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Sep 07, 2015

Improvements of Xinjiang Astronomical Observatory in the Recognition of Pulsar Signals

Recently, the associate professor Hao Shan in the Xinjiang Astronomical Observatory (XAO) of Chinese Academy of Sciences (CAS) implemented classification and recognition for 401 observed radio pulsar signals in the frequency range of 1.4...
Jul 24, 2015

Professor Christian Henkel from Max Planck Institute for Radio Astronomy, Germany, Visited Xinjiang Astronomical Observatory

During June 23rd to July 22nd, 2015, Professor Christian Henkel, the Distinguished Research Fellow in Xinjiang Astronomical Observatory (XAO), from Max Planck Institute for Radio Astronomy visited XAO.During his visit, Professor Henkel h...
Jul 22, 2014

Pulsar wind model for the spin-down behavior of intermittent pulsars

Intermittent pulsars are part-time radio pulsars. They have higher slow down rates in the on state (radio-loud) than in the off state (radio-quiet). This gives evidence that particle wind may play an important role in pulsar spin-down.LI...
Jul 22, 2014

Electron Cyclotron Maser Emission in Coronal Arches and Solar Radio Type V Bursts

According to the close association of type V solar bursts with type III bursts, we propose that solar radio type V bursts are excited by the electron cyclotron maser instability. The work by J. F. Tang, D. J. Wu and C. M. Tan has been pu...
Nov 25, 2013

Particle Simulations Reveal Small-Scale Energy Dissipation of Solar Storm

Because the transportation of energy from a solar storm is a large scale problem, in the long term, the Magnetohydrodynamics (MHD) method can better resolve processes related to transportation of the solar wind in the heliosphere.However...
Nov 20, 2013

XAO Developed the OTF Observation Model to Improve Observing Efficiency

OTF model is an observation method which controls the telescope moving uniformly, in the same time, recording the spectrum line data in a high sample rate, to finish a map of specifically region. OTF model can highly improve the efficien...

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