Showing posts with label HAARP. Show all posts
Showing posts with label HAARP. Show all posts

July 24, 2018

Stay tuned for HAARP WSPR transmissions!

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Ok, what are they up to at HAARP (the High Frequency Auroral Research Program in Gakona, Alaska)? Are they really going to do it? Some recent posts by HAARP Chief Scientist Chris Fallen KL3WX on Twitter (see below) suggest that they're really going to do some tests in WSPR mode during the summer research campaign coming up soon!
I like the thought of maybe being one of the initiators of these HAARP WSPR tests; I suggested using WSPR mode to Chris Fallen in a Twitter post long time ago, and I also suggested it in my blog post / open letter to Chris Fallen here.
I'm really excited about this news, and I'm really looking forward to catching some WSPR signals from HAARP soon.










During the last research campaign, in the spring of 2018, I was quite successful at receiving and identifying one of the HAARP transmissions. The observed odd off time of one of their transmissions on 9.500 MHz helped me identify with 100 percent certainty the received signal as coming from HAARP.

HAARP signal as received by PA7MDJ on 9.500 MHz on April 8th, 2018 made visible in Spectran and Argo which clearly shows the off time of 01:29:30 UTC, exactly as announced by Chris Fallen on Twitter (see below). This positively identifies the signal as coming from HAARP. Click to enlarge.




During one of their earlier campaigns I was already successful at receiving HAARP on 9.500 MHz, but then the observed off time of exactly at the hour left some room for doubt (although not much, see my blog post here).
The received HAARP signals consisted of a carrier only, and there was no other way to identify the signals than by observing the start / off times of the received signal and to see if they correspond to the announced start / off times. The HAARP WSPR signals without doubt will be a lot easier to identify.

If you're interested in my other blog entries about HAARP, take a look here.

April 03, 2018

Next research campaign at HAARP due this April

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The next research campaign at HAARP is due this April. Between April 6th and April 14th, hams and shortwave listeners might get another chance to pick up the signals of the HAARP research facility located in Gakona, Alaska. See also my blog entries of January 29th, 2018 and August 18th, 2017.

Assistant research professor Chris Fallen, KL3WX, of the University of Alaska Fairbanks Geophysical Institute on March 29th twittered the following:

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I must stay at @UAFairbanks for much of the @UAFHAARP campaign April 6-14, but will continue to tweet selected experiment freqs and modes when available. Have not forgotten about earlier QSLs (mea culpa!) and am working on a better system moving forward.
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Follow Chris Fallen on Twitter for the latest updates.


The following news about the upcoming research campaign recently appeared on the ARRL website:

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HAARP Facility to Resume Ionospheric Research this Week
04/02/2018

Alaska’s super-power High-Frequency Active Auroral Research Program (HAARP) transmitters in Gakona, Alaska, will fire up again for the spring research campaign April 6 – 14. University of Alaska Fairbanks (UAF) Space Physics Group researcher and HAARP Chief Scientist Chris Fallen, KL3WX, told ARRL that more than 40 hours of “externally funded” experiments are in the queue.

“Scientists from US universities and government labs will explore the physics of scintillations, magnetic field-aligned plasma irregularities, artificial and natural atmospheric airglow, stimulated electromagnetic emissions, plasma waves, and radio-enhanced ionization,” Fallen said. “The HAARP transmitter is still at 80% net power, but by summer we expect to have the final ‘column’ of transmitters restored, bringing the array back to 100%.”

For his part, Fallen said he still has some time remaining on his National Science Foundation (NSF) grant to study artificial airglow, but added that this is “a tough time of year in a tough year of the solar cycle” for such experiments. “It will not be dark enough in Gakona to observe artificial airglow emissions until 10 PM at the beginning of the campaign and 10:30 PM at the end of the campaign, due to the rapidly lengthening days in the Land of Midnight Sun.”

Fallen said that due to weakening solar activity, the critical frequency of the ionosphere’s F2 layer (foF2) is relatively low during the day, peaking at a little more than 4 MHz above Gakona in the late afternoon, and falling rapidly in the evening. “This limits the time available for experiments, since airglow is usually only created when the HAARP transmission frequency is near or below foF2,” Fallen explained. “The lower limit of the HAARP transmitter is approximately 2.7 MHz, and so we can only expect perhaps 30 minutes or less of usable airglow experiment time each day.”

Fallen said he is considering his options and plans to continue “bundling” amplitude modulations in the airglow experiments of interest to hams. His previous airglow experiments were accompanied by tones and music to illustrate the Luxembourg effect and slow-scan television (SSTV) images in Scottie 1 format.

