Solute transport and interface evolution in dissolutive wetting

Yang, Jinhong; Yuan, Quanzi; Zhao, Ya‐Pu

doi:10.1007/s11433-019-9425-y

Cited by 15 publications

(21 citation statements)

References 27 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…This indicates that the p/p data can yield compatible results on δ 2 with the B/C data. However, as seen from Figure 2, DR-LR model can not reproduce the PAMELA 2 H/ 4 He, 3 He/ 4 He data and p/p below 1 GeV. By adding the 2 H/ 4 He and 3 He/ 4 He ratios in the fitting, the estimated low-energy parameters, such as δ 1 , ∆δ or v A , are slightly varied compared with the PDbr-LR and DR-LR models.…”

Section: B Fit To the Light Elementsmentioning

confidence: 92%

“…However, as seen from Figure 2, DR-LR model can not reproduce the PAMELA 2 H/ 4 He, 3 He/ 4 He data and p/p below 1 GeV. By adding the 2 H/ 4 He and 3 He/ 4 He ratios in the fitting, the estimated low-energy parameters, such as δ 1 , ∆δ or v A , are slightly varied compared with the PDbr-LR and DR-LR models. These parameters influence the evaluation on high-energy diffusion slope, thus the δ 2 values are varied to 0.373 ± 0.008 for PDbr-L model and 0.351 ± 0.008 for DR-L model.…”

Section: B Fit To the Light Elementsmentioning

confidence: 92%

“…The corresponding models are suffixed with "-LR". Then we include the 2 H/ 4 He and 3 He/ 4 He data in the analyses. The corresponding models are suffixed with "-L".…”

Section: B Fit To the Light Elementsmentioning

confidence: 99%

“…Therefore, the secondary-to-primary ratios reflect the propagation characteristics of cosmic rays. In previous theoretical studies, the cosmic ray propagation paradigm is commonly established by using the boron-to-carbon (B/C) ratio [1][2][3][4][5]. But the importance of other secondary-to-primary ratios, especially the low-mass ones has been emphasized in literatures [6][7][8][9].…”

Section: Introductionmentioning

confidence: 99%

“…Since the AMS02 measurements cover a complex polarity reversal period in Heliospheric magnetic field (HMF) for which the solar effect is difficult to model, we only deal with the AMS02 data [21][22][23][24][25][26] (including p, He, C, p/p, Li/C, Be/C, B/C) with energies larger than 20 GeV. On the contrary, no cut is performed on the PAMELA data [28][29][30][31] (including p, He, C, p/p, 2 H/ 4 He, 3 He/ 4 He, B/C), since the PAMELA data was collected during a solar minimum period from 2006 to 2008, and the solar modulation during this period is simpler and easier to describe. We also employ the low-energy B/C and C data measured by ACE-CRIS [54] during the same observational time of PAMELA.…”

Section: Introductionmentioning

confidence: 99%

See 4 more Smart Citations

Testing the consistency of proapgation between light and heavy cosmic ray nuclei

Wang,

Wu,

Long

2021

Preprint

View full text Add to dashboard Cite

One of the fundamental issues in cosmic ray physics is to explain the nature of cosmic ray acceleration and propagation mechanisms. Thanks to the precise cosmic ray data measured by recent space experiments, we are able to investigate the cosmic ray acceleration and propagation models more comprehensively and reliably. In this paper, we combine the secondary-to-primary ratios and the primary spectra measured by PAMELA, AMS02, ACE-CRIS and Voyager-1 to constrain the cosmic ray source and transport parameters. The study shows that the Z > 2 data yield a high-energy diffusion slope δ2 ∼ (0.37, 0.44). The Z ≤ 2 species obtain a looser constraint on δ2 ∼ (0.34, 0.44). The overlap infers the heavy and light particles can give compatible results at high energies. Meanwhile, at low energies, significant disagreements exist between the heavy and light elements. The B/C ratio requires a much larger diffusion slope variation δ2-δ1 around 4 GV or a stronger Alfvén velocity vA than the low-mass data. This indicates that the heavy and light particles may suffer different low-energy transport behaviors in Galaxy. However, better understanding on the consistency/inconsistency between the heavy and light relies on more precise cross-sections, better constraints on correlations in systematic errors of data, and more accurate description for Solar modulation during the reversal period of HMF.

show abstract

Section: B Fit To the Light Elementsmentioning

confidence: 92%

Section: B Fit To the Light Elementsmentioning

confidence: 92%

“…The corresponding models are suffixed with "-LR". Then we include the 2 H/ 4 He and 3 He/ 4 He data in the analyses. The corresponding models are suffixed with "-L".…”

Section: B Fit To the Light Elementsmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

See 3 more Smart Citations

Testing the consistency of proapgation between light and heavy cosmic ray nuclei

Wang,

Wu,

Long

2021

Preprint

View full text Add to dashboard Cite

show abstract

Moving Contact Line Instability on Soluble Fibers

Yang

Yuan

2022

Adv Materials Inter

Self Cite

View full text Add to dashboard Cite

This paper presents a new kind of instability when inserting a soluble fiber into liquid. After wetting and dissolving the fiber by the liquid, the moving contact line (MCL) spontaneously loses stability. Because the sculpted shape of the fiber looks like a Chinese pagoda, this instability is named as the pagoda instability (PI). The coupling of dissolution and wetting leads to other special phenomena, i.e., dissolving‐induced jet flow, and optimizes the fiber shape, etc. A criterion of PI is proposed and the competition between the interfacial energy and chemical potential to deduce the MCL motion and PI is shown. A phase diagram is used to summarize the final shapes of the fibers. By conducting atomic force microscopy (AFM) measurements, it is found that fibers with optimized shapes have a low adhesion force. Using the optimized fiber can decrease the influence of the capillary force during AFM measurements in humid environments by 70%.

show abstract

Steady state response of an infinite beam on a viscoelastic foundation with moving distributed mass and load

Zhang

2020

Sci. China Phys. Mech. Astron.

View full text Add to dashboard Cite

Solute transport and interface evolution in dissolutive wetting

Cited by 15 publications

References 27 publications

Testing the consistency of proapgation between light and heavy cosmic ray nuclei

Testing the consistency of proapgation between light and heavy cosmic ray nuclei

Moving Contact Line Instability on Soluble Fibers

Steady state response of an infinite beam on a viscoelastic foundation with moving distributed mass and load

Contact Info

Product

Resources

About