caa a22 4500 475821238 CHVBK 20180406123819.0 cr unu---uuuuu 170329e20000101xx s 000 0 eng 10.1007/BF02513003 doi (NATIONALLICENCE)springer-10.1007/BF02513003 Method of kinematic projecting of pulsar-emission profiles [Elektronische Daten] [V. Bordovitsyn, V. Épp, V. Gushchina, V. Bulenok] A method for constructing profiles of incoherent pulsar emission based on the instantaneous angular phase distribution function of radiant power emitted by a relativistic source that moves in the magnetosphere of a neutron star is suggested. In general, this phase function depends on the kinematic parameters of the radiation source (its velocity and acceleration) and on the direction of radiation emission with respect to the rotating neutron star (the observation direction). The method is illustrated by the example of calculated profiles of fan pulsar radiation with the use of the phase function of synchrotron radiation. It is stated that his method can easily be generalized for other types of relativistic radiation. Kluwer Academic/Plenum Publishers, 2000 Bordovitsyn V. aut Épp V. aut Gushchina V. aut Bulenok V. aut Russian Physics Journal Kluwer Academic Publishers-Plenum Publishers 43/1(2000-01-01), 23-27 1064-8887 43:1<23 2000 43 11182 https://doi.org/10.1007/BF02513003 text/html Onlinezugriff via DOI 1 research-article jats NATIONALLICENCE 856 40 https://doi.org/10.1007/BF02513003 text/html Onlinezugriff via DOI NATIONALLICENCE 700 1- Bordovitsyn V. aut NATIONALLICENCE 700 1- Épp V. aut NATIONALLICENCE 700 1- Gushchina V. aut NATIONALLICENCE 700 1- Bulenok V. aut NATIONALLICENCE 773 0- Russian Physics Journal Kluwer Academic Publishers-Plenum Publishers 43/1(2000-01-01), 23-27 1064-8887 43:1<23 2000 43 11182 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer