Skip to main content Accessibility help
×
Home

Radio Radiation Characteristics of Pulsars and Magnetic Dipole Angle

  • Wang Zhen-ru (a1) and Chu Yi (a1)

Extract

The structure of the pulsar magnetosphere, the location of the radio emission region and the radio emission mechanism are important theoretical subjects in the research of pulsars. There may be close relations between these subjects. Nevertheless, it should be possible to set up some empirical relations among them which can be considered as a foundation for studying these important subjects. In this paper some of these relations are studied.

    • Send article to Kindle

      To send this article to your Kindle, first ensure no-reply@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about sending to your Kindle. Find out more about sending to your Kindle.

      Note you can select to send to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be sent to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

      Find out more about the Kindle Personal Document Service.

      Radio Radiation Characteristics of Pulsars and Magnetic Dipole Angle
      Available formats
      ×

      Send article to Dropbox

      To send this article to your Dropbox account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Dropbox.

      Radio Radiation Characteristics of Pulsars and Magnetic Dipole Angle
      Available formats
      ×

      Send article to Google Drive

      To send this article to your Google Drive account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Google Drive.

      Radio Radiation Characteristics of Pulsars and Magnetic Dipole Angle
      Available formats
      ×

Copyright

References

Hide All
Backer, D.C.: 1976, Astrophys. J. 209, p. 895.
Ferguson, D.C.: 1977, Astron. Astrophys. 54, p. 355.
Henry, G.R. and Park, H.J.: 1969, Nature 224, p. 1188.
Lyne, A.G. and Smith, F.G.: 1979, Mon. Not. R. Astr. Soc. 188, p. 675.
Qin-yue, Qu, Zhen-ru, Wang, Tan, Lu, and Liao-fu, Luo: 1976, Kexue Tongbao 21, No. 4, p. 176.

Metrics

Full text views

Total number of HTML views: 0
Total number of PDF views: 0 *
Loading metrics...

Abstract views

Total abstract views: 0 *
Loading metrics...

* Views captured on Cambridge Core between <date>. This data will be updated every 24 hours.

Usage data cannot currently be displayed