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  • Book
  • © 2011

Principles of Stellar Interferometry

  • Enables PhD students and scientist specialised in other fields to start a research project in interferometry
  • Pedagogically and carefully written with detailed explanations
  • Well illustrated with line-drawings, greyscale and colour figures
  • Based on the author's longtime experience in ESO's Very Large Telescope Interferometer team
  • Includes supplementary material: sn.pub/extras

Part of the book series: Astronomy and Astrophysics Library (AAL)

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Table of contents (8 chapters)

  1. Front Matter

    Pages i-xvii
  2. Introduction

    • Andreas Glindemann
    Pages 1-4
  3. Propagation of Light

    • Andreas Glindemann
    Pages 5-72
  4. Atmospheric Turbulence

    • Andreas Glindemann
    Pages 157-215
  5. Instrumental Techniques

    • Andreas Glindemann
    Pages 217-274
  6. Observing Through Atmospheric Turbulence

    • Andreas Glindemann
    Pages 275-315
  7. Modern Interferometers

    • Andreas Glindemann
    Pages 317-318
  8. Erratum

    • Andreas Glindemann
    Pages E1-E2
  9. Back Matter

    Pages 319-342

About this book

Over the last decade, stellar interferometry has developed from a specialist tool to a mainstream observing technique, attracting scientists whose research benefits from milliarcsecond angular resolution. Stellar interferometry has become part of the astronomer’s toolbox, complementing single-telescope observations by providing unique capabilities that will advance astronomical research.

This carefully written book is intended to provide a solid understanding of the principles of stellar interferometry to students starting an astronomical research project in this field or to develop instruments and to astronomers using interferometry but who are not interferometrists per se.

Illustrated by excellent drawings and calculated graphs

  • the imaging process in stellar interferometers is explained starting from first principles on light propagation and diffraction,
  • wave propagation through turbulence is described in detail using Kolmogorov statistics,
  • the impact of turbulence on the imaging process is discussed both for single telescopes and for interferometers,
  • instrumental techniques like beam combination and array layout are described, and the requirements for delay lines are derived,
  • visibility measurements (modulus and phase) through turbulence are analyzed and limitations are quantified,
  • correction methods (fringe tracking and adaptive optics) are presented, discussing closed loop operation with a dual feed system.
The book closes with examples of contemporary stellar interferometers and useful appendices on the Fourier transform and atmospheric transmission bands.

Authors and Affiliations

  • European Southern Observatory (ESO), Garching, Germany

    Andreas Glindemann

Bibliographic Information

Buy it now

Buying options

eBook USD 89.00
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 119.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book USD 169.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access