program (HAARP) was an ionospheric research program jointly funded by the U. S. Navy, the University of Alaska. The IRI is used to temporarily excite a limited area of the ionosphere. Other instruments, such as a VHF and a UHFradar, a fluxgatemagnetometer, a digisonde (an ionospheric sounding device), and an induction magnetometer, were used to study the physical processes that occur in the excited region. Work on the HAARP Station began in 1. The current working IRI was completed in 2. BAE Systems Advanced Technologies. It was reported to be temporarily shut down in May 2. In May 2. 01. 4, it was announced that the HAARP program would be permanently shut down later in the year. Such theorists blamed the program for causing earthquakes, droughts, storms and floods, diseases such as Gulf War syndrome and chronic fatigue syndrome, the 1. TWA Flight 8. 00, and the 2. Columbia. Commentators and scientists say that proponents of these theories are . In July 2. 01. 3, HAARP program manager James Keeney said, . The University plan to make the facilities available for researchers on a pay- per- use basis. The signal may be pulsed or continuous. Then, effects of the transmission and any recovery period can be examined using associated instrumentation, including VHF and UHF radars, HF receivers, and optical cameras. According to the HAARP team, this will advance the study of basic natural processes that occur in the ionosphere under the natural but much stronger influence of solar interaction, and how the natural ionosphere affects radio signals. This will enable scientists to develop methods to mitigate these effects to improve the reliability or performance of communication and navigation systems which would have a wide range of both civilian and military uses, such as an increased accuracy of GPS navigation and advances in underwater and underground research and applications. This may lead to improved methods for submarine communication or an ability to remotely sense and map the mineral content of the terrestrial subsurface, and perhaps underground complexes, of regions or countries, among other things. The current facility lacks range to be used in regions like the Middle East, according to one of the researchers involved, but the technology could be put on a mobile platform. Many other universities and educational institutions of the United States were involved in the development of the project and its instruments, namely the University of Alaska Fairbanks, Stanford University, Penn State University (ARL), Boston College, UCLA, Clemson University, Dartmouth College, Cornell University, Johns Hopkins University, University of Maryland, College Park, University of Massachusetts Amherst, MIT, Polytechnic Institute of New York University, and the University of Tulsa. The project's specifications were developed by the universities, who continued to play a major role in the design of future research efforts. According to HAARP's original management, the project strove for openness, and all activities were logged and publicly available. Scientists without security clearances, even foreign nationals, were routinely allowed on site. The HAARP facility regularly (once a year on most years according to the HAARP home page) hosted open houses, during which time any civilian could tour the entire facility. In addition, scientific results obtained with HAARP were routinely published in major research journals (such as Geophysical Research Letters, or Journal of Geophysical Research), written both by university scientists (American and foreign) and by U. S. Department of Defense research lab scientists. Each summer, the HAARP held a summer school for visiting students, including foreign nationals, giving them an opportunity to do research with one of the world's foremost research instruments. Research. Essentially a transition between the atmosphere and the magnetosphere, the ionosphere is where the atmosphere is thin enough that the sun's X- rays and UV rays can reach it, but thick enough that there are still enough molecules present to absorb those rays. Consequently, the ionosphere consists of a rapid increase in density of free electrons, beginning at ~7. Various aspects of HAARP can study all of the main layers of the ionosphere. The profile of the ionosphere is highly variable, changing constantly on timescales of minutes, hours, days, seasons, and years. This profile becomes even more complex near Earth's magnetic poles, where the nearly vertical alignment and intensity of earth's magnetic field can cause physical effects like aurorae. The ionosphere is traditionally very difficult to measure. Balloons cannot reach it because the air is too thin, but satellites cannot orbit there because the air is still too thick. Hence, most experiments on the ionosphere give only small pieces of information. HAARP approaches the study of the ionosphere by following in the footsteps of an ionospheric heater called EISCAT near Troms. There, scientists pioneered exploration of the ionosphere by perturbing it with radio waves in the 2. HAARP performs the same functions but