Shock diamond

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SR-71
fuel before the program ended.

Shock diamonds (also known as Mach diamonds or thrust diamonds) are a formation of

exhaust plume of an aerospace propulsion system, such as a supersonic jet engine, rocket, ramjet, or scramjet, when it is operated in an atmosphere. The "diamonds" are actually a complex flow field made visible by abrupt changes in local density and pressure as the exhaust passes through a series of standing shock waves and expansion fans. The physicist Ernst Mach was the first to describe a strong shock normal to the direction of fluid flow, the presence of which causes the diamond pattern.[1]
: 48 

Mechanism

Shock diamonds behind a Lockheed SR-71 Blackbird.
Shock diamonds from an F-16 taking off with afterburner
Aerojet Rocketdyne RS-25 engine test at NASA's Stennis Space Center
F-22 Raptor
with shock diamonds behind it
USAF F-22 Raptor flying in knife edge during a high-speed low-altitude pass over Airventure in full afterburner with Mach diamonds at sunset
USAF F-22 Raptor flying in knife edge during a high-speed low-altitude pass over Airventure in full afterburner with Mach diamonds at sunset

Shock diamonds form when the supersonic exhaust from a

air pressure. The higher ambient pressure compresses the flow, and since the resulting pressure increase in the exhaust gas stream is adiabatic, a reduction in velocity causes its static temperature to be substantially increased.[2]
The exhaust is generally over-expanded at low altitudes, where air pressure is higher.

As the flow exits the nozzle, ambient air pressure will compress the flow.

normal shock wave or Mach disk. This locates the first shock diamond, and the space between it and the nozzle is called the "zone of silence".[3]
The distance from the nozzle to the first shock diamond can be approximated by

where x is the distance, D0 is the nozzle diameter, P0 is flow pressure, and P1 is atmospheric pressure.[3]

As the exhaust passes through the normal shock wave, its temperature increases, igniting excess fuel and causing the glow that makes the shock diamonds visible.

diamonds
, giving them their name.

Eventually the flow expands enough so that its pressure is again below ambient, at which point the expansion fan reflects from the contact discontinuity (the outer edge of the flow). The reflected waves, called the compression fan, cause the flow to compress.

turbulent shear at the contact discontinuity causes the wave pattern to dissipate with distance.[4]

Diamond patterns can similarly form when a nozzle is under-expanded (exit pressure higher than ambient), in lower atmospheric pressure at higher altitudes. In this case, the expansion fan is first to form, followed by the oblique shock.[2]

Alternative sources

Shock diamonds beneath Masten Space Systems Xoie rocket during the Lunar Lander Challenge competition-winning landing.

Shock diamonds are most commonly associated with jet and rocket propulsion, but they can form in other systems.

Natural gas pipeline blowdowns

Shock diamonds can be seen[by whom?] during gas pipeline blowdowns because the gas is under high pressure and exits the blowdown valve at extreme speeds.[citation needed]

Artillery

When artillery pieces are fired, gas exits the cannon muzzle at supersonic speeds and produces a series of shock diamonds. The diamonds cause a bright muzzle flash which can expose the location of gun emplacements to the enemy. It was found that when the ratio between the flow pressure and atmospheric pressure is close, which can be achieved with a flash suppressor, the shock diamonds were greatly minimized. Adding a muzzle brake to the end of the muzzle balances the pressures and prevents shock diamonds.[1]: 41 

Radio jets

Some

radio galaxies, are observed to have regularly-spaced knots of enhanced radio emissions.[1]: 68  The jets travel at supersonic speed through a thin "atmosphere" of gas in space,[1]: 51  so it is hypothesized that these knots are shock diamonds.[5][6]

See also

References

  1. ^ a b c d Michael L. Norman; Karl-Heinz A. Winkler (July 1985). "Supersonic Jets". Los Alamos Science. 12: 38–71.
  2. ^ a b c d e f Scott, Jeff (17 April 2005). "Shock Diamonds and Mach Disks". Aerospaceweb.org. Retrieved 6 November 2011.
  3. ^ .
  4. ^ "Exhaust Gases' Diamond Pattern". Florida International University. 12 March 2004. Archived from the original on 7 December 2011. Retrieved 6 November 2011.
  5. ^ "Shock Diamonds In Space: Extragalactic Afterburner From PKS 0637-752 | Science 2.0". www.science20.com. 27 August 2014. Retrieved 13 March 2024.
  6. ^ Barnes, Luke; Filipovic, Miroslav; Norris, Ray; Velović, Velibor; Conversation, The. "Astronomers have detected one of the biggest black hole jets in the sky". phys.org. Retrieved 13 March 2024.

External links