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Correlations between the Rotations and Magnetospheres of the Terrestrial Planets and the Sun’s Formation in Our Solar System

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World j.urnal of Condensed Matter Physics 2022年第2期12卷 18-26页

作者： fred j. cadieu Physics Department Queens College of CUNY New York USA

Correlations between the rotations of the terrestrial planets in our solar system and the magnetic field of the Sun have been previously noted. These correlations account for the opposite rotation of Venus as a result of the magnetic field of the Sun being dragged across the conducting core of Venus. Currently, the Sun’s magnetic field is not sufficiently strong to account for the proposed correlations. But recently meteorite paleomagnetism measurements have indicated that during the Sun’s formation the magnetic field of the Sun was of sufficient strength to have resulted in the observed correlations. Also, dating back to the Sun’s formation are measurements showing that the Sun’s core rotates four times faster than the Sun’s surface. Both the counter rotation of Venus and the initial period of strong Sun magnetic fields are believed to be relics of the time period when the Sun’s core to surface differential rotation was established. As a part of these correlations, it was hypothesized that for a terrestrial planet to exhibit a magnetosphere, the average density must be ≥5350 ± 50 kg/m3. On this basis, only the Earth and Mercury would have formed initial magnetospheres, while Venus, Mars, and the “Moon” would not have developed magnetospheres. For such correlations to still be present today requires our Sun to have been formed as a sole star and with what might be termed a friendly j.piter. Otherwise, the observed correlations would have been disrupted over time.

关键词： Earth Mercury Venus Mars Magnetic Fields Sun Early Solar System Plate Tectonics

A Consistent Model of Terrestrial Planet Magnetospheres and Rotations in Our Solar System

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World j.urnal of Condensed Matter Physics 2021年第2期11卷 13-27页

作者： fred j. cadieu Physics Department Queens College of CUNY Flushing NY USA

The Sun comprises 99.9% of the solar system mass so it is expected that Sun terrestrial planet interactions can influence the motion as well as the rotation of the terrestrial planets. Gravity affects the planet orbital motions while the changing magnetic fields of the Sun can influence the planet rotations. Planets that manifest a magnetic field dominate any weaker magnetic fields from the Sun, but the rotation of terrestrial planets without a magnetic field interacts with the changing Sun’s field dependent on the electrical conductivity of the core region. It is determined that the average planet density becomes a useful quantity to describe the magnetic state of a terrestrial planet. An average density of 5350 ± 50 kg/m3 is hypothesized to separate planets that develop magnetospheres from those that do not. Planets with higher average densities, Mercury and Earth, developed magnetospheres. While those with lower average densities, Venus and Mars never developed magnetospheres. Terrestrial planets with magnetospheres are the ones to also exhibit plate tectonics. The small size of Mercury led to Mercury only exhibiting a frozen in magnetization of potentially magnetic regions. The lack of magnetospheres as well as lack of plate tectonics prevented the continual transfer of core heat to the surface that limited the surface vulcanism to an initial phase. For Venus, it meant that the surface regions would only sporadically convulse. In this picture, the apparent anomalous axial rotation of Venus is a natural consequence of the rotation of the Sun. For Mars with relatively low surface temperatures, it meant that there was little heat exchange through the crust that would allow the lower crust to retain large amounts of water. For Mars to have initially had flowing liquid water required that the atmosphere at that time contained high concentrations of infrared absorbing gases at least as compared to the present level of infrared absorbing gases on the Earth.

关键词： Earth Mercury Venus Mars Magnetic Fields Sun Early Solar System Plate Tectonics

j.st a Bit of Physics Can Tell So Much: A Unique Story of the Start of the Earth-Moon System

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World j.urnal of Condensed Matter Physics 2020年第2期10卷 88-103页

作者： fred j. cadieu Department of Physics Queens College of CUNY New York NY USA

The start of the Earth-Moon system has been studied to show that this was an exceptionally violent event. One result was that Earth became the terrestrial planet with the highest average density. Another result was that Earth acquired enough mass and radioactive elements that it is expected to maintain a molten core region and magnetic field for the expected life of the Earth. Earth alone of the terrestrial planets was then able to develop plate tectonics as a long term energy release mechanism. The dipole magnetic field of the Sun reverses periodically, currently at the rate of about every 11 years, so that there was a magnetic braking action acting on the core of Venus that accounts for the slow rotation of that planet. A key result is that the impact event that resulted in the Earth-Moon system led to long term stability on Earth that allowed the eventual development of complex life forms on the Earth.

关键词： Earth Moon Magnetic Fields Sun Venus Plate Tectonics

Nanometer Thick Diffused Hafnium and Titanium Oxide Light Sensing Film Structures

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World j.urnal of Condensed Matter Physics 2017年第1期7卷 36-45页

作者： fred j. cadieu Lev Murokh Department of Physics Queens College of CUNY Flushing NY USA Graduate Center of CUNY New York NY USA

We examine 10 nm thick film structures containing either Hf or Ti sandwiched between two respective oxide layers. The layers are deposited onto heated substrates to create a diffusion region. We observe a high degree of light sensitivity of the electric current through the film thickness for one polarity of an applied voltage. For the other polarity, the current is not affected by the light. We explain the observed phenomenology using the single-particle model based on the existence of interface states on the metal-oxide interfaces.

