Ting Xiao

ORCID: 0000-0003-1938-8669
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About
Contact & Profiles
Research Areas
  • Galaxies: Formation, Evolution, Phenomena
  • Meat and Animal Product Quality
  • Geomagnetism and Paleomagnetism Studies
  • Solar and Space Plasma Dynamics
  • Astronomy and Astrophysical Research
  • Astrophysics and Star Formation Studies
  • Ionosphere and magnetosphere dynamics
  • Microencapsulation and Drying Processes
  • Freezing and Crystallization Processes
  • Microbial Inactivation Methods
  • Metamaterials and Metasurfaces Applications
  • Antenna Design and Analysis
  • Stellar, planetary, and galactic studies
  • Advanced Antenna and Metasurface Technologies
  • Insect Utilization and Effects
  • Spectroscopy and Laser Applications
  • Bee Products Chemical Analysis
  • Listeria monocytogenes in Food Safety
  • Atmospheric and Environmental Gas Dynamics
  • Experimental and Theoretical Physics Studies
  • Astrophysical Phenomena and Observations
  • Proteins in Food Systems
  • Scientific Research and Discoveries
  • Dental Erosion and Treatment
  • Smart Materials for Construction

Zhejiang University
2019-2025

Ministry of Agriculture and Rural Affairs
2022-2025

CCCC Highway Consultants (China)
2024

Guangxi Veterinary Research Institute
2023

Jiangxi University of Finance and Economics
2023

Guilin University of Electronic Technology
2020

Shandong University
2012-2017

Shanghai Astronomical Observatory
2015-2017

Chinese Academy of Meteorological Sciences
2015

Chinese Academy of Sciences
2012-2015

An understanding of the transport solar wind plasma into and throughout terrestrial magnetosphere is crucial to space science weather. For non-active periods, there little agreement on where how entry might occur. Moreover, behaviour in high-latitude region behind magnetospheric cusps, for example, lobes, poorly understood, partly because lack coverage by previous missions. Here, using Cluster multi-spacecraft data, we report an unexpected discovery regions Earth's tailward cusps. From...

10.1038/ncomms2476 article EN cc-by-nc-sa Nature Communications 2013-02-12

Using HST observations of 147 host galaxies low-mass black holes (BHs), we systematically study the structures and scaling relations these active galaxies. Our sample is selected to have central BHs with virial masses ~10^5-10^6 solar mass. The total I-band magnitudes -23.2<M_I<-18.8 mag bulge -22.9<M_I<-16.1 mag. Detailed bulge-disk-bar decompositions GALFIT show that 93% extended disks, 39% bars 5% no bulges at all limits our observations. Based on Sersic index bulge-to-total ratio,...

10.1088/0004-637x/742/2/68 article EN The Astrophysical Journal 2011-11-07

Abstract. Magnetic holes with relatively small scale sizes, detected by Cluster and TC-1 in the magnetotail plasma sheet, are studied this paper. It is found that these magnetic spatial structures they not depressions generated flapping movement of current sheet. Most (93%) were observed during intervals Bz larger than Bx, i.e. more likely to occur a dipolarized field topology. Our results also suggest occurrence might have close relationship dipolarization process. The typically size...

10.5194/angeo-30-583-2012 article EN cc-by Annales Geophysicae 2012-03-26

Current densities associated with dipolarization fronts (DFs) have been calculated in the geomagnetic tail using curlometer technique applied to high‐resolution magnetic field data obtained by four Cluster spacecraft. We then use relation characterize behavior of field‐aligned current (FAC) during 25 DF events. Our results show that magnitude FAC density ( J // ) ranges from 5 20 nA/m 2 , and they are observed Northern Southern Hemispheres flowing along both directions ‐field. The FACs...

10.1002/grl.50902 article EN Geophysical Research Letters 2013-08-27

We study the spatially resolved star formation history and molecular gas distribution of 58 nearby galaxies, using integral field spectroscopy from CALIFA survey CO $J=1\rightarrow 0$ intensity mapping CARMA EDGE survey. use 4000 \AA\ break (D$_n$4000), equivalent width H$\delta$ absorption line (EW H$\delta_A$), H$\alpha$ emission H$\alpha$) to measure recent (SFH) these galaxies. radial profiles three SFH indicators mass surface density, which we level centrally enhanced concentration....

10.1093/mnras/stz349 article EN Monthly Notices of the Royal Astronomical Society 2019-02-01

We investigate the recent star formation history (SFH) in inner region of 57 nearly face-on spiral galaxies selected from Calar Alto Legacy Integral Field Area (CALIFA) survey. For each galaxy we use integral field spectroscopy CALIFA to obtain two-dimensional maps and radial profiles three parameters that are sensitive indicators SFH: 4000\AA\ break (D$_n$(4000)), equivalent width H$\delta$ absorption (EW(H$\delta_A$)) H$\alpha$ emission (EW(H$\alpha$)). have also performed photometric...

