ULF, ELF and VLF generation with HF transmissions from ionospheric heaters

Polar electrojet heating and Ionospheric Current Drive heating


There are two ways to heat the ionosphere and perform ELF generation: polar electrojet heating and ionospheric current drive heating


Ionospheric heaters are powerful HF transmitters (2.8-10 MHz) that induce controlled temporary modification to the electron temperature at desired altitude. Creation of virtual ULF/ELF/VLF antennas.



Selected sources cited at "ELF Generation 101" (video/slides) by Climate Viewer managed by J. Lee, including mainly the presentation and discussion of three slides from D. Papadopoulos' 2013 presentation. Suggested reading: Papadopoulos et al 2011.



Polar electrojet (PEJ) heating 


Reference: https://youtu.be/lu0_lTXHICs?t=1067

Ionosphere heaters at high latitudes (near polar regions), such as EISCAT, HAARP and HIPAS, can use the polar electrojet, a naturally-occurring electric current in the D/E region (70-90 Km) of the ionosphere as both an amplifier and a virtual antenna. The polar electrojet is depicted in Climate 3D Viewer in Figure 1. 


There also exists an equatorial electrojet. The mid-latitude Arecibo heater (Puerto Rico) and the equatorial Jicamarca heater (Peru) have  used the equatorial electrojet (Cohen et al 2010, Lunnen et al 1984).




Figure 1: Climate 3D viewer screen capture showing the electrojet in the polar region.




Figure 2: Slide 5 from D. Papadopoulos' presentation (PDF).



Reference: https://youtu.be/lu0_lTXHICs?t=1143 (reads section "Polar electrojet (PEJ) heating")

The electrojet consists of natural currents which flow in the auroral and equatorial ionosphere at 80-100 Km (Figure 2). The high frequency (HF) signal of the ionospheric heater modulated at ELF/VLF frequencies is directed to the electrojet where it performs heating and thereby causes changes in the local conductivity of the ionosphere (Figure 2). The electrojet current is then caused to vary at the same ELF/VLF rate. Propagating ELF wave signals are radiated by this "virtual antenna". Polar electrojet heating will produce waves from 0.001 Hertz to 20.000 Hertz with a 2.8 to 8 KHz peak efficiency.







Ionospheric Current Drive (ICD) heating


Reference: https://youtu.be/lu0_lTXHICs?t=1267 (reads section "Ionospheric Current Drive (ICD) heating")

"Both high latitude and equatorial ionospheric heaters may use an alternate method to produce UFL/ELF waves that does not require the electrojet."
F-region heating leads to generation of magnetosonic (MS) waves as demonstrated in Figure 3. This is similar to having an antenna represented in the figure by the oval shape that radiates MS waves (yellow lines). The MS waves travel downwards in the E-region where they drive a Hall current. The Hall current generates ELF waves into the Earth-ionosphere waveguide and shear Alfvén waves (SAW) upwards in the magnetosphere (Papadopoulos et al. 2011). In other words, the Hall current acts as a secondary antenna or a virtual antenna which plays the role that had the electrojet in the case of the polar electrojet heating. MS and SAW waves are shown in Figure 5.

Figure 3: Slide 9 from D. Papadopoulos' presentation (PDF). Figure 1 from Papadopoulos et al. 2011





Reference: https://youtu.be/lu0_lTXHICs?t=1312 

"They're going to heat it way out here (arrow on Fig. 4). Now the MS (magnetosonic) waves, the very low frequency waves are what's creating the antenna now. They're not actually just powering the ionosphere - the polar electric jet - they're shooting it way out here into space; and these waves are traveling down and creating another antenna. This is very important and I know this is high-level but there are people who are going to understand this that need to hear it and they will do something about it I am sure."


There is a lot of debate on the internet about who's making a specific few Hertz tone.
"This proves beyond a shadow of a doubt that it is HAARP producing it, so guys over there on Tromsø, Stanford VLF, please get that updated".


"What they're doing is creating a virtual antenna in the sky that radiates extremely low-frequency signals that travel worldwide and can be heard in the deepest depths of our oceans."


"When you move it up here (arrow on Fig. 4), a standing wave can occur along these magnetic field lines and compressive magnetohydrodynamic waves, (that is) magnetosonic waves come straight through". "Magnetosonic are the lowest of low frequencies". Cf. fractions of a Hertz. 
Magnetohydrodynamic waves within the Earth's magnetosphere are geomagnetic pulsations. They are distinguished in magnetosonic waves (compressive) and Alfén waves (incompressible).
It is mentioned that when they turn HAARP on, the spectrum upon HAARP "ULF start" shows: "noise increase by 10 to 20 decibels between 0.7 to 10 Hertz". It has been alleged that covert signals may escape attention because signal processing personnel would consider that this "new" noise represents background noise and would therfore adjust the baseline accordingly.





Figure 5: Magnetostatic waves and shear Alfvén waves. Slide 14 from D. Papadopoulos' presentation (PDF).




Ionospheric Current Drive (ICD) heating can produce 0.1 Hz magnetosonic (MS) waves, 2.5 Hz shear Alfvén waves (SAW) and ULF/ELF waves up to 50-70 Hz (Figure 5).


Note on the ionospheric Alfvén resonator (IAR) and fast magnetosonic (FMS) waveguide.




Injection of ULF/ELF/VLF waves within field-aligned ducts, in the L-shell that spans the heater

Transmitted electromagnetic radiation may propagate along the magnetic field lines of the Earth termed L-shells (ducted propagation)


(Note: A specific set of Earth's magnetic field lines are described with L-shells (https://en.wikipedia.org/wiki/L-shell) i.e. ellipsoids similar to those of Fig.6).
https://youtu.be/lu0_lTXHICs?t=956 "If you fire a shot off into space and you're up here at the North Pole (Figure 6, top right, cf. EISCAT L-shell 5.8), it's going to travel a long distance and come down and land at the South Pole." If firing from the Sura Ionospheric Heating Facility, which corresponds to an L-shell 2.5, landing will take place at a shorter distance, closer to the Equator. If firing from HAARP landing will occur at what is referred to as the "congugate point" found near the shore of Australia.





Figure 6: Slide 15 from D. Papadopoulos' presentation (PDF).


"Then some of it bounces off - and, you know, aggravates the heads of people all in this region - then bounces back into space. Now, once it makes it all the way back to HAARP, that's called a hop. Now why am I telling you this? Well, they have a thing out here in the middle of the ocean called the HAARP buoy and it's part of the one-hop-experiment." "It's a VLF buoy, so basically (at) the place where HAARP lands in the ocean, they put a receiver out there to listen for it. And that conjugate point is right off the shore of Australia." (Stanford VLF buoy shown in Figure 7.)



Figure 7: Figure 1 from Golkowski M. et al, 2018 illustrating ducted propagation excited by the HAARP HF heater and image of Stanfold VLF buoy (HAARP receiver).



Figure 8: Raising maximal usable frequency (MUF) to GHz.  Field-aligned scatter (FAS). Platteville FAS reference. Slide 65 from D. Papadopoulos' presentation (PDF).