Asset Details
MbrlCatalogueTitleDetail
Do you wish to reserve the book?
Giant micropulse emission in the Vela pulsar at C band
by
Wen, Z G
, Li, Z X
, Mijit, M
, Yuen, R
, J Li
, Lee, K J
, Wang, N
, Xu, Y H
, Wang, H G
, Yuan, J P
, Yan, W M
, Chen, J L
, Huang, Y X
, Hao, L F
in
C band
/ Emission
/ Flux density
/ Pulsars
/ Radio telescopes
2020
Hey, we have placed the reservation for you!
By the way, why not check out events that you can attend while you pick your title.
You are currently in the queue to collect this book. You will be notified once it is your turn to collect the book.
Oops! Something went wrong.
Looks like we were not able to place the reservation. Kindly try again later.
Are you sure you want to remove the book from the shelf?
Oops! Something went wrong.
While trying to remove the title from your shelf something went wrong :( Kindly try again later!
Do you wish to request the book?
Giant micropulse emission in the Vela pulsar at C band
by
Wen, Z G
, Li, Z X
, Mijit, M
, Yuen, R
, J Li
, Lee, K J
, Wang, N
, Xu, Y H
, Wang, H G
, Yuan, J P
, Yan, W M
, Chen, J L
, Huang, Y X
, Hao, L F
in
C band
/ Emission
/ Flux density
/ Pulsars
/ Radio telescopes
2020
Please be aware that the book you have requested cannot be checked out. If you would like to checkout this book, you can reserve another copy
We have requested the book for you!
Your request is successful and it will be processed during the Library working hours. Please check the status of your request in My Requests.
Oops! Something went wrong.
Looks like we were not able to place your request. Kindly try again later.
Paper
Giant micropulse emission in the Vela pulsar at C band
J Li,
2020
Request Book From Autostore
and Choose the Collection Method
Overview
We present here the analysis of giant micropulses from the Vela pulsar. A total of 4187 giant micropulses with peak flux density \\(>\\)2.5 Jy were detected during almost 4 hours of observations carried out with the Yunnan 40-m radio telescope at 6800 MHz. Nine of the giant micropulses arrived approximately 3 to 4 ms earlier than the peak of average pulse profile, longer than that at lower frequencies. The remaining giant micropulses were clustered into three distributions which correspond to three main emission regions, including four occurring on the trailing edge of averaged profile.
Publisher
Cornell University Library, arXiv.org
Subject
This website uses cookies to ensure you get the best experience on our website.