“In future experiments, I want to try sending text and images using one of the MFSK modes,” Fallen told ARRL. “Several hams have requested I try the smoking hot FT8 mode with HAARP. Since that is a mode primarily designed for two-way contacts and makes use of time synchronization to help achieve amazing efficiency, it is not yet clear to me how to best do this with HAARP which currently has no receive capability.”

Fallen said he has to be at UAF for much of the April campaign but will be at HAARP toward the end. He plans to tweet selected transmitter frequencies and other information throughout the campaign from his personal Twitter page. HAARP’s official Twitter page will share photos and other information of general interest, “such as what the HAARP dog is up to,” Fallen said.

Operation of the HAARP research facility was transferred from the US Air Force to UAF in 2015.

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January 29, 2018

The Quest for HAARP

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The HAARP research facility in Gakona, Alaska under the lights of the Aurora borealis

As a radio hobbyist and space physics enthusiast I've always been highly fascinated by the HAARP research facility. HAARP stands for High Frequency Active Auroral Research Program. The facility is owned and operated by the University of Alaska Fairbanks and is located in Gakona, Alaska.
The most prominent instrument of the HAARP research facility is the so called "ionospheric heater", a huge array of transmitters and antennas (capable of transmitting up to a power of 4 GW ERP) with which temporarily a limited area of the ionosphere can be excited or "heated". For more technical, scientific, and historical information on HAARP I would like to refer you to the internet; a search on Google will give you plenty of hits. You'll also find a list of selected links below, and you might like to read my previous blog entry about HAARP here.

Already in early 1997 the first amateur-radio dedicated test of the then brand new HAARP facility (then still a US Military facility) was announced. The ARRL issued special bulletin ARLX005 which read as follows:

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SB SPCL @ ARL $ARLX005
ARLX005 HAARP to air test transmission for hams

ZCZC AX05
QST de W1AW
Special Bulletin 5  ARLX005
From ARRL Headquarters
Newington CT  February 21, 1997
To all radio amateurs

SB SPCL ARL ARLX005
ARLX005 HAARP to air test transmission for hams

The High Frequency Active Auroral Research Program (HAARP) facility
in Gakona, Alaska, will transmit a test signal on March 8, 1997,
seeking reports from hams and SWLs in Alaska and in the ''Lower 48''
to determine how well the HAARP transmissions can be heard to the
south.

During this test, the HAARP facility will transmit on or near the
frequencies 3.4 MHz and 6.99 MHz to give listeners the opportunity
to listen for the HAARP facility and to claim a QSL card. The test
will be conducted beginning at 0430 UTC on March 8 (2330 Eastern
Time on March 7).

The format of the test will be to transmit a constant carrier (no
modulation) signal followed by a CW message at 10 WPM, according to
the following schedule:

TIME     FREQ         SIGNAL          ANTENNA POSITION

0430     6.99 MHz    Carrier only      Pointed up
0435     6.99 MHz    CW message        Pointed up
0440     6.99 MHz    Carrier only      Pointed to SE
0445     6.99 MHz    CW message        Pointed to SE
0450     3.4 MHz     Carrier only      Pointed up
0455     3.4 MHz     CW message        Pointed up

The transmission beginning at 0450 is primarily for Alaskan hams.
Reception reports should include signal strength during the constant
carrier transmission period along with the text of the CW message.

Complete details on this test and a QSL address will be listed on
the HAARP home page at
http://server5550.itd.nrl.navy.mil/announce.html.

The HAARP facility--now in the developmental prototype stage--has
been undergoing testing since it was completed in late 1994.
Multiple transmitters feed multiple antenna elements (there are 48
antenna elements on the site, arranged in eight rows of six columns;
however, at this time, only 18 elements are active. The test will
use 17 antennas with a net transmitter power of 340 kW). The final
configuration could have 180 antenna elements and a combined
transmitter power of 3.6 MW. HAARP's stated scientific purpose is to
study ''the properties and behavior of the ionosphere, with
particular emphasis on being able to understand and use it to
enhance communications and surveillance systems for both civilian
and defense purposes.'' HAARP is managed by the US Air Force and the
US Navy.

For more information, see ''The High Frequency Active Auroral
Research Program'' (QST, Sep 1996, p 33), or check out the HAARP home
page, http://server5550.itd.nrl.navy.mil/haarp.html.
NNNN
/EX
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In those days I was a keen SWL, and I remember the announcements, but for some reason I missed the actual test. I believe at the time I was busy preparing for travelling to, or was already travelling in, northern Scandinavia, which might explain things. Or did the announcements reach me too late? I can't remember clearly. I can't recall either ever having read or heard anything about the test being successful or not.

