Biqiang Zhao

Dr. Biqiang Zhao

Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China

Research Focus & Metrics

Academic Career Length

24Years (2003-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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17 September 2024 in Journal of Geophysical Research: Space Physics
Verified
Journal Article
Closed access
XGXu Guo
Xu Guo
Biqiang ZhaoBiqiang Zhao
Biqiang Zhao
TYTingting Yu
Tingting Yu
HHHonglian Hao
Honglian Hao
WSWenjie Sun
Wenjie Sun
ZRZhipeng Ren
Zhipeng Ren

23 August 2022 in Journal of Geophysical Research: Space Physics
Verified
Journal Article
Open access
XYXinan Yue
Xinan Yue
WWWeixing Wan
Weixing Wan
BNBaiqi Ning
Baiqi Ning
LJLin Jin
Lin Jin
FDFeng Ding
Feng Ding
FLFanyu Liu
Fanyu Liu
Led by the Institute of Geology and Geophysics, Chinese Academy of Sciences, we have built a brand‐new modular active digital phased array, with all solid‐state transmission and digital receiving incoherent scatter radar (ISR) in Sanya (18.3°N, 109.6°E), a station in low latitude China called Sanya ISR (SYISR) since 2015. The development of SYISR involved the indoor design and development of key components, an outdoor prototype test, and the production and debugging of the entire array. The unique features of SYISR include a single‐channel directly connected T/R unit and antenna, a radar array monitoring and calibration network, environmental adaptability design and open architecture. The entire radar has 4,096 channels and 5,930 modules in total. All the technical indices, mainly including a >2 MW peak power, a 43 dBi antenna gain and a <120 K noise temperature, either meet or are superior to the designed value through an independent evaluation. Waveforms of single pulse, linear frequency modulation, Barker code, long pulse and alternating code have been implemented to meet multiple purposes. Four observational modes for ionospheric experiments, including zenith stare, perpendicular to geomagnetic field, meridian scan, and all sky scan, have been developed. We have implemented time domain decoding, frequency domain decoding, and statistical inversion methods in calculating the autocorrelation function and power spectra in signal processing. The preliminary experimental results on ionospheric parameters, plasma lines, irregularities and hard targets are reasonable and encouraging, which greatly enhances our confidence in achieving our scientific goals in the future.

31 January 2013 in Journal of Geophysical Research: Space Physics
Verified
Journal Article
Closed access
PDF file
Biqiang ZhaoBiqiang Zhao
Biqiang Zhao
MWMin Wang
Min Wang
YWYungang Wang
Yungang Wang
ZRZhipeng Ren
Zhipeng Ren
XYXinan Yue
Xinan Yue
BXBo Xiong
Bo Xiong

22 December 2024 in Journal of Geophysical Research: Space Physics
Verified
Journal Article
Closed access
WSWenjie Sun
Wenjie Sun
Guozhu LiGuozhu Li
Guozhu Li
SZShun‐Rong Zhang
Shun‐Rong Zhang
Biqiang ZhaoBiqiang Zhao
Biqiang Zhao
YLYu Li
Yu Li
LLLibo Liu
Libo Liu

29 October 2024 in Geophysical Research Letters
Verified
Journal Article
Open access
WSWenjie Sun
Wenjie Sun
Guozhu LiGuozhu Li
Guozhu Li
Biqiang ZhaoBiqiang Zhao
Biqiang Zhao
SZShun‐Rong Zhang
Shun‐Rong Zhang
Yuichi OtsukaYuichi Otsuka
Yuichi Otsuka
SPSepti Perwitasari
Septi Perwitasari
Plasma blob is generally a low‐latitude phenomenon occurring at the poleward edge of equatorial plasma bubble (EPB) during post‐sunset periods. Here we report a case of midlatitude ionospheric plasma blob‐like structures occurring along with super EPBs over East Asia around sunrise during the May 2024 great geomagnetic storm. Interestingly, the blob‐like structures appeared at both the poleward and westward edges of EPBs, reached up to 40°N magnetic latitudes, and migrated westward several thousand kilometers together with the bubble. The total electron content (TEC) inside the blob‐like structures was enhanced by ∼50 TEC units relative to the ambient ionosphere. The blob‐like structure at the EPB poleward edge could be partly linked with field‐aligned plasma accumulation due to poleward development of bubble. For the blob‐like structure at the EPB west side, one possible mechanism is that it was formed and enhanced accompanying the bubble evolution and westward drift.

16 July 2010 in International Journal of Remote Sensing
Verified
Journal Article
Closed access
Biqiang ZhaoBiqiang Zhao
Biqiang Zhao
MWMin Wang
Min Wang
TYTao Yu
Tao Yu
GXGuirong Xu
Guirong Xu
WWWeixing Wan
Weixing Wan
LLLibo Liu
Libo Liu
On 12 May 2008 at 06:28 UT a major earthquake of magnitude 8.0 struck Wenchuan County (31.0° N, 103.4° E) in southwest China. Ionospheric total electron content (TEC) values, derived from a network of 58 global positioning system (GPS) receivers over China and nearby countries, were used to investigate the ionospheric precursor of the great earthquake. The observations revealed that there was an anomalous enhancement in TEC (100% increase on the 15-day median) during the afternoon–evening sector on 9 May 2008 while geomagnetic conditions were quiet (Kp ≤ 2). The TEC variations on the west side and east side of the epicentre show large dissimilarity on 9 May 2008. By constructing the longitude/latitude TEC map, the distribution of the region predominated by increased TEC values was shown to be localized at longitudes 90–130° E. Our results suggest that this abnormal enhancement was most possibly a seismo-ionospheric signature.