Prompt nuclear EMP and Synchrotron radiation: a resolution of two approaches

The geomagnetic component of nuclear EMP generated by the prompt (t/sub max//spl sim/2 /spl mu/s) /spl gamma/-ray, neutron, and X-ray radiation from a nuclear explosion has been the subject of intense scrutiny for over 40 years. Recent work by certain members of the scientific community has suggeste...

Full description

Saved in:
Bibliographic Details
Published inIEEE transactions on electromagnetic compatibility Vol. 47; no. 3; pp. 552 - 558
Main Author Roussel-Dupre, R.A.
Format Journal Article
LanguageEnglish
Published New York, NY IEEE 01.08.2005
Institute of Electrical and Electronics Engineers
The Institute of Electrical and Electronics Engineers, Inc. (IEEE)
Subjects
Online AccessGet full text
ISSN0018-9375
1558-187X
DOI10.1109/TEMC.2005.851724

Cover

Loading…
More Information
Summary:The geomagnetic component of nuclear EMP generated by the prompt (t/sub max//spl sim/2 /spl mu/s) /spl gamma/-ray, neutron, and X-ray radiation from a nuclear explosion has been the subject of intense scrutiny for over 40 years. Recent work by certain members of the scientific community has suggested that a discrepancy exists in the calculations/derivation of nuclear EMP between treatments based on Maxwell's equations and the high-frequency approximation and those derived from a summation over particles emitting synchrotron radiation. In principle, the two approaches should be identical simply because the well-known Lie/spl acute/nard-Wiechert potentials for accelerating particles are derived from Maxwell's equations. In this paper, we start from the Lie/spl acute/nard-Wiechert potentials and derive an expression for nuclear EMP that is identical to previous work based on a solution of Maxwell's equations. Thus, the putative discrepancy between the two approaches is resolved and Maxwell's equations in this regard are again vindicated.
Bibliography:ObjectType-Article-2
SourceType-Scholarly Journals-1
ObjectType-Feature-1
content type line 14
ObjectType-Article-1
ObjectType-Feature-2
content type line 23
ISSN:0018-9375
1558-187X
DOI:10.1109/TEMC.2005.851724