. 24/7 Space News .
ROCKET SCIENCE
Simulating hypersonic flow transitions from smooth to turbulent
by Staff Writers
Chicago IL (SPX) Nov 07, 2018

Computed Schlieren image of the high -Re case at t = 30.6; T: triple point; R: reattachment shock; C1, C2, and C3: contact discontinuity surfaces. The insets are the normalized pressure P/Pmax and Mach contours in the neighborhood of the triple point, and the yellow lines show the streamlines.

To break out of Earth's lower orbit, hypersonic vehicles will need to reach speeds greater than 28000 kmh. At these speeds, the air particles and gases that flow around the vehicle and interact with the surfaces generate heat and create shock waves that disturb the flow's equilibrium. New research at the University of Illinois at Urbana-Champaign created a model to simulate and better understand flow transitions.

"At hypersonic speeds, the flow is moving at high Mach numbers, but there are also wings or flaps on the vehicle. At each of those junctures, you can have very strong recirculation, which leads to unsteadiness. It's difficult to predict how bad the unsteadiness can become before the flow is no longer smooth, and becomes turbulent," said Deborah Levin, professor in the Department of Aerospace Engineering in the College of Engineering at the U of I.

She and her doctoral student Ozgur Tumuklu, along with Professor Vassilis Theofilis from the University of Liverpool, conducted research that brings a revolutionary understanding to the field of hypersonic flow.

Levin said she studies flow at a very fundamental level to understand the flow, the forces that the flow can create, and the length of time the flow remains stable in terms of microseconds to milliseconds - faster than the blink of an eye.

"From the very fundamental aspects of the flow, when the speed is so high, the gases around the surfaces become very hot," Levin explained. "The frictional heat starts to cause chemical reactions. The gas no longer remains 79 percent nitrogen and 21 percent oxygen like we have in our atmosphere.

"When all of these effects occur, they're called non-equilibrium effects. It's a phenomenon that occurs as the air gets thinner as you move faster," Levin said.

"Coupling all of that - the non-equilibrium and the stability - that's what's really novel about this research and hasn't been done before. The outcome of this research is a model and the ability to now use this technique in the future to design shapes and induce chemical reactions that will or will not induce stability or quench it."

Levin said some of the original work in this field began with experiments at the U of I with Professor Joanna Austin, before leaving for a position at California Technical. A major part of her work at Illinois was designing a new facility that could measure some of the features of flow.

"She has a hypervelocity expansion tube - a class of measurement techniques that can be used to induce a flow over a double-wedge model about the size of my hand," Levin said.

"Dr. Austin creates a hypersonic flow over the entire model. It used a tremendous about of energy to accomplish but it can be used for low density (thinner air) cases. But the double wedge can be a difficult shape to understand what's going on. We ran numerous simulations but could not get the flow to reach a stable or steady result."

Levin said collaborating with Theofilis helped moved the work forward, particularly with respect to a new approach and toward the shape of the model.

"He said to me, 'I know this condition [sic double wedge] is difficult to understand from a stability point of view, but if you start to print out from your flow calculations the temperature here, here, and here, you'll see that the temperature will never stabilize. You'll see swirls and vortices that come and go.' When an expert tells you that, you pay attention," Levin said.

One thing that they did do before leaving the double wedge was to "artificially reduce the conditions in the hypervelocity expansion tube by by a factor of about an eighth," Levin said. "We still saw a lot of the features like the shocks, and recirculation, but the flow calmed down and we were able to simulate a steady state."

The researchers put the double wedge aside for the moment and moved to a double cone design as a model. Levin said, "It has axial symmetry - like a top, it has symmetry around all angles - making it a lot easier to compute."

The research provided new understanding about the points of transition in flow from smooth to turbulent, which can ultimately inform safer vehicle design.

Research Report: "On the unsteadiness of shock - laminar boundary layer interactions hypersonic flows over a double cone,"


Related Links
University of Illinois College of Engineering
Rocket Science News at Space-Travel.Com


Thanks for being there;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.
SpaceDaily Monthly Supporter
$5+ Billed Monthly


paypal only
SpaceDaily Contributor
$5 Billed Once


credit card or paypal


ROCKET SCIENCE
Soyuz launch failed due to assembly problem: Russia
Korolyov, Russia (AFP) Nov 1, 2018
Russia said on Thursday the launch of a Soyuz rocket failed last month because of a sensor that was damaged during assembly at the Baikonur cosmodrome but insisted that the spacecraft remains reliable. Russia, the only country able to ferry astronauts to the International Space Station, suspended all launches after a Soviet-designed Soyuz rocket failed on October 11 just minutes after blast-off - the first such incident in the history of post-Soviet space travel. Oleg Skorobogatov, the head of ... read more

Comment using your Disqus, Facebook, Google or Twitter login.



Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle

ROCKET SCIENCE
Russia plans first manned launch to ISS Dec 3 after accident

Thrusters with additively manufactured components qualified to fly humans on Orion spacecraft

Plant hormone makes space farming a possibility

Installing life support the hands-free way

ROCKET SCIENCE
Rocket Lab enters high frequency launch operations

Soyuz launch failed due to assembly problem: Russia

NASA conducts a 'BOO-tiful' RS-25 engine test

Soyuz launch failed due to assembly problem: Russia

ROCKET SCIENCE
Water cycle along the northern rim of Hellas Basin throughout Mars' history

Five things to know about InSight's Mars landing

Naturally occurring 'batteries' fueled organic carbon synthesis on Mars

NASA launches a new podcast to Mars

ROCKET SCIENCE
China's space programs open up to world

China's commercial aerospace companies flourishing

China launches Centispace-1-s1 satellite

China tests propulsion system of space station's lab capsules

ROCKET SCIENCE
Telstar 18 VANTAGE satellite now operational over Asia Pacific

How Max Polyakov from Zaporozhie develops the Ukrainian space industry

SpaceFund launches the world's first space security token to fund the opening of the high frontier

ESA on the way to Space19+ and beyond

ROCKET SCIENCE
Video game action heads for the cloud

Making steps toward improved data storage

Super-computer brings 'cloud' to astronauts in space

Disorder plays a key role in phase transitions of materials

ROCKET SCIENCE
NASA retires Kepler Space Telescope, passes planet-hunting torch

Rocky and habitable - sizing up a galaxy of planets

Some planetary systems just aren't into heavy metal

Giant planets around young star raise questions about how planets form

ROCKET SCIENCE
SwRI team makes breakthroughs studying Pluto orbiter mission

ALMA maps temperature of Jupiter's icy moon Europa

NASA's Juno Mission Detects Jupiter Wave Trains

WorldWide Telescope looks ahead to New Horizons' Ultima Thule glyby









The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us.