To my knowledge no other special amateur-radio dedicated tests were conducted thereafter (please correct me if I'm wrong). Then the US Air Force in 2014 announced that the facility would be completely closed down and HAARP went silent for good.
Or so was thought! The facility was taken over by the University of Alaska Fairbanks, and in February and September of 2017 HAARP was again heating up the ionosphere. Since the equipment of the facility had not been used for a couple of years, it was decided to go easy on the generators and transmitters, and the ionospheric heater was used at only a part of its full capacity, both antenna and power wise.




Excellent article on HAARP in the October 1996 issue of the legendary Monitoring Times magazine. Great article debunking the early myths and conspiracy theories about HAARP*. MT magazine from the collection of PA7MDJ.

The campaigns at HAARP in 2017 were primarily scientific research projects of course, but they had a ham radio flavour to it!
The ionospheric research campaigns done in 2017 were led by Assistant research professor Chris Fallen of the University of Alaska Fairbanks Geophysical Institute. And Chris Fallen also happens to be radio amateur KL3WX! Chris announced the tests on his website and on his Twitter account, and radio amateurs and shortwave listeners were asked to participate by monitoring for the HAARP signals. During the actual campaigns, Chris announced on and off times, frequencies, and mode on his Twitter account, helping radio hobbyists to tune in to the signals, and feedback was given to reports and questions from listeners.
The signals mainly consisted of unmodulated carriers or carrier pulses, but during the September 2017 campaign especially for the radio amateurs and SWLs listening in, also some SSTV images were transmitted! Also some AM transmissions were done with tones and musical tunes to generate the Luxembourg or cross-modulation effect. But both the SSTV and AM signals were transmitted on lower frequencies and were difficult or impossible to receive outside of North America.

During the February 2017 campaign I did not manage to receive the HAARP signals. During the September 2017 campaign I again did not manage to pick up the HAARP signals on the lower frequencies, but this time also a higher frequency was used: 9.500 MHz. And this higher frequency proved to be suitable to propagate the unmodulated carrier of the HAARP experiments to me in the Netherlands several times. I used my Yaesu FT-991 transceiver and a HyEndFed 10/20/40 wire antenna to pick up the signals.

On 9.500 MHz I do have a lot of interference from PLC devices, and at times there was also some interference from broadcast stations on nearby frequencies. But by using a narrow digital filter of 300 to 50 Hz in CW mode, wide enough for just an unmodulated carrier, much of this could be eliminated. And nowadays we have the advantage of being able to detect received carriers and make them visible with the computer and spectrum analyzer software like for instance Spectran or Argo. And that's what I did.

I was surprised and still am by the choice of the higher frequency; 9.500 MHz is in the middle of the 31m broadcast band, and there's no way of determining if the received carrier is from a weak broadcast station or from HAARP except by watching closely for the on and off times of the carrier, as these were announced by Chris Fallen on Twitter.

Only one time I was able to determine both the exact on and off time of the received carrier, which enabled me to identify the signal with almost 100% certainty as coming from HAARP. On September 24th, 2017 a carrier was received starting at 0100 UTC and ending at 0200 UTC, exactly as announced by Chris Fallen on his Twitter account.

I checked this website https://www.shortwaveschedule.com/index.php?freq=9500 for the schedules of broadcast stations on 9.500 MHz. Only one station was transmitting on this frequency during the time of reception and that is China National Radio 1. But this station broadcasts continuously from 1825 to 0600 UTC and does not have a sign-on and sign-off time of respectively 0100 and 0200 hours UTC.

But still the on and off times exactly at the hour are of course common for broadcast stations, and there's always a slight chance that the carrier was originating from some broadcast station that no schedule is known of. To be really sure an odd on or off time of for instance a couple of minutes after the hour would have been helpful. At one occasion when I was able to detect the carrier an odd off time was announced but unfortunately the carrier had faded out by the time it was turned off. Also if the carrier would have been pulsed there wouldn't have been any doubt left, but I did not receive any of the pulsed carrier transmissions.

Furthermore, I'd like to note that at times the carrier was strong enough to actually be audible through the speaker of my transceiver, beside also being detected in Spectran.

Carrier detected on 9.500MHz with Spectran with on time of 0100 UTC (Spectran shows local time UTC+2). My receiver's CW sidetone pitch is set to 880 Hz, explaining the frequency of the carrier in the screenshot. The ticks are placed at one second intervals.

The same carrier with off time 0200 UTC

I know the campaigns at HAARP are primarily scientific research experiments, but from an amateur radio point of view I hope I may be so bold to make some suggestions, or requests as you will, to Assistant research professor Chris Fallen for future HAARP campaigns. In case of implementation these suggestions will not directly add scientific value but might cater to the radio amateur, and in particular the ones at DX locations. This is the point where I'd like to consider this blog entry doubling as an open letter to Assistant research prof. Chris Fallen.

