scholarly journals THE MAGNETIC PROPERTIES MEASUREMENT OF COIL FOR GRAVITATIONAL ACCELERATION DETERMINATION

2020 ◽  
Vol 5 (2) ◽  
pp. 119-128
Author(s):  
Cherly Salawane ◽  
Supriyadi Supriyadi ◽  
Ronaldo Talapessy ◽  
Mirtha Yunitha Sari Risakotta

The value of the gravitational acceleration of the earth above the earth’s surface depends on the position of the latitude and longitude of the earth’s surface, in other words, because the shape of the earth’s surface is not round like a ball. The magnitude of gravity is not the same everywhere on the surface of the earth. The purpose of this study is to analyze the value of the earth’s gravitational acceleration in a laboratory using a current balance with a graphical method. Fluctuations in the value of the magnetic field strength (B) and the value of the electric current strength (i) on the current balance cause the value of laboratory gravitational acceleration (glab) to vary in the transfer of electric charge (q) according to coil type. The magnitude of the earth’s gravitational acceleration value obtained in a laboratory with a current balance for each type of coil is as follows: SF-37 glab-nr=9.89 m/s2, SF-38 glab-nr=9.90 m/s2, SF-39 glab-nr=9.76 m/s2, SF-40 glab-nr=9.95 m/s2, SF-41 glab-nr=9.75 m/s2 dan SF-42 glab-nr=9.93 m/s2. The results obtained indicate that the value of the earth’s gravitational acceleration in a laboratory close to the literature value is the value of the glab-nr in the SF-37 coil type of 9.89 m/s2.

2020 ◽  
Vol 12 (2) ◽  
pp. 12
Author(s):  
Jiri Stavek

In our approach we have combined knowledge of Old Masters (working in this field before the year 1905), New Masters (working in this field after the year 1905) and Dissidents under the guidance of Louis de Broglie and David Bohm. Based on the great works of Julian Schwinger and John Archibald Wheeler we will study properties of geons formed by fusion of two soft x-ray particles (dyons) in the Schwarzschild gravitation core in our Sun at temperature 16 * 106 K. There are now several Teams that are able to achieve this fusion temperature in their special instruments (Tokamak, HL-2M Tokamak, Wendelstein 7-X, NIF, etc.) and to study properties of those formed geons. Thermal geons are with us all the time but they are very deeply hidden in our experiments. We have newly introduced Mareš - Šesták constant as the ratio of geon momentum to heat quantum of geon. The key information to enter into the World of geons was the empirical formula of David Bohm - the very well-known Bohm diffusion. From this formula we have extracted the amplitude, wavelength, frequency, quantum of the geon action, displacement law for geons, etc. It was found that geons are highly sensitive to the magnetic field strength. At a low magnetic field strength, the “inflation of geons” can occur. This effect could explain the Superheating of the Solar corona and the observed Heating of the Earth during two last centuries influenced by the changes in the Earth´s magnetic field. Geon engineering might modify the geon volume through the magnetic field strength. On the other hand, we were stimulated by the works of Mordehai Milgrom and Eric Verlinde and derived the Milgrom-Verlinde constant describing the gravitational field strength leading to the Newtonian gravitational constant on thermodynamic principles. The quantum of the geon momentum might open a new way how to understand gravitational phenomena. Can it be that Nature cleverly inserted geons into our experimental apparatuses and into our very-well known Old Formulae? We want to pass this concept into the hands of Readers of this Journal better educated in the Mathematics, Physics, and Thermodynamics.


2022 ◽  
Author(s):  
A.V. Mikhailov

Abstract. In this work, using a series of numerical experiments, the dependence of the magnetic field strength of the response of the reinforcing bar to an external magnetizing field on the magnetic properties of the reinforcing bar was investigated. The possibility of determining with high accuracy the diameter of reinforcing bars, regardless of the magnetic properties of the material from which they are made, has been proven.


