Skip to main content

The Solar Spectrum

Proceedings of the Symposium held at the University of Utrecht 26–31 August 1963

  • Conference proceedings
  • © 1965

Overview

Part of the book series: Astrophysics and Space Science Library (ASSL, volume 1)

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

Access this book

eBook USD 74.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever

Tax calculation will be finalised at checkout

Other ways to access

Licence this eBook for your library

Institutional subscriptions

Table of contents (22 papers)

  1. Opening Address

  2. Fourty Years of Solar Spectroscopy

  3. The Photosphere

  4. The Quiet Chromosphere

  5. The Active Photosphere and Chromosphere; Spots, Plages, Flares and Prominences

  6. The Corona

Keywords

About this book

A good deal of our information on solar physics and on solar phenomena is derived from the solar spectrum. A quantitative interpretation of this spectrum was only possible after 1920, after the establishment of Bohr's atomic model, the discovery of Saha's law, and the development of spectrophotometry. The resolving and light gathering powers of our instruments have greatly increased since. We have seen an enormous progress in our theoretical under­ standing of basic atomic phenomena, and of the intricate problems concerned with the transfer of energy through a complicated structure like the sun's outer layers. In particular the observable part of the solar spectrum tremen­ dously enlarged since the introduction, in the years after 1945, of radio­ astronomy, enabling us to study the solar spectrum between wavelengths of some mm to about 15 m, of space research, giving access to the whole electro­ magnetic spectrum below 3000 A, down to about 0. 01 A. Further, the low and high energetic components of the solar particles spectrum have been dis­ covered with space probes (the solar wind), rockets, balloons (the so-called sub­ cosmic-ray particles) and cosmic ray monitors (solar cosmic ray bursts). The extreme wealth of this spectrum, much vaster in extent than the earlier investigators could only dream of, is an important source of information. It looked appropriate to us, after the rapid development of this branch of science,' to invite the world's leading solar physicists to Utrecht for a summa­ rizing symposium on the whole solar spectrum.

Bibliographic Information

  • Book Title: The Solar Spectrum

  • Book Subtitle: Proceedings of the Symposium held at the University of Utrecht 26–31 August 1963

  • Editors: C. Jager

  • Series Title: Astrophysics and Space Science Library

  • DOI: https://doi.org/10.1007/978-94-010-3587-3

  • Publisher: Springer Dordrecht

  • eBook Packages: Springer Book Archive

  • Copyright Information: D. Reidel Publishing Company, Dordrecht - Holland 1965

  • eBook ISBN: 978-94-010-3587-3Published: 06 December 2012

  • Series ISSN: 0067-0057

  • Series E-ISSN: 2214-7985

  • Edition Number: 1

  • Number of Pages: 431

  • Topics: Astrophysics and Astroparticles

Publish with us