1. The higher frequency of 9.500 MHz proved to be suitable for easy worldwide reception of the HAARP transmissions, but in the future could maybe a frequency be chosen in the same range but outside of the 31m broadcast band, for instance 9.300 MHz?

2. Is there a possibility to have HAARP transmitting WSPR signals, or even better JT9 (as in JT9 a free-text message can be transmitted; in WSPR you'll have to transmit a callsign)? WSPR or JT9 would enable radio amateurs to pick up and identify the signals up to a signal to noise ratio of about -30 dB. So even extremely weak signals will be detected. If desired, announce a WSPR or JT9 test to the weak signal community, and you'll have a huge audience worldwide. WSPR and JT9 are FSK type emissions and possibly might be generated by the HAARP computers/software that drive the transmitters.

3. In order to make identification easier, could some intelligence be added to each continuous unmodulated carrier transmission, like for instance a morse code identification? QRSS (very slow CW) could be used with a "dit" length of for instance 6 seconds. Even when the signal is inaudible, with for instance Argo a QRSS morse code identifier could still be made visible. Argo is already widely used by hams and SWLs listening for HAARP.
The SSTV was very nice, but is useless when the signals are weak, or at the low frequencies that were used aren't present at all, like at my station in the Netherlands.

Last but not least I'd like to thank Assistant research prof. Chris Fallen for giving hams and SWLs the opportunity to participate in the fascinating research done at HAARP. I'm looking forward to the next research campaign!

Addendum 01.02.2018
* The full Monitoring Times article can be found here:
http://www.oocities.org/marksrealm/project145.html


See also:

https://en.wikipedia.org/wiki/High_Frequency_Active_Auroral_Research_Program
https://en.wikipedia.org/wiki/Ionospheric_heater
http://www.gi.alaska.edu/haarp
http://www.arrl.org/news/alaska-s-haarp-facility-once-again-open-for-business
https://twitter.com/UAFGI
https://twitter.com/uafhaarp
https://twitter.com/ctfallen

August 18, 2017

HAARP and Arecibo ionospheric HF heating research facilities

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I've always been highly fascinated by the HAARP facility in Gakona, Alaska. I already was back in the 1990s, when the research station was still operated by the US military and I was still an SWL.
HAARP stands for High Frequency Active Auroral Research Program. At the facility ionospheric research is done. The most prominent instrument at HAARP is the so called "ionospheric heater", a high power HF radio transmitter and antenna array which is used to temporarily excite a limited area of the ionosphere. Wikipedia states that the HAARP facility is capable of transmitting with a power of up to 4 GW ERP.
In 2014, the US Air Force announced that, starting that same year, the HAARP facility would be completely shut down and dismantled. In 2015 however, the control of the facility and all its equipment was taken over by University of Alaska Fairbanks and continues to operate. In February 2017, the first UAF-led research campaign was done. The UAF is not new to HAARP, as they already participated in the program when it was still operated by the military.


Assistant Research Professor Chris Fallen KL3WX of the University of Alaska Fairbanks Geophysical Institute, nowadays is one of the researchers doing ionospheric experiments at the facility, and keeps us posted on the ones that might be of interest to radio amateurs and shortwave listeners. The last research campaign of interest done at the facilty was in February 2017, and the next one will be in September 2017. During the February campaign, the signals of HAARP were picked up by radio amateurs all over the world. For more information, follow @ctfallen on Twitter, or visit his blog at https://sites.google.com/alaska.edu/gakonahaarpoon/.

The HAARP site from the beginning has always been subject to conspiracy theories. Read some more about it at www.haarp.net.

Another ionospheric HF heater recently was constructed at the famous Arecibo Radio Telescope in Puerto Rico. The heater at Arecibo has a nominal power of 600 kW, 100 to 200 MW ERP.
The first research campaign was done this summer, and the signals were received by radio amateurs worldwide, including at PA7MDJ in the Netherlands. A short video compilation of the Arecibo listening sessions done at PA7MDJ, including audio recordings of the signals received, can be found here:


Some more technical info about the Arecibo ionospheric heater can be found here.

Here are some more pictures of the HAARP facility:





HAARP QSL cards!

See also:

https://en.wikipedia.org/wiki/High_Frequency_Active_Auroral_Research_Program 
https://en.wikipedia.org/wiki/Ionospheric_heater
http://www.gi.alaska.edu/haarp
http://www.arrl.org/news/alaska-s-haarp-facility-once-again-open-for-business
https://twitter.com/UAFGI
https://twitter.com/uafhaarp
https://twitter.com/ctfallen
https://en.wikipedia.org/wiki/Arecibo_Observatory
http://www.naic.edu/~astro/ao50/Arecibo_50th_Paper_Breakall_revised_Oct_23_2013.pdf