Showing posts with label Circuit Analysis. Show all posts
Showing posts with label Circuit Analysis. Show all posts

RADIO FREQUENCY CIRCUITS BASIC AND TUTORIALS



Radio-frequency circuits are represented here by only a few general examples, because the circuits and design methods that have to be used are fairly specialized, particularly for transmission; the reader who wishes more information on purely RF circuits is referred to the excellent amateur radio publications.

At one time, a reference book would have shown discrete circuits for RF and IF receiver stages, but for conventional analogue radio reception these functions are now invariably carried out by ICs.

The Philips TEA5711 is an IC, now quite old (1992) and established, that integrates all the functions of an AM/FM radio from front end to AM detector and FM stereo output in a 32-pin DIL package.

Figure 7.37 shows a suggested application from the datasheet, using a separate TDA5070 output chip. The TEA5711 chip allows a wide range of supply voltage, from 1.8 V to 12 V, and has a low current consumption of 15 mA on AM and 16 mA on FM.

fig 7.37

The input sensitivity for FM is 2.0 μV, with high selectivity, and the FM input uses a high impedance MOSFET. The main applications are in portable radios.


The Chorus FS1010 from Frontier Silicon is a 179-pin BGA package that implements the most difficult sections of a DAB digital radio receiver, needing only an external RF stage, audio D to A, flash memory, keypad and display for a complete radio.

The chip incorporates 16 K of ROM, 384 K of RAM, and two 8 K cache memories. It is likely that some day we shall have all of these functions on one chip, but until DAB radios sell in more significant numbers and until gaps in transmitting areas are filled in this is not likely to happen rapidly.  One significant difference from radio as we used to know it is that there is no chance of using discrete components.


Much more specialized devices are used for microwave frequencies, and a specialist in semiconductors for these ranges is Tquint Semiconductors. As example, the Tquint TGC1430G multiplier is intended as a ×3 multiplier with an output in the range of 20–40 GHz using stripline architecture with GaAs semiconductors.


MOORE AND MEALY CIRCUIT BASIC AND TUTORIALS



Autonomous circuits are those with no external inputs (except for the clock line) and which therefore perform independently (autonomously) of other circuits\ around them. Such circuits move through a set cycle of states as the circuit is\ clocked.

The synchronous counters in the last chapter come into this category. However, the states of a general autonomous circuit obviously need not follow a binary sequence and furthermore the external ouputs need not simply be the outputs from the flip-flops (as with the synchronous counters) but could be functions of these (present state) signals.

General (Moore and Mealy) circuits
The next state of a general synchronous sequential circuit is dependent not only on the present state, as in an autonomous circuit, but also on the external inputs. Such general circuits can be further subdivided into two classes which are commonly referred to as Moore and Mealy models.

Moore model
The Moore model describes a general synchronous sequential circuit where the external outputs are only functions of the circuit's present states (i.e. the flip-flops' outputs). Because of this in the state diagram of such a circuit the external outputs can be linked explicitly to the nodes (i.e. states).

Mealy model
The Mealy model is the most general since not only is the next state dependent upon the present state and the external inputs, but the external outputs are also functions of both of these sets of variables.

Since the external outputs also depend upon the external inputs then in the state diagram of Mealy circuits the external outputs cannot simply be associated with a node but rather must be linked to the arrows (connecting the nodes) which are labelled with the output conditions as appropriate.

SEMICONDUCTORS DEFINITION BASICS AND TUTORIALS


WHAT IS A SEMICONDUCTOR? INFORMATION ABOUT SEMICONDUCTORS

Semiconductors are a categoryofmaterialswith an electrical conductivity that is between that of conductors and insulators. Good conductors, which are all metals, have electrical resistivities down in the range of 10^−6 OHM -cm.

Insulators have electrical resistivities that are up in the range from 10^6 to as much as about 10^12 OHM - cm. Semiconductors have resistivities that are generally in the range of 10^−4–10^4 OHM -cm.

The resistivity of a semiconductor is strongly influenced by impurities, called dopants, that are purposely added to the material to change the electronic characteristics.

We will first consider the case of the pure, or intrinsic semiconductor. As a result of the thermal energy present in the material, electrons can break loose from covalent bonds and become free electrons able to move through the solid and contribute to the electrical conductivity.

The covalent bonds left behind have an electron vacancy called a hole. Electrons from neighboring covalent bonds can easily move into an adjacent bond with an electron vacancy, or hole, and thus the hold can move from one covalent bond to an adjacent bond.

As this process continues, we can say that the hole is moving through the material. These holes act as if they have a positive charge equal in magnitude to the electron charge, and they can also contribute to the electrical conductivity.

Thus, in a semiconductor there are two types of mobile electrical charge carriers that can contribute to the electrical conductivity, the free electrons and the holes. Since the electrons and holes are generated in equal numbers, and recombine in equal numbers, the free electron and hole populations are equal.

