Welcome to the new HAARP website (2024)

New Website

The University of Alaska Fairbanks High-frequency Active Auroral Research Program is pleased to announce the launch of our newly redesigned website:https://haarp.gi.alaska.edu/.Learn about HAARP news, frequently asked questions, diagnostic instruments, research support services, merchandise and more. Plus, in collaboration with our international and national research partners, you can see a diagnostic suite of on-site geophysical instruments and view real-time data.

Open House

After three successful open house events in 2016, 2017 and 2018, the HAARP Ionospheric and Radio Science Laboratory in Gakona, Alaska, will not be having an open house in 2020. We’re optimistic we’ll be able to open the facility to the public again in 2021.

Due to the COVID-19 pandemic, we are not hosting large public events. After consultation with Geophysical Institute leadership, we are taking this step to prevent both the public and staff members at the site from being infected with the novel coronavirus in our remote setting, which is far from medical assistance. As there are COVID-19 cases across the globe, there is no reasonable way to assure travelers to Gakona are free of the virus.

We recognize not having an open house this year is disappointing for many of you who plan your summer vacations around it. The good news is we’ve been hard at work growing the research site, and are excited to share our progress:

Planning for Sustainability

We’re continuing our work with University of Alaska leadership and our Alaska congressional delegation to develop policy language and funding models that will sustain the research facility well into the future. To further discussions at a national level, a HAARP Summit was conducted at the Woodrow Wilson Center in Washington, DC, in April 2019, which resulted in strong support from the research community. HAARP was also included in the United States Arctic Research Commission Goals and Objectives For Arctic Research Report for 2019-2020 which can be found here (page 20).

Public Information

We’ve revitalized our public web page, installed new research instruments, and added links to real time data feeds. Check out new information on our diagnostic suite and research support services.

Diagnostic Suite

Many passive scientific instruments at the site operate continuously to monitor the natural geomagnetic environment. In collaboration with our international and national researcher partners, we’ve made real time data collected at the site available here.

Research Growth

While the 33-acre Ionospheric Research Instrument gets most of the attention, the research site also maintains a suite of equipment, sensors and cameras. In addition to our current diagnostic suite that includes a riometer, ionosonde, weather station, seismic station, magnetometer, Wrangell webcam, and aurora forecast, here’s what’s new:

  • Reeve Observatory.A high-frequency (HF) amateur space weather, planetary radio emissions and radio propagation research station which monitors solar radio bursts and Jupiter radio emissions. Data collected is publicly available and is used to study space weather effects on high-latitude radio propagation.
  • e-CALLISTO Project. A solar radio wave spectrometer that contributes data to the International Space Weather Initiative (ISWI) CALLISTO project. The main applications are observation of solar radio bursts and radio frequency interference (RFI) monitoring used for astronomical science, education and outreach.
  • NASA Radio JOVE Project. A hands-on inquiry-based outreach project that allows students, teachers and the general public to learn about radio astronomy by building their own radio telescope from an inexpensive kit and/or using remote radio telescopes through the internet. Participants collaborate with each other through interactions and sharing of data on the network. Institutions and more advanced observers can set up a radio spectrometer designed to monitor radio waves from Jupiter and the Sun in the 15-30 MHz spectrum, as well as, study radio propagation through the ionosphere and space weather.
  • Earth Networks Lightning Detection Network Sensor. Equipment supplied by Earth Networks, with data available through their worldwide lightning detection network.

Community Support and Engagement

While we won’t be putting on an open house this year, we’re continuing to look for ways to bring HAARP research to the public. You’ll find a network of #UAFHAARP supporters on social media. Follow real-time developments with us on Twitter @UAFHAARP and @UAFGI and our Facebook pages. We encourage you to share the social media posts with your network so we can extend the conversation with a broader range of Alaskans and research stakeholders.

Thank you for your continued support. For further questions, please email UAF-GI-HAARP@alaska.edu or call 907-474-1100.

Welcome to the new HAARP website (2024)

FAQs

How much energy does HAARP produce? ›

The principal instrument is the Ionospheric Research Instrument (IRI), a phased array of 180 HF crossed-dipole antennas spread across 33 acres and capable of radiating 3.6 megawatts into the upper atmosphere and ionosphere.

