Monday, June 12, 2017

Shock Impingement Heating Is Very Dangerous

Update 2-6-18:  see two added paragraphs at end of article.

Update 6-8-19:  I see lots of readership from a NASA-related spaceflight forum looking at this particular posting of mine.  You might be interested in some closely related postings about hypersonic flight as well.  Be aware that the hypersonic transient problem of entry is fundamentally different and distinct from the hypersonic steady cruise problem.

These are "Heat Protection is the Key to Hypersonic Flight" dated 4 July 2017,  "Thermal Protection Trends for High-Speed Atmospheric Flight" dated 2 January 2019,  "A Look at Nose Tips (Or Leading Edges) dated 6 January 2019,  and "Subsonic Inlet Duct Investigation" dated 9 January 2019.  That last deals with a subsonic duct inside a supersonic or hypersonic vehicle with an inlet.  

Use the access tool on the left of my page.  Click first on the year,  then the month,  then the title.  

Given the discussions on your forum of the design of the Spacex "Starship",  you might also want to view the articles I have written on that topic,  too.  These include (but are not limited to) "Reverse Engineering the 2017 Version of the Spacex BFR" dated 17 April 2018,  "Relevant Data for the 2018 BFS Second Stage" dated 24 September 2018,  and "Designing Rough Field Capability Into the Spacex Starship" dated 4 February 2019. 

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The X-15-A-2 was rebuilt from ship #2 after a crash.  In October 1967 Pete Knight flew this craft to Mach 6.7 as part of a flight envelope expansion project,  with a dummy scramjet pod attached to the ventral fin stub.  There was severe heating damage to the ventral fin stub from spike shock shed from the from dummy scramjet pod.  The pod separated in flight.  Inconel-X skins suffered about 7 times-normal heating rate due to shock wave impingement. 


The first photo shows the vehicle about to be dropped from its mothership B-52.  Note the white heat protection coating applied to vehicle,  and the dummy scramjet pod attached to ventral fin stub.  The white heat protection coating did not prove to be successful.  This version of the X-15 had two big drop tanks of rocket propellants.  


The second photo is actually 3 images combined to get 3 views of damaged ventral fin stub.  It shows clearly the damage to the ventral fin,  obviously of a meltback nature.  The material was simply overheated by shockwave impingement.  These skins were Inconel-X,  with a listed max useful temperature about 1500 F,  and with meltpoint well beyond 2500 F but far less than 3000 F.


The third image is another view of the damaged ventral fin,  with damage to the aft fuselage also visible.  The separated scramjet pod was also recovered,  and is shown.


What this proves is that the “parallel nacelle” arrangement is a really bad idea when flight speeds exceed about Mach 5 or 6,  varying with the toughness of the materials involved.   If you let this situation go on long enough,  the impinging shock wave will cut away all the adjacent structure that it strikes.

That is the fundamental reason there have been no successful hypersonic vehicles using the “parallel nacelle” arrangement.  The SR-71 and similar aircraft simply did not fly fast enough to incur this kind of damage.  The X-15 did,  and any entry vehicle far exceeds the heating risks that the X-15 saw. 

Schematically,  this is illustrated in the sketch.  The areas at risk are subject to direct impingement,  meaning the shock wave is “headed directly toward” the surface at risk,  as if that surface is “in the way” of the wave.  For waves that propagate 90 degrees away from the “headed toward” direction,  the effects are very much less.  That is why fins do not damage the surface from which they extend.  There can be a little local heating,  but nothing at all like direct wave impingement.  


As to when the damage occurs,  that depends upon the material and upon the flight speed.  Even the turbine blade superalloys fail by melting under 3000 F,  and fail structurally at temperatures not much over 2000 F.  For a steady state exposure,  the energy balance is convective input to the material,  balanced by internal convective cooling,  or by external re-radiation of heat to environment,  or by a combination of both.  If neither cooling occurs,  the material soaks out to the recovery temperature.

The convective input is driven by the difference between the recovery temperature and the material temperature.  The re-radiation ability is driven by the infrared (and optical) emissivity of the material and its temperature.  In the case of the X-15 flight,  there was no internal cooling,  and the white coating had drastically reduced the material’s emissivity (the normal surface finish was nearly black).
 
At Mach 6.7 and 100,000 feet on a 1962 standard day,  the turbulent recovery temperature that drives convective input calculates as about 3250 F,  well beyond the melting point of any superalloy,  much less its maximum use temperature.  With re-radiative cooling suppressed by the white coating (and no internal cooling),  it should not be surprising in retrospect that the test nacelle bow shock did extensive damage to the fin stub and aft fuselage. 


The only real surprise is that this X-15 survived that particular flight at all.  The exposure was brief enough that these effects did not have the time to sever its tail section. 

Update 2-6-18:

Shock impingement heating may act as a multiplier upon whatever correlation for convective film coefficient you are using to predict heating.  It's a large multiplier,  7 in the case of the cited X-15 flight.  The film coefficient itself is more or less proportional to atmospheric pressure to the 0.8 power as you increase altitude.  The higher you are,  the smaller the film coefficient,  and the lower the convective heating,  all else equal.

Typical staging in a launch vehicle takes place nearer Mach 2 or 3,  at nearer 200,000 feet than 100,000 feet.  Both the lower speed (reduced recovery temperature) and the thinner air (lower film coefficient) reduce heating,  even shock impingement heating.  That's how launch vehicles get away with parallel-nacelle-mounted side boosters,  and aluminum alloy tank construction.

6 comments:

  1. The one visible project that this issue will affect is Skylon spaceplane of course. The single heaviest item on the subsystem list behind the engines is the cooling system for wings and leading edges. 5t compared to 11t for the engines.

    https://www.google.si/url?sa=t&source=web&rct=j&url=https://www.aiaa.org/WorkArea/DownloadAsset.aspx%3Fid%3D14414&ved=0ahUKEwiByIbhn7rUAhVGtBQKHSh1Dl0QFggoMAM&usg=AFQjCNHkTH30xBOB8c5gwrgzmPQlLFp15g&sig2=388cOP_qHaCVw02ObcQO0g. Page 33.

    Assuming they have done the math.

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    1. It would take extraordinary means to keep the spike shocks from cutting off the wings during reentry. No other serious entry vehicle proposals have ever undertaken this risk. And for good reason. -- GW

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    2. Good post & diagram on shock impingement Gary.
      Yeah, the first time I saw a rendering of Skylon my first thought was "surely you're joking". If the engine tests start to pan out, I presume they will produce a more realistic airframe design.
      Frankly, the current goofy Skylon airframe must turn off a lot of investors who would otherwise be interested in the propulsion concept. Maybe the Skylon guys figured that if they presented a rendering that looked like another NASP, people would say "meh, that's old news".

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  2. An interesting phenomenon. Thanks for writing on it!

    If the shockwaves are spaced apart, can they theoretically can cancel each other?

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    Replies
    1. Theoretically? I don't know. In the real world, I don't think so. I see no cancellation in the shock diamond train of a propulsion nozzle. -- GW

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