In the extrinsic or doped semiconductor, impurities are purposely added to modify the electronic characteristics. In the case of silicon, every silicon atom shares its four valence electrons with each of its four nearest neighbors in covalent bonds.

If an impurity or dopant atom with a valency of five, such as phosphorus, is substituted for silicon, four of the five valence electrons of the dopant atom will be held in covalent bonds. The extra, or fifth electron will not be in a covalent bond, and is loosely held.

At room temperature, almost all of these extra electronswill have broken loose fromtheir parent atoms, and become free electrons. These pentavalent dopants thus donate free electrons to the semiconductor and are called donors.

These donated electrons upset the balance between the electron and hole populations, so there are now more electrons than holes. This is now called an N-type semiconductor, in which the electrons are the majority carriers, and holes are the minority carriers.

In an N-type semiconductor the free electron concentration is generally many orders of magnitude larger than the hole concentration. If an impurity or dopant atom with a valency of three, such as boron, is substituted for silicon, three of the four valence electrons of the dopant atom will be held in covalent bonds.

One of the covalent bonds will be missing an electron. An electron from a neighboring silicon-to-silicon covalent bond, however, can easily jump into this electron vacancy, thereby creating a vacancy, or hole, in the silicon-to-silicon covalent bond. Thus, these trivalent dopants accept free electrons, thereby generating holes, and are called acceptors.

These additional holes upset the balance between the electron and hole populations, and so there are now more holes than electrons. This is called a P-type semiconductor, in which the holes are the majority carriers, and the electrons are the minority carriers. In a P-type semiconductor the hole concentration is generally many orders of magnitude larger than the electron concentration.

The transition between the two sides is called the PN junction. As a result of the concentration difference of the free electrons and holes there will be an initial flow of these charge carriers across the junction, which will result in the N-type side attaining a net positive charge with respect to the P-type side.

This results in the formation of an electric potential hill or barrier at the junction. Under equilibrium conditions the height of this potential hill, called the contact potential is such that the flow of the majority carrier holes from the P-type side up the hill to the N-type side is reduced to the extent that it becomes equal to the flow of the minority carrier holes from the N-type side down the hill to the P-type side.

Similarly, the flow of the majority carrier free electrons fromthe N-type side is reduced to the extent that it becomes equal to the flow of the minority carrier electrons from the P-type side. Thus, the net current flow across the junction under equilibrium conditions is zero.

COMMON COLLECTOR TRANSISTOR CONFIGURATION BASICS AND TUTORIALS


WHAT IS COMMON COLLECTOR TRANSISTOR CONFIGURATION

Figure 1 is a practical example of a common-collector transistor amplifier. Note that the output is taken off of the emitter instead of the collector (as in the common-emitter configuration).

A common-collector amplifier is not capable of voltage gain. In fact, there is a very slight loss of voltage amplitude between input and output.








However, for all practical purposes, we can consider the voltage gain at unity. Common-collector amplifiers are noninverting, meaning the output signal is in phase with the input signal.

Essentially, the output signal is an exact duplicate of the input signal. For this reason, common-collector amplifiers are often called emitter-follower amplifiers, because the emitter voltage follows the base voltage.

Common-collector amplifiers are current amplifiers. The current gain for the circuit illustrated in Fig. 1 is the parallel resistance value of R1 and R2, divided by the resistance value of R3. R1 and R2 are both 20 Kohms in value, so their parallel resistance value is 10 Kohms.

This 10 Kohms divided by 1 Kohm (the value of R3) gives us a current gain of 10 for this circuit. Because the voltage gain is considered to be unity (1), the power gain for a common-collector amplifier is considered equal to the current gain (10, in this particular case).

The input impedance of common-collector amplifiers is typically higher than the other transistor configurations. It is the parallel resistive effect of R1, R2, and the product of the value of R3 times the beta value.

Because beta times the R3 value is usually much higher than that of R1 or R2, you can closely estimate the input impedance by simply considering it to be the parallel resistance of R1 and R2. In this case, the input impedance would be about 10 Kohms.

The traditional method of calculating the output impedance of common-collector amplifiers is to divide the value of R3 by the transistor’s beta value. Although this method is still appropriate, a closer estimate can probably be obtained by considering the output impedance of most transistors to be about 80 ohms.

This 80-ohm output impedance should be viewed as being in parallel with R3, giving us a calculated output impedance of about 74 ohms (80 ohms in parallel with 1000 ohms). Resistors R1 and R2 have the same function within a common-collector amplifier as previously discussed with common-emitter amplifiers.

The high negative feedback produced by R3 provides excellent temperature stability and immunity from transistor variables. The circuit illustrated in Fig. 1 can be a valuable building block toward future projects.