with more power and a more flexible and agile HF beam. Some of the main scientific findings from HAARP include. Generating very low frequency radio waves by modulated heating of the auroral electrojet, useful because generating VLF waves ordinarily requires gigantic antennas. Generating weak luminous glow (measurable, but below that visible with a naked eye) from absorbing HAARP's signal. Generating extremely low frequency waves in the 0. Hz range. These are next to impossible to produce any other way, because the length of a transmit antenna is dictated by the wavelength of the signal it must emit. Generating whistler- mode VLF signals that enter the magnetosphere and propagate to the other hemisphere, interacting with Van Allen radiation belt particles along the way. VLF remote sensing of the heated ionosphere. Research at the HAARP included. Plasma line observations. Stimulated electron emission observations. Gyro frequency heating research. Spread F observations (blurring of ionospheric echoes of radio waves due to irregularities in electron density in the F layer)High velocity trace runs. Airglow observations. Heating induced scintillation observations. VLF and ELF generation observations. The presence of multiple radars spanning both HF and VHF bands allows scientists to make comparative measurements that may someday lead to an understanding of the processes that form these elusive phenomena. Research into extraterrestrial HF radar echos: the Lunar Echo experiment (2. This is a high power, high- frequency phased array radio transmitter with a set of 1. The IRI is used to temporarily energize a small portion of the ionosphere. The study of these disturbed volumes yields important information for understanding natural ionospheric processes. During active ionospheric research, the signal generated by the transmitter system is delivered to the antenna array and transmitted in an upward direction. At an altitude between 7. IRI. The intensity of the HF signal in the ionosphere is less than 3 . The small effects that are produced, however, can be observed with the sensitive scientific instruments installed at the HAARP Station, and these observations can provide information about the dynamics of plasmas and insight into the processes of solar- terrestrial interactions. The Effective Radiated Power (ERP) of the IRI is limited by more than a factor of 1. Much of this is due to higher antenna losses and a less efficient antenna pattern. The IRI can transmit between 2. MHz, a frequency range that lies above the AM radio broadcast band and well below Citizens' Band frequency allocations. The HAARP Station is licensed to transmit only in certain segments of this frequency range, however. When the IRI is transmitting, the bandwidth of the transmitted signal is 1. Hz or less. The IRI can transmit in continuous waves (CW) or in pulses as short as 1. CW transmission is generally used for ionospheric modification, while transmission in short pulses frequently repeated is used as a radar system. Researchers can run experiments that use both modes of transmission, first modifying the ionosphere for a predetermined amount of time, then measuring the decay of modification effects with pulsed transmissions. There are other geophysical instruments for research at the Station. Some of them are: A fluxgatemagnetometer built by the University of Alaska Fairbanks Geophysical Institute, available to chart variations in the Earth's magnetic field. Rapid and sharp changes of it may indicate a geomagnetic storm. A digisonde that provides ionospheric profiles, allowing scientists to choose appropriate frequencies for IRI operation. The HAARP makes current and historic digisonde information available online. An induction magnetometer, provided by the University of Tokyo, that measures the changing geomagnetic field in the Ultra Low Frequency (ULF) range of 0. An environmental impact statement led to permission for an array of up to 1. A large structure, built to house the OTH now houses the HAARP control room, kitchen, and offices. Several other small structures house various instruments. The HAARP site has been constructed in three distinct phases. It was fed with a total of 3. W) combined transmitter output power. The DP transmitted just enough power for the most basic of ionospheric testing. The Filled Developmental Prototype (FDP) had 4. W of transmitter power. It was fairly comparable to other ionospheric heating facilities. This was used for a number of successful scientific experiments and ionospheric exploration campaigns over the years. The Final IRI (FIRI) is the final build of the IRI. It has 1. 80 antenna units, organized in 1. Sylvia Woods Harp Center - Harpsicle Harp Company. Harpsicle Prices: Harpsicle. Sylvia will personally assist you in ordering your harp. Range: 2. 6 nylon strings. They are great for beginners, kids, harp therapy practitioners, or just for taking to the beach or the park. Types of Harpsicles: There are 4 types of 'Sicles, depending on how many sharping levers are included: Harpsicles.
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