Where is the new HAARP site? ›

Site. The project site ( 62°23′30″N 145°09′03″W) is north of Gakona, Alaska just west of Wrangell-Saint Elias National Park. An environmental impact statement led to permission for an array of up to 180 antennas to be erected. HAARP was constructed at the previous site of an over-the-horizon radar (OTH) installation.

Who is funding HAARP? ›

The number of experiments is the highest so far under a five-year, $9.3 million grant awarded last year by the National Science Foundation to establish the Subauroral Geophysical Observatory at HAARP. The observatory's purpose is the exploration of Earth's upper atmosphere and geospace environment.

When did HAARP begin? ›

The HAARP facility began operating in 1999 with a 6 × 8 array of transmitting antennas that, in total, produced 960 kW of RF power—about the same as generated by 10 AM radio stations. (The figure shows today's 12 × 15 array.)

Does the ionosphere affect weather? ›

Since the temperature of the thermosphere fluctuates due to the Sun's radiation, that can cause the area of the ionosphere to expand. Temperature variations range from 200 Kelvin to 500 Kelvin. The ionosphere is too high up to affect the weather far below in the troposphere. It's more the other way around.

What frequency does Haarp use? ›

HAARP uses powerful radio waves at HF (3–30 MHz) to heat the ionospheric plasma. It is located near Gakona in Alaska.

What are harp technologies? ›

Harp Technologies provides technology and research and development (R&D) services in RF, microwave, and millimetre-wave engineering. Complementary R&D services in embedded electronics, software, and thermo-mechanical design are provided as well.

What does Haarp stand for in Muse? ›

For their performances at Wembley, Muse had the stadium decked out with massive props to dress it as the Ionospheric Research Instrument of the High Frequency Active Auroral Research Program (HAARP), a US government-funded ionospheric research program in Gakona, Alaska which uses high frequency radio waves to cause ...

How do I contact Haarp? ›

Investigators interested in deploying diagnostic apparatus including radio receivers and radar, lidar, optical imagers and spectrometers, and interferometers are encouraged to contact the HAARP Ionospheric and Radio Science Laboratory at UAF-GI-HAARP@alaska.edu or 907-474-1100.

Where are HAARP stations located? ›

HAARP, scientific facility for studying the ionosphere, located near Gakona, Alaska. The main instrument is the Ionospheric Research Instrument (IRI), an array of 180 radio antennas spread over an area of 0.13 square kilometer (33 acres). The ionosphere is the outermost layer of Earth's atmosphere.

What is artificial airglow? ›

It is possible to enhance the natural airglow by transmitting a high power high frequency (HF) radio beam that modifies the ionosphere when the ionospheric conditions are favourable (i.e. high enough electron concentration and at high latitudes little or no auroral activity).

What happens when you heat the ionosphere? ›

As a heating pulse propagates through the ionosphere, energy absorbed from it is converted to electron heat- ing (Eq. 8). Electron heating modifies the absorbing properties in the region of propagation (since X is a func- tion of Te) through its dependence on the electron neu- tral collision frequency, v (Te).

What is the simple definition of the ionosphere? ›

ionosphere. noun. ion·​o·​sphere ī-ˈän-ə-ˌsfi(ə)r. : the part of the earth's atmosphere beginning at an altitude of about 30 miles (50 kilometers) and extending outward that contains free electrically charged particles.

What are ionospheric heaters used for? ›

An ionospheric heater, or an ionospheric HF pump facility, is a powerful radio wave transmitter with an array of antennas which is used for research of plasma turbulence, the ionosphere and upper atmosphere.

What happens when you heat up the ionosphere? ›

As a heating pulse propagates through the ionosphere, energy absorbed from it is converted to electron heat- ing (Eq. 8). Electron heating modifies the absorbing properties in the region of propagation (since X is a func- tion of Te) through its dependence on the electron neu- tral collision frequency, v (Te).

Where are Haarp stations located? ›

HAARP, scientific facility for studying the ionosphere, located near Gakona, Alaska. The main instrument is the Ionospheric Research Instrument (IRI), an array of 180 radio antennas spread over an area of 0.13 square kilometer (33 acres). The ionosphere is the outermost layer of Earth's atmosphere.

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