Late-Time Sources for Close-In EMP (Electromagnetic Pulses)

Abstract

The report describes calculations of ionization rates and electric currents in air and ground resulting from neutron sources. In particular, the report describes the numerical methods, nuclear data, and computer programs employed and presents results for a typical thermonuclear neutron spectrum. A discussion of fitting of earlier electromagnetic pulse (EMP) source calculations is also presented. The latest ENDF/B neutron transport and gamma ray production data for air and ground are used and sensitivity of EMP calculations to cross section changes have been estimated. A new source energy band version of the Monte Carlo code 05RNIES has been developed which makes it possible to compute EMP sources by folding in various desired neutron spectra. New analytical approaches have also been introduced to accurately treat neutron capture events in air to times as late as one second. Analytical gamma-ray transport calculations away from the air-ground interface are used. Various neutron and gamma-ray contributions to ionization rates and electric currents have been tabulated as functions of fast and thermal reactions to assist in fitting of these quantities.

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Document Details

Document Type
Technical Report
Publication Date
Aug 01, 1972
Accession Number
AD0763489

Entities

People

  • Charles A. Stevens
  • David A. Sargis
  • Ernest R. Parkinson
  • John N. Wood
  • Ronald E. Dietz

Tags

Communities of Interest

  • Energy and Power Technologies

DTIC Thesaurus Topics

  • Absorption Cross Sections
  • Band Structures
  • Charged Particles
  • Computer Programs
  • Computers
  • Diffusion Theory
  • Elastic Scattering
  • Electric Current
  • Energy Bands
  • Energy Levels
  • Gamma Rays
  • Inelastic Scattering
  • Ionization
  • Neutron Capture
  • Neutron Capture Gamma Rays
  • Neutron Reactions
  • Neutron Spectrum

Fields of Study

  • Physics

Readers

  • Calculus or Mathematical Analysis
  • Optical Fiber Sensing and Electromagnetic Propagation.
  • Solar Physics