Capillary channel flow experiments aboard the International Space Station

M. Conrath, P. J. Canfield, P. M. Bronowicki, M. E. Dreyer, M. M. Weislogel, and A. Grah
Phys. Rev. E 88, 063009 – Published 10 December 2013

Abstract

In the near-weightless environment of orbiting spacecraft capillary forces dominate interfacial flow phenomena over unearthly large length scales. In current experiments aboard the International Space Station, partially open channels are being investigated to determine critical flow rate-limiting conditions above which the free surface collapses ingesting bubbles. Without the natural passive phase separating qualities of buoyancy, such ingested bubbles can in turn wreak havoc on the fluid transport systems of spacecraft. The flow channels under investigation represent geometric families of conduits with applications to liquid propellant acquisition, thermal fluids circulation, and water processing for life support. Present and near future experiments focus on transient phenomena and conduit asymmetries allowing capillary forces to replace the role of gravity to perform passive phase separations. Terrestrial applications are noted where enhanced transport via direct liquid-gas contact is desired.

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  • Received 8 May 2013

DOI:https://doi.org/10.1103/PhysRevE.88.063009

©2013 American Physical Society

Authors & Affiliations

M. Conrath1, P. J. Canfield1, P. M. Bronowicki1, M. E. Dreyer1,*, M. M. Weislogel2, and A. Grah3

  • 1Center of Applied Space Technology and Microgravity (ZARM), University of Bremen, Am Fallturm 01, 28359 Bremen, Germany
  • 2Department of Mechanical and Materials Engineering, Portland State University, PO Box 751, Portland, Oregon 97207, USA
  • 3European Commission, Institute for Energy and Transport, Petten, The Netherlands

  • *Corresponding author: michael.dreyer@zarm.uni-bremen.de

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Issue

Vol. 88, Iss. 6 — December 2013

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