You will need

- - stopwatch or a watch$
- calculator.

Instruction

1

Lightning is a threat to human life, natural phenomenon. However, ironically, it is the fault of the people they are becoming more. This happens due to the extremely irresponsible attitude to the environment: pollution of air in cities increases the heating of the air environment and the rise of the steam condensate. This reinforces the electric intensity in the clouds provokes lightning discharges.

2

The need to determine the

**distance**to**lightning**was caused not only by the need to expand the horizon and the elementary instinct of self-preservation. If it is too close and you are in open space, it is better as quickly as possible to escape from there. The electric current chooses the shortest path to the ground, and the skin is a great conductor for it.3

Start counting seconds as soon as you see the sky light flash, use a clock or stopwatch. As soon as you hear the first clap of thunder, stop the account, so you get the time.

4

To find

**distance**, you need time multiply by speed. If accuracy for you is not very important, then it can be taken equal to 0.33 km/s, i.e., multiply number of seconds by 1/3. For example, you estimate the time until the**zipper**was 12 seconds, after dividing by 3, you get 4 km.5

To determine the

**distance**to**lightning**more precisely, take the average speed of sound in air is equal to 0,344 km/s. Its true value depends on many factors: humidity, temperature, type of terrain (open space, forest, urban high-rise buildings, water surface), wind speed, etc. for Example, when rainy autumn weather, the speed of sound is approximately equal to 0,338 km/s, in summer the dry heat is about 0.35 km/s.6

Dense forest and tall buildings significantly slow down the speed of sound. It is reduced because of the need to go around many obstacles, diffraction. An accurate calculation in this case is quite difficult, impractical and most importantly: despite the fact that lightning does not hit the earth, it may strike a tall tree near you. So wait it among low-growing trees with dense foliage, best squat, and if you were on a city street, then take cover in a nearby building.

7

Pay attention to the wind. If he is strong enough and blowing in your face from

**the zipper**, then the sound goes faster. Then its average speed can be taken approximately equal to 0.36 km/h When wind direction from you to**the lightning**the sound movement, on the contrary, slows down and speed is approximately equal to 0,325 km/h.8

The average length of

**zipper**up to 2.5 km and extends to a discharge**distance**up to 20 km, and Therefore should be removed from the open space of the nearest building or structure. Remember that when approaching**lightning**need to close all doors and Windows and unplug electrical appliances, since it can be defeat through the antenna and network to harm your technique.9

The lightning are not only land, but also vnutrioblastnaya. They are not dangerous for those who are on the ground, however, can damage flying objects: planes, helicopters and other vehicles. In addition, a metal object caught in the cloud with a strong electric field capable of supporting, but not to create a charge can initiate

**lightning**and provoke its appearance.Note

Interesting fact: some native American peoples struck by lightning is considered a kind of initiation, necessary to achieve a shaman of higher level abilities.

# Advice 2: How to determine the distance to planets

Despite the fact that most close from us

**planets**extremely far from Earth,**distance**it is of ultimate importance. And if so, it can be determined. And this was first done a long time ago – in the days of the Ancient Greek astronomer, mathematician and philosopher Aristarchus from the island of Samos proposed a method of determining the distance to the moon and its size. How can you determine**the distance**to planets? The method is based on the phenomenon of parallax.You will need

- calculator;
- - radar;
- - stopwatch;
- - Handbook of astronomy.

Instruction

1

Radar is one of the modern methods of determining the distance from Earth to the planets (geocentric distance). It is based on a comparative analysis of the sent and reflected signal.Send a radio signal in the direction of interest

**of the planet**and turn on the stopwatch. When will the reflected signal to stop the clock. By the known velocity of propagation and the time during which the signal reaches**the planet**is reflected, calculate the**distance**to**the planet**. It is equal to the product of the speed at half the stopwatch.2

Before the advent of radar to determine the distance to objects in the Solar system using the method of the horizontal parallax. The error of this method is kilometer, and the measurement error of the distance using the radar centimeter.

3

The essence of the definition of the distances to the planets by the method of the horizontal parallax is to change the direction of the object when moving the observation point (parallax) – as a base is taken maximally spaced points together: the radius of the Earth. That is, the determination of distances to

**the planets**by the method of the horizontal parallax is a simple trigonometric problem. If you know all the data.4

Multiply 1 radian (the angle formed by the arc length is equal to radius expressed in seconds (206265) on the radius of the Earth (6370 km) and divide by the amount of parallax

**of the planet**at this time. The resulting value**is the distance**to**the planet**in astronomical units.5

At an annual or trigonometric parallax (base is the semimajor axis of earth's orbit) calculate distances to very distant planets and stars. By the way, parallax equal to one second determines

**the distance of**one parsec, and 1 PS = 206265 astronomical units. Divide 206265 seconds (1 radians) on the value of trigonometric parallax. The resulting quotient is**the distance of**to the interest**of the planet**.6

Finally,

**distance**to planets can be calculated using the third law of Kepler. The calculation is quite complicated, so let's proceed to the final part.Construct the squared value of the orbital period**of the planet**around the Sun. Calculate the cube root of this value. The resulting number is**the distance**from the interest**of the planet**to the Sun in astronomical units, or heliocentric**distance**. Knowing the heliocentric**distance**and the position of the planets (angular**distance****of the planet**from the Sun), you can easily calculate the geocentric**distance**.