Steps to the scientific notation
Illustrate the steps to the scientific notation? Briefly illustrate the steps.
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To write down in scientific notation, you must first move the decimal point of the number to where the number is among 1 and 9. For illustration, change 567 to 5.67. Then count the number of position you moved the decimal. When you moved it left then the number is positive. When you moved it right then the number is negative. Lastly the number with the decimal point by 10 to the power of number, the decimal moved.
A thermocouple of K type is suddenly exposed to air with temperature of 1273K, Initial temperature was 293 K. Calculate the time needed for the thermocouple read the temperature with accuracy of better that 99%. Ignore radiation and conduction. The measuring element has a ball shape of diameter o
Planck constant: h: The basic constant equivalent to the ratio of the energy of a quantum of energy to its frequency. This is the quantum of action. This has the value 6.626 196 x 10-34 J s.
sir, Would you please help me to develop an algorithm to reduce noise and to detect weak signals under water using Green's function?
what is the characteristics of electronics ?
Hawking temperature: The temperature of a black hole is caused by the emission of the hawking radiation. For a black hole with mass m, it is illustrated as: T = (hbar c3)/(8 pi G k m).
Systeme Internationale d'Unites (SI): The rationalized and coherent system of units derived from the m.k.s. system (that itself is derived from metric system) in common utilization in physics nowadays.
What do you mean by the term curvilinear motion? State in brief?
Eotvos law of capillarity (Baron L. von Eotvos; c. 1870): The surface tension gamma of a liquid is associated to its temperature T, the liquid's critical temperature, T*, and its density rho by: gamma ~=
: A voltage v = 150 + j180 is applied across an impedance and the current flowing is I = 5 - j4 find ? A, impedance . B, resistance. C, reactance. D, power consumed.
Cosmic background radiation: primal glow: The background of radiation is generally in the frequency range of 3 x 1011 to 3 x 108 Hz discovered in space in the year 1965. It is believed to be the cosmologically re
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