10.3847/1538-4357/aa657a article EN The Astrophysical Journal 2017-03-31

In this study, a self-cooling laboratory system was used for pressure−shift freezing (PSF), and the effects of (PSF) at 150 MPa on quality largemouth bass (Micropterus salmoides) during frozen storage −30 °C were evaluated compared with those conventional air (CAF) liquid immersion (LIF). The thawing loss cooking PSF significantly lower than CAF LIF whole period. loss, L* value, b* value TBARS fish increased storage. After 28 days storage, values 0.54 0.65, respectively, higher (p < 0.05)...

10.3390/foods11131842 article EN cc-by Foods 2022-06-22

Abstract Using data from ALFALFA, xGASS, H i -MaNGA, and the Sloan Digital Sky Survey (SDSS), we identify a sample of 47 “red but -rich” (RR) galaxies with near-UV (NUV) − r &gt; 5 unusually high -to-stellar mass ratios. We compare optical properties local environments between RR control -normal” (RN) that are matched in stellar color. The two samples similar typical massive red (quenched) Universe. tends to be associated slightly lower-density has lower clustering amplitudes smaller...

10.3847/1538-4357/ad1ce3 article EN cc-by The Astrophysical Journal 2024-03-01

Abstract The sudden enhancements of magnetic strength, named peaks (MPs), are often observed in the magnetosheath magnetized planets. They usually identified as flux ropes (FRs) or mirror mode structures. Previous studies MPs mostly on magnetohydrodynamics (MHD) scale. In this study, an electron scale MP is reported Earth magnetosheath. We present a typical case with ~7 gyroradii and duration ~0.18 s. A strong disturbance associated electrical current detected. Electron vortex found...

10.1002/2017gl075711 article EN cc-by-nc-nd Geophysical Research Letters 2017-12-29

Ensuring food safety and quality is paramount for consumers. Water, a fundamental component of food, exhibits diverse crystalline structures under high pressure (HP) experiences alterations in freezing points. Exploiting these water characteristics has spurred the development innovative high-pressure sub-zero temperature (HPST) techniques. This review systematically categorizes HPST technologies based on their adherence to temperature-pressure phase diagram, encompassing (HPF), thawing...

10.1080/87559129.2024.2370947 article EN Food Reviews International 2024-06-27

We present empirical relations between the global dust reddening and other physical galaxy properties including Hα luminosity, surface brightness, metallicity axial ratio for star-forming disc galaxies. The study is based on a large sample of ∼22 000 well-defined galaxies selected from Sloan Digital Sky Survey. parametrized by colour excess E(B−V) derived Balmer decrement. Besides dependency luminosity/surface brightness gas phase metallicity, it also correlated with inclination, in sense...

10.1111/j.1365-2966.2011.20327.x article EN Monthly Notices of the Royal Astronomical Society 2012-01-01

Abstract We present a new H i mass estimator that relates <?CDATA ${\mathrm{log}}_{10}$?> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msub> <mml:mrow> <mml:mi>log</mml:mi> </mml:mrow> <mml:mn>10</mml:mn> </mml:msub> </mml:math> ( M HI / * ) to linear combination of four galaxy properties: stellar surface density, color index u − r , mass, and concentration index, with the scatter individual galaxies around mean modeled Gaussian distribution function....

10.3847/1538-4357/ac9ccb article EN cc-by The Astrophysical Journal 2022-12-01

Abstract Using multipoint data from three Time History of Events and Macroscale Interactions during Substorms (THEMIS) satellites, we report a magnetospheric flow vortex driven by negative solar wind dynamic pressure pulse. The observed rotated in direction opposite to that associated with positive pulses. was moving tailward, as confirmed global magnetohydrodynamics (MHD) simulation. In addition, the equivalent ionospheric currents (EICs) deduced ground magnetometer station reveal current...

10.1002/2015ja021646 article EN Journal of Geophysical Research Space Physics 2015-09-29

Using data taken as part of the Bluedisk project, we study connection between neutral hydrogen (H i) in environment spiral galaxies and that themselves. We measure total H i mass present a statistical way by studying distribution noise peaks cubes obtained for 40 observed with Westerbork Synthesis Radio Telescope. find whose fraction is high relative to standard scaling relations have an excess surrounding well. Gas consists gas clumps which are individually below detection limit our data....

10.1093/mnras/stv1767 article EN Monthly Notices of the Royal Astronomical Society 2015-09-01
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