MEASUREMENT OF INTERSTELLAR MAGNETIC FIELD

被引：40

作者：

SMITH, FG

机构：

[1] University of Manchester, Nuffield Radio Astronomy Laboratories

来源：

NATURE | 1968年 / 218卷 / 5139期

关键词：

D O I：

10.1038/218325a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

The discovery that signals from pulsating radio sources are linearly polarized means that interstellar magnetic fields in the local part of the Galaxy can be measured. © 1968 Nature Publishing Group.

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页码：325 / &

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共 3 条

[1] PULSATING RADIO SOURCE AT ALPHA=19H19M BETA=+22 DEGREES
DAVIES, JG
HORTON, PW
LYNE, AG
RICKETT, BJ
SMITH, FG
[J]. NATURE, 1968, 217 (5132) : 910 - &
[2] OBSERVATION OF A RAPIDLY PULSATING RADIO SOURCE
HEWISH, A
BELL, SJ
PILKINGT.JD
SCOTT, PF
COLLINS, RA
[J]. NATURE, 1968, 217 (5130) : 709 - &
[3] LINEAR POLARIZATION IN PULSATING RADIO SOURCES
LYNE, AG
SMITH, FG
[J]. NATURE, 1968, 218 (5137) : 124 - &