Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/2794| Title: | Radio pulsar emission altitudes |
| Authors: | Kapoor, R. C Shukre, C. S |
| Keywords: | Radio Pulsar Emission Altitudes Magnetic Field Line |
| Issue Date: | Sep-2002 |
| Publisher: | Astronomical Society of India |
| Citation: | BASI, Vol. 30, No. 3, pp. 695 - 696 |
| Abstract: | By attributing the often seen longitude offsets between the core and conal component centres of pulsar radio pulses to different emission altitudes, we present a new method for investigating these altitudes. OUf method can explain these offsets and also sheds light on them. |
| URI: | http://hdl.handle.net/2248/2794 |
| Appears in Collections: | BASI Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| kapoor.pdf | 32.89 kB | Adobe PDF | ![]() View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.