2006 ◽  
Vol 984 ◽  
Author(s):  
Hans Malissa ◽  
Wolfgang Jantsch ◽  
Friedrich Schäffler ◽  
Zbyslaw Wilamowski

AbstractWe report the observation of a particularly simple effect of spin-orbit coupling which allows for efficient manipulation of spins by an electric current in semiconductor nanostructures. Passing an electric current density of j = 2.5 mA/cm through a modulation doped Si quantum well (density of 5 × 1011 cm-2) perpendicular to an in-plane magnetic field, we observe a shift of the spin resonance of the conduction electrons (CESR) by about 0.1 mT. This shift reverses sign when we invert (i) the current direction, (ii) the magnetic field direction and it vanishes for perpendicular magnetic field. We show that this current-induced shift in g-factor, i.e., its dependence on current and carrier density, its temperature dependence and its anisotropy can be consistently and quantitatively explained in terms of the Bychkov-Rashba coefficient determined earlier from the CESR broadening and the g-factor anisotropy [1]. Other sources of magnetic field (e.g. the Oersted effect) are negligible. This effect can be utilized for g-factor tuning, and thus for local spin manipulation: passing a current through some part of a sample may be utilized to bring those electrons into resonance with a microwave field. These spins are thus excited to Rabi oscillations and, using current pulses of suitable duration, π rotations (or by any other angle) can be achieved.


1984 ◽  
Vol 24 (03) ◽  
pp. 269-274 ◽  
Author(s):  
Arthur F. Kuckes ◽  
T. Lautzenhiser ◽  
A.G. Nekut ◽  
R. Sigal

Abstract This paper describes an electromagnetic method to facilitate drilling a well to intersect a target well casing. It has an important application in control of blown out oil and gas wells. By this method, a relief well was directionally drilled to intersect the casing of a blowout at 8,000 ft [2700 m]. The relative distance and azimuthal direction to the target casing can be determined when the relief well is up to more than 100 ft [30 m] from the blowout. Introduction There is a need, particularly in the control of runaway oil or gas wells, for the ability to drill a relief well to intersect a target well casing at a specified subsurface depth. Our method consists of detecting and analyzing the magnetic field generated by alternating electric current flow on a target well casing, drillstem, or fish. By comparison to the earth, steel is a very good electrical conductor; a steel well casing has a strong "short-circuiting" effect on the parallel component of electric current now in its vicinity, The magnetic field generated by current flow on the target casing and measured in the relief well can be used to determine the relative distance and direction from the relief well to the target. In this paper, we present the principles of operation along with the results of some field tests. An alternative scheme using a wireline current source is described in the Appendix. Principle of the Method Principle of the Method Consider the apparatus shown in Fig. 1. The dimensions shown can vary greatly: those given are for reference. A low-frequency AC is injected into the ground by use of surface electrodes near the blowout. The return current is collected by remote surface electrodes. If the blowout casing were not present, this arrangement would produce a very small magnetic field response on or near the blowout axis. With the blowout casing in place, there is a large enhancement of the current flowing down the blowout axis, which results in a large enhancement of the magnetic field as indicated by Ampere's law. Considering the geometry of the magnetic field resulting from a current-carrying conductor, the apparent direction to the conductor can be deduced. It is useful to introduce a parameter re that is the radius of a circular column of earth having the same resistance per unit length as the blown out well casing. If the conductivity of the earth is given by sigma e, that of the casing by sigma c, and the well casing has a radius rc and wall thickness hc, then re is given by (1) The electrical conductivity of steel is about 107 (omega.m)-1, whereas that of country rock in a petroleum environment is within an order of magnitude of 0.1 (omega.m)-1. Thus, a well casing with a 1/2-in. [1.3-cm] wall, 10 in. [25 cm] in diameter, has the same electrical resistance per unit length as a column of earth [sigma c = 1(omegam)-1] about 1,000 ft [300 m] in diameter. Such well casing has a short-circuiting effect to vertical current flow on a column of earth approximately this diameter. The sensitivity of standard magnetometers is such that after 100 seconds of signal averaging, an AC magnetic induction of less than 10–2 gammas or alternatively a magnetic field of 10–5 A/m can be detected. This corresponds to the magnetic field generated by a current of 2 mA on well casing 100 ft [30 m] away. The parameter re also indicates the scale length over which current builds up on a casing. Thus, for a semi-infinite casing surrounded by a uniform conductor of much lower conductivity, the current on the casing will build up to its asymptotic value within re of the end of the casing. Consequently, it is a valid approximation to calculate the current on the casing, Ic, by (2) when the electric field, E, parallel to the casing varies slowly on the scale re. This is the situation far from the surface injection electrodes. When a distance on the order of re from the blowout casing, the low-frequency magnetic field signal is caused predominantly by current flow on the blowout: predominantly by current flow on the blowout: (3) SPEJ P. 269


