1 / 33

ELECTROMAGNETIC SPECTRUM

ELECTROMAGNETIC SPECTRUM. Transverse waves created by the sun as well as electrical and magnetic energy sources and sent through the vacuum of space to Earth. What is the Electromagnetic Wave. ?. الموجة. [wikipedia.org هذه الصورة منقولة عن ]. EM Spectrum Parameters.

Download Presentation

ELECTROMAGNETIC SPECTRUM

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. ELECTROMAGNETIC SPECTRUM Transverse waves created by the sun as well as electrical and magnetic energy sources and sent through the vacuum of space to Earth.

  2. What is the Electromagnetic Wave ?

  3. الموجة [wikipedia.org هذه الصورة منقولة عن]

  4. EM Spectrum Parameters • Actually, the electromagnetic spectrum can be expressed in terms of energy, wavelength, or frequency. Each way of thinking about the EM spectrum is related to the others in a precise mathematical way. So why do we have three ways of describing things, each with a different set of physical units? After all, frequency is measured in cycles per second (which is called a Hertz), wavelength is measured in meters, and energy is measured in electron volts.

  5. What is the relationship between frequency and wavelength ? C = 3*108 m/s

  6. يستغرق انتقال الضوء (أو الإشارة اللاسلكية) 1،3 ثانية للإنتقال من القمر إلى الأرض، 8 دقائق من الشمس إلى الأرض و 300 مايكروثانية (0،3 ميلي ثانية) للإنتقال مسافة تعادل 100 كيلومتر. • From Moon to Earth (1.3 s) • From Sun to Earth (8 min and 300 u s) • For 100 km (0.3 ms) • From Aflaj to Riadh (0.9 ms)

  7. What is the relationship between wavelength, frequency, and energy ?

  8. What is the Electromagnetic Spectrum ?

  9. EM Spectrum • We may think that radio waves are completely different physical objects or events than gamma-rays. They are produced in very different ways, and we detect them in different ways. But are they really different things? The answer is 'no'. Radio waves, visible light, X-rays, and all the other parts of the electromagnetic spectrum are fundamentally the same thing. They are all electromagnetic radiation.

  10. Measuring the electromagnetic spectrum • You actually know more about it than you may think! • The electromagnetic (EM) spectrum is just a name that scientists give a bunch of types of radiation when they want to talk about them as a group. • Radiation is energy that travels and spreads out as it goes-- visible light that comes from a lamp in your house or radio waves that come from a radio station are two types of electromagnetic radiation. • Other examples of EM radiation are microwaves, infrared and ultraviolet light, X-rays and gamma-rays. • Hotter, more energetic objects and events create higher energy radiation than cool objects. • Only extremely hot objects or particles moving at very high velocities can create high-energy radiation like X-rays and gamma-rays.

  11. Electromagnetic SpectrumDiagram

  12. Electromagnetic Waves

  13. Radio Waves • Here are the different types of radiation in the EM spectrum, in order from lowest energy to highest: • Radio: yes, this is the same kind of energy that radio stations emit into the air for your boom box to capture and turn into your favorite Mozart, Madonna, or Coolio tunes. But radio waves are also emitted by other things ... such as stars and gases in space. You may not be able to dance to what these objects emit, but you can use it to learn what they are made of.

  14. Microwaves Wave • Infrared wavelengths span from 710 nanometers to 1 millimeter (from the width of a pinpoint to the size of small plant seeds). At a temperature of 37 degrees C, our bodies radiate with a peak intensity near 900 nanometers.

  15. Microwaves Waves • Microwaves: they will cook your popcorn in just a few minutes! In space, microwaves are used by astronomers to learn about the structure of nearby galaxies, including our own Milky Way!

  16. Infra-Red (IR) Wave • Infrared wavelengths span from 710 nanometers to 1 millimeter (from the width of a pinpoint to the size of small plant seeds). At a temperature of 37 degrees C, our bodies radiate with a peak intensity near 900 nanometers.

