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CAS IR Grid
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长春光学精密机械与物... [1]
西双版纳热带植物园 [1]
昆明植物研究所 [1]
高能物理研究所 [1]
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OAI收割 [4]
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期刊论文 [3]
会议论文 [1]
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2020 [1]
2016 [2]
2011 [1]
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The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition
期刊论文
OAI收割
Monthly Notices of the Royal Astronomical Society, 2020, 卷号: 494, 页码: 1865-1870
作者:
HXMT
  |  
收藏
  |  
浏览/下载:54/0
  |  
提交时间:2022/02/08
stars: magnetic field
stars: neutron
pulsars: general
Astrophysics
- High Energy Astrophysical Phenomena
Abstract: In 2011 December, PSR B054-69 experienced a spin-down rate transition (SRT), after which the spin-down power of the pulsar increased by $\sim 36{{\ \rm per\ cent}}$. About 1000 d after the SRT, the X-ray luminosity of the associated pulsar wind nebula (PWN) was found to brighten by $32\pm 8{{\ \rm per\ cent}}$. After the SRT, the braking index n of PSR B0540-69 changes from n = 2.12 to 0.03 and then keeps this value for about five years before rising to n = 0.9 in the following years. We find that most of the current models have difficulties in explaining the measured braking index. One exceptive model of the braking index evolution is the increasing dipole magnetic field of PSR B0540-69. We suggest that the field increase may result from some instabilities within the pulsar core that enhance the poloidal component at the price of toroidal component of the magnetic field. The increasing dipole magnetic field will result in the X-ray brightening of the PWN. We fit the PWN X-ray light curve by two models: one assumes a constant magnetic field within the PWN during the brightening and the other assumes an enhanced magnetic field proportional to the energy density of the PWN. It appears that the two models fit the data well, though the later model seems to fit the data a bit better. This provides marginal observational evidence that magnetic field in the PWN is generated by the termination shock. Future high-quality and high-cadence data are required to draw a solid conclusion.
Responses of Photosystem I Compared with Photosystem II to Fluctuating Light in the Shade-Establishing Tropical Tree Species Psychotria henryi
期刊论文
OAI收割
FRONTIERS IN PLANT SCIENCE, 2016, 卷号: 7
作者:
Huang, Wei
;
Yang, Ying-Jie
;
Hu, Hong
;
Zhang, Shi-Bao
收藏
  |  
浏览/下载:32/0
  |  
提交时间:2017/01/05
constant high light
fluctuating light
PSI photoinhibition
excess excitation energy
shade-establishing species
Responses of Photosystem I Compared with Photosystem II to Fluctuating Light in the Shade-Establishing Tropical Tree Species Psychotria henryi
期刊论文
OAI收割
FRONTIERS IN PLANT SCIENCE, 2016, 卷号: 7, 期号: x, 页码: 1549
Huang, Wei
;
Yang, Ying-Jie
;
Hu, Hong
;
Zhang,Shi-Bao
收藏
  |  
浏览/下载:23/0
  |  
提交时间:2016/11/17
constant high light
fluctuating light
PSI photoinhibition
excess excitation energy
shade-establishing species
Design of programmable near infrared cold light source (EI CONFERENCE)
会议论文
OAI收割
2011 International Conference on Electronics and Optoelectronics, ICEOE 2011, July 29, 2011 - July 31, 2011, Dalian, China
作者:
Fu Q.
;
Wang B.
;
Wang B.
;
Wang R.
收藏
  |  
浏览/下载:30/0
  |  
提交时间:2013/03/25
In the near infrared spectroscopy
detector of Charge-coupled Device requires very high stability for light source. We design the cold light source in the measurement of near infrared spectroscopy. Cold light source consists of high-power op amp OPA549 high current constant current source and proportion integral differential (PID) control algorithm. As is shown in the experimental results
the method is better
the overshoot is very small
the stability is excellent in the process of soft-start. While light intensity was able to meet the requirements of near-infrared instruments to measure. 2011 IEEE.