Using a new method of multi-frequency of K parameter, we estimate the ratio of altitudes of radio emission region of pulsars at 430 and 1418 MHz. The value of the ratio is 1.34+/-0.12 and the power law index of altitude-frequency is 0.24+/-0.08. It is indicated that the lower radio frequencies originate further out and the emission region is radially narrow.http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000079124600026&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=8e1609b174ce4e31116a60747a720701Physics, MultidisciplinarySCI(E)中国科学引文数据库(CSCD)4ARTICLE174-751
It is found that pulsar radiation altitude ratios between different radio frequencies are weak-depen...
Using the method of Gaussian Fit Separation of Average Profile (GFSAP), we re-examine the average pr...
We have observed a total of 67 pulsars at five frequencies ranging from 243 to 3100 MHz. Observation...
An important parameter in the study of the radial structure of the pulsar radio emission region is t...
Pulsar evolution is discussed for the first time by term of a new parameter K in a K-lgt(c) diagram ...
Emission geometries, including emission region heights, beam shapes and radius-to-frequency mapping,...
Contains fulltext : 36190.pdf (publisher's version ) (Open Access)This thesis cons...
The region in which pulsars radiate is very important to constrain pulsar emission mechanisms. A thr...
Abstract. We have collected pulsar flux density observa-tions and compiled spectra of 281 objects. T...
The region in which pulsars radiate is very important to constrain pulsar emission mechanisms. A thr...
We investigate radio emission efficiency, xi, of pulsars and report a near-linear inverse correlatio...
We have observed a total of 67 pulsars at five frequencies ranging from 243 to 3100 MHz. Observation...
Presented at the 21st meeting of the Astronomical Society of India, Pune, 2002.By attributing the of...
Many models for the pulsar radio and gamma-ray emissions have been developed. The tests for these mo...
The method of emission altitude estimation in radio pulsars based on pulse width measurements at the...
It is found that pulsar radiation altitude ratios between different radio frequencies are weak-depen...
Using the method of Gaussian Fit Separation of Average Profile (GFSAP), we re-examine the average pr...
We have observed a total of 67 pulsars at five frequencies ranging from 243 to 3100 MHz. Observation...
An important parameter in the study of the radial structure of the pulsar radio emission region is t...
Pulsar evolution is discussed for the first time by term of a new parameter K in a K-lgt(c) diagram ...
Emission geometries, including emission region heights, beam shapes and radius-to-frequency mapping,...
Contains fulltext : 36190.pdf (publisher's version ) (Open Access)This thesis cons...
The region in which pulsars radiate is very important to constrain pulsar emission mechanisms. A thr...
Abstract. We have collected pulsar flux density observa-tions and compiled spectra of 281 objects. T...
The region in which pulsars radiate is very important to constrain pulsar emission mechanisms. A thr...
We investigate radio emission efficiency, xi, of pulsars and report a near-linear inverse correlatio...
We have observed a total of 67 pulsars at five frequencies ranging from 243 to 3100 MHz. Observation...
Presented at the 21st meeting of the Astronomical Society of India, Pune, 2002.By attributing the of...
Many models for the pulsar radio and gamma-ray emissions have been developed. The tests for these mo...
The method of emission altitude estimation in radio pulsars based on pulse width measurements at the...
It is found that pulsar radiation altitude ratios between different radio frequencies are weak-depen...
Using the method of Gaussian Fit Separation of Average Profile (GFSAP), we re-examine the average pr...
We have observed a total of 67 pulsars at five frequencies ranging from 243 to 3100 MHz. Observation...