  17. Infra-Red (IR) Waves • Infrared: we often think of this as being the same thing as 'heat', because it makes our skin feel warm. In space, IR light maps the dust between stars.

  18. Visible Wave • Visible light covers the range of wavelengths from 400 to 700 nanometers (from the size of a molecule to a protozoan). The Sun emits most of its radiation in the visible range, which our eyes perceive as the colors of the rainbow. Our eyes are sensitive only to this small portion of the electromagnetic spectrum. Visible light covers the range of wavelengths from 400 to 700 nanometers (from the size of a molecule to a protozoan). The Sun emits most of its radiation in the visible range, which our eyes perceive as the colors of the rainbow. Our eyes are sensitive only to this small portion of the electromagnetic spectrum.

  19. Visible Waves • Visible: yes, this is the part that our eyes see. Visible radiation is emitted by everything from fireflies to light bulbs to stars ... also by fast-moving particles hitting other particles.

  20. Ultraviolet (UV) Wave • Ultraviolet radiation has wavelengths of 10 to 310 nanometers (about the size of a virus). Young, hot stars produce a lot of ultraviolet light and bathe interstellar space with this energetic light.

  21. Ultraviolet (UV) Waves • Ultraviolet: we know that the Sun is a source of ultraviolet (or UV) radiation, because it is the UV rays that cause our skin to burn! Stars and other "hot" objects in space emit UV radiation.

  22. X-rays Waves • X-rays range in wavelength from 0.01 to 10 nanometers (about the size of an atom). They are generated, for example, by super-heated gas from exploding stars and quasars, where temperatures are near a million to ten million degrees.

  23. EM Spectrum • X-rays: your doctor uses them to look at your bones and your dentist to look at your teeth. Hot gases in the Universe also emit X-rays .

  24. Gamma-rays Waves • Gamma rayshave the shortest wavelengths, of less than 0.01 nanometers (about the size of an atomic nucleus). This is the highest frequency and most energetic region of the electromagnetic spectrum. Gamma rays can result from nuclear reactions taking place in objects such as pulsars, quasars, and black holes.

  25. Gamma-rays Waves • Gamma-rays: radioactive materials (some natural and others made by man in things like nuclear power plants) can emit gamma-rays. Big particle accelerators that scientists use to help them understand what matter is made of can sometimes generate gamma-rays. But the biggest gamma-ray generator of all is the Universe! It makes gamma radiation in all kinds of ways.

  26. مفاهيم للوقاية من بعض انواع الإشعاع

  27. أولا: استعراض بعض مصادر الإشعاع فى حياتنا اليومية 1- الشمس و ينبعث منها: - أشعة كهرومغناطيسية - رياح شمسية (p + e )1

  28. 2- الشعاع الكوني: يوجد غلبا خارج الغلاف الجوي ومكون من p وأيونات ثقيلة لها سرعة الضوء.2

  29. 3- النظائر المشعة: الطبيعى منها والمصنع:- الطبيعي3: - عدد ذري كبير 92 ~ 81 = Z و T1/2 كبير, مثلا اليورانيوم T1/2 = 4.5 billion years - عدد ذري صغير وT1/2 كبير. يوجد بنسب صغيرة جدا. - عدد ذري صغير وT1/2 صغير. مثل كربون14 الذى يوجد بنسبة 10-10 % وله T1/2 = 5730 years . يعاد تصنيعه في الطبيعة في الغلاف الخارجي 14N + n →14C + p المُصنع4: - ينتج عن المفاعلات النووية و المعجلات منها90Sr , 131I

  30. 4- أجهزة تصدر أشعة مثل: الحاسوب الليزر المحمول الرائي

  31. EM Spectrum • Electromagnetic radiation from space is unable to reach the surface of the Earth except at a very few wavelengths, such as the visible spectrum, radio frequencies, and some ultraviolet wavelengths. Astronomers can get above enough of the Earth's atmosphere to observe at some infrared wavelengths from mountain tops or by flying their telescopes in an aircraft

More Related