关键词： Thin Film Light Sensing Current Enhancement Interface States Hafnium Titanium

Physical Simulation of Thermally Induced Martensite Formation from Retained Austenite in TRIP Steels

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j.urnal of Materials Science & Technology 2003年第Z1期19卷 105-108页

作者： Lie ZHAO fred j. VERMOLEN j.lt SIETSMA Sybrand van der ZWAAG Netherlands Institute for Metals Research P.O.Box 5008 2600 GA Delft The Netherlands Department of Materials Science Delft University of Technology R otterdamseweg 137 2628 AL Delft The Netherlands Department of Applied Mathematics Delft University of Technology Mekelweg 4 2628 CD Delft The Netherlands Department of Materials ScienceDelft University of TechnologyRotterdamseweg 1372628 AL DelftThe Netherlands Netherlands Institute for Metals Research P.O.Box 5008 2600 GA Delft The Netherlands Faculty of Aerospace Engineering Delft University of Technology Kluyverweg 1 2629 HS Delft The Netherlands

The present work analyses the total free energy of the material during the martensitic transformation. A general expression for the martensite fraction as a function of temperature is derived, assuming that the nonchemical free energyis proportional to the volume of martensite. This expression indicates that the temperature-dependent martensitefraction can be predicted once the characteristic transformation temperatures and the relation between the chemicalfree energy and temperature of the martensite and austenite are known. An advantage of this development is thatthe proposed equation is valid for all types of relations between the chemical free energy and temperature. Thissimulation is successfully applied to the martensitic transformation upon further cooling of retained austenite in alow-alloyed TRIP steel, in which the relation between chemical free energy and temperature is quadratic and thefraction is determined from a thermo-magnetic measurement.

关键词： Thermodynamics, Martensitic transformation, Retained austenite, TRIP steels.

Universal optimality of digital nets and lattice designs

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Science China Mathematics 2009年第11期52卷 2309-2320页

作者： HICKERNELL fred j Department of Applied Mathematics Illinois Institute of Technology

This article considers universal optimality of digital nets and lattice designs in a regression model. Based on the equivalence theorem for matrix means and maj.rization theory,the necessary and sufficient conditions for lattice designs being φp-and universally optimal in trigonometric function and Chebyshev polynomial regression models are obtained. It is shown that digital nets are universally optimal for both complete and incomplete Walsh function regression models under some specified conditions,and are also universally optimal for complete Haar wavelet regression models but may not for incomplete Haar wavelet regression models.

关键词： Chebyshev polynomial Haar wavelet Trigonometric function Walsh function 62K15 62K10

Universally consistent estimation for stochastic regression models

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Chinese Science Bulletin 1995年第10期40卷 802-807页

作者：安鸿志 Hickernell fred j. 朱力行 Probability Lab Institute of Applied Mathematics Chinese Academy of Sciences Beijing 100080 China Department of Matbematice Hong Kong Baptist University Hong Kong.

Addressed problem Consider multivarate lincar regression model in which x is pdimensional random

关键词： multivariate regression model characteristic function consistency of estimation.

Direct Load Control of Thermostatically Controlled Loads Based on Sparse Observations Using Deep Reinforcement Learning

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CSEE j.urnal of Power and Energy Systems 2019年第4期5卷 423-432页

作者： frederik Ruelens Bert j.Claessens Peter Vrancx fred Spiessens Geert Deconinck Department of Electrical Engineering KU Leuven/EnergyVille3001 LeuvenBelgium REstore Centrica2600 AntwerpBelgium AI-lab Vrije Universiteit Brussel1050 BrusselsBelgium Vito/EnergyVille 2600 MolBelgium

This paper considers a demand response agent that must find a near-optimal sequence of decisions based on sparse observations of its *** a relevant set of features from these observations is a challenging task and may require substantial domain *** way to tackle this problem is to store sequences of past observations and actions in the state vector,making it high dimensional,and apply techniques from deep *** paper investigates the capabilities of different deep learning techniques,such as convolutional neural networks and recurrent neural networks,to extract relevant features for finding near-optimal policies for a residential heating system and electric water heater that are hindered by sparse *** simulation results indicate that in this specific scenario,feeding sequences of time-series to an Long Short-Term Memory(LSTM)network,which is a specific type of recurrent neural network,achieved a higher performance than stacking these time-series in the input of a convolutional neural network or deep neural network.

关键词： Convolutional networks deep reinforcement learning long short-term memory residential demand response

Dynamics and functions of E‑cadherin complexes in epithelial cell and tissue morphogenesis

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Marine Life Science & Technology 2023年第4期5卷 585-601页

作者： Na Zhang Matthias Häring fred Wolf j.rg Großhans Deqing Kong Department of Biology Philipps University35043 MarburgGermany Göttingen Campus Institute for Dynamics of Biological Networks(CIDBN) Georg August University Göttingen37073 GöttingenGermany

Cell–cell adhesion is at the center of structure and dynamics of epithelial tissue.E-cadherin–catenin complexes mediate Ca^(2+)-dependent trans-homodimerization and constitute the kernel of adherens *** the basic function of cell–cell adhesion,recent progress sheds light the dynamics and interwind interactions of individual E-cadherin–catenin complex with E-cadherin superclusters,contractile actomyosin and mechanics of the cortex and *** nanoscale architecture of E-cadherin complexes together with cis-interactions and interactions with cortical actomyosin adj.st to j.nctional tension and mechano-transduction by reinforcement or weakening of specific features of the *** post-translational modifications such as phosphorylation and glycosylation have been implicated,their role for specific aspects of in E-cadherin function has remained ***,we provide an overview of the E-cadherin complex in epithelial cell and tissue morphogenesis focusing on nanoscale architectures by super-resolution approaches and post-translational modifications from recent,in particular in vivo,***,we review the computational modelling in E-cadherin complexes and highlight how computational modelling has contributed to a deeper understanding of the E-cadherin complexes.

关键词： Nanoscale architectures Phosphorylation Glycosylation Computational modelling