Skip to main content

Ambipolar Diffusion

  • Reference work entry
Encyclopedia of Astrobiology
  • 293 Accesses

Definition

Ambipolar diffusion is the slippage of neutral matter in a plasma with respect to an internal magnetic field. This slippage occurs when the ionization fraction is so low that collisions between neutral species and ions become relatively rare. At this point, the neutral atoms can move relative to the ions, which are effectively tied to the magnetic field. Ambipolar diffusion is thought to occur in molecular clouds, which are dense enough to shield much of the external, ionizing radiation. The cloud’s self-gravity can then cause the gas to condense, in spite of its internal magnetic field. This condensation ultimately leads to star formation.

See also

Collapse, Gravitational

Dense Core

Fragmentation (Interstellar Clouds)

Molecular Cloud

Star Formation

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 749.99
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Steven Stahler .

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 2011 Springer-Verlag Berlin Heidelberg

About this entry

Cite this entry

Stahler, S. (2011). Ambipolar Diffusion. In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-11274-4_59

Download citation

Publish with us

Policies and ethics