Author(s):  
P. E. Tereshchenko

An analytical expression for the vertical component of the magnetic field has been obtained, with the help of which calculations have been made showing the effect of the ionosphere on the low-frequency field in the Earth-ionosphere waveguide. At distances from the source that are less than the doubled waveguide height, in ELF, and a lower frequency range, noticeable changes in the field strength caused by the state of the ionosphere are found.


Author(s):  
A.V. Moshkov ◽  

Projects of active experiments in the ionosphere and the magnetosphere of the Earth and planets often include powerful low-frequency transmitters installed on-board of a spacecraft. Such sources are very effective, but their radiation is extremely heterogeneous in space because of the anisotropy of the ionospheric plasma due to the presence of the magnetic field of the Earth. This paper is devoted to numerical modeling of a distribution of the wave field strength near the Earth surface. The work examines a specific active wave experiment with a 20 m loop as a transmitting antenna. The satellite is assumed to orbit with an inclination of 82.5 degrees at an average altitude of 1000 km. All calculations are performed in linear approximation using the cold magneto-active plasma model. The computation model uses ray approximation everywhere except for the highly heterogeneous lower ionosphere, where a full wave equations set is applied. It is shown that the maximum magnetic field value is decreased with increasing of the geomagnetic latitude value and the strength range is 1… 2 nA/m for frequency 10 kHz and loop current 100 A. The magnitude of the vertical component of the electric field lies in the range of 0.4 ... 0.8 μV/m. An average Doppler frequency shift is equal to ~0.4 Hz. A comparison is made between the data of the numerical experiment and the results of simple estimations of the values of the magnetic field strength at the maximum of the ground distribution.


2001 ◽  
Vol 19 (10/12) ◽  
pp. 1711-1720 ◽  
Author(s):  
J. G. Trotignon ◽  
P. M. E. Décréau ◽  
J. L. Rauch ◽  
O. Randriamboarison ◽  
V. Krasnoselskikh ◽  
...  

Abstract. The Wave Experiment Consortium, WEC, is a highly integrated package of five instruments used to study the plasma environment around the Earth. One of these instruments, the Waves of HIgh frequency and Sounder for Probing of Electron density by Relaxation, Whisper, aims at the thermal electron density evaluation and natural wave monitoring in the 4–83 kHz frequency range. In its active working mode, which is our primarily concern here, the Whisper instrument transmits a short wave train at a swept frequency and receives echoes after a delay. Incidentally, it behaves like a classical ground-based ionosonde. Natural modes of oscillations may thus be excited in the surrounding medium. This means that with suitable interpretations, the Whisper sounding technique becomes a powerful tool for plasma diagnosis. By taking into account the characteristic frequencies of the magnetoplasmas encountered by the Cluster spacecraft, it is indeed possible to reliably and accurately determine the electron density and, to a lesser degree, the magnetic field strength from the Whisper electric field measurements. Due to the predominantly electrostatic nature of the waves that are excited, observations of resonances may also lead to information on the electron velocity distribution functions. The existence of a hot population may indeed be revealed and the hot to cold density ratio can be estimated.Key words. Magnetospheric physics (plasma waves and instabilities). Space plasma physics (active perturbation experiments; instruments and techniques)


1976 ◽  
Vol 32 ◽  
pp. 613-622
Author(s):  
I.A. Aslanov ◽  
Yu.S. Rustamov

SummaryMeasurements of the radial velocities and magnetic field strength of β CrB were carried out. It is shown that there is a variability with the rotation period different for various elements. The curve of the magnetic field variation measured from lines of 5 different elements: FeI, CrI, CrII, TiII, ScII and CaI has a complex shape specific for each element. This may be due to the presence of magnetic spots on the stellar surface. A comparison with the radial velocity curves suggests the presence of a least 4 spots of Ti and Cr coinciding with magnetic spots. A change of the magnetic field with optical depth is shown. The curve of the Heffvariation with the rotation period is given. A possibility of secular variations of the magnetic field is shown.


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