المرجع الالكتروني للمعلوماتية
المرجع الألكتروني للمعلوماتية

علم الفيزياء
عدد المواضيع في هذا القسم 11580 موضوعاً
الفيزياء الكلاسيكية
الفيزياء الحديثة
الفيزياء والعلوم الأخرى
مواضيع عامة في الفيزياء

Untitled Document
أبحث عن شيء أخر المرجع الالكتروني للمعلوماتية
استخدامات الطاقة الشمسية Uses of Solar Radiation
2024-11-28
Integration of phonology and morphology
2024-11-28
تاريخ التنبؤ الجوي
2024-11-28
كمية الطاقة الشمسية الواصلة للأرض Solar Constant
2024-11-28
صفاء السماء Sky Clearance
2024-11-28
زاوية ميلان المحور Obliquity
2024-11-28


GAIN  AND   LOSS  IN  A  CAVITY  
  
1465   03:18 مساءاً   date: 17-3-2016
Author : Mark Csele
Book or Source : FUNDAMENTALS OF LIGHT SOURCES AND LASERS
Page and Part : p160

GAIN  AND   LOSS  IN  A  CAVITY

      Assume that a laser operates with an output of 1 mW and has an output coupler with a reflectivity of 99.0% (and hence a transmission of 1.0%). This implies that the power circulating inside the cavity (the circulating power) is 100 mW. Of course, such intracavity power level is not usable: It is required to keep the rate of stimulated emission large enough and hence sustain laser action. The output beam (defined by the transmissivity of the output coupler) represents a loss in a laser cavity. Other losses include absorption and scattering in the laser medium itself and losses at windows terminating the lasing medium (e.g., windows on a gas laser plasma tube). Most laser gain media have low gains, so it is essential that losses be kept to a minimum. Since the output coupler represents a loss, the amount of transmissivity depends on the gain of the laser. When total losses in the laser exceed the gain of the medium, the laser will fail to oscillate.

     An experiment in which a variable loss (a glass slide) is inserted into the cavity of a He Ne laser. Let us reexamine the experiment by plotting the output power (which is, of course, proportional to circulating power) against loss in the cavity, as shown in Figure 1.1. Circulating power is easily measured simply by measuring laser output and multiplying by the transmission of the OC. In this experiment the OC has a transmission of 1.0%, so that for a measured output of 370 μW, the intracavity circulating power is 37 mW. The maximum inserted loss that may be tolerated in this laser is found to be 1.2%. When this loss is summed with other losses in the laser, such as absorption in the medium itself and the loss of the OC (1.0%), the gain of the laser medium may be calculated.

      It is obvious from Figure 1.1 that even small losses have a large effect on the output power of a laser losses in a real laser must thus be kept as low as possible. Where possible, such as in a He Ne laser, mirrors are often sealed directly into the ends of the tube so that there are no windows in the optical path to increase loss. In many lasers, though, cavity mirrors must be isolated from the discharge to prevent attack from the plasma. Use of external optics is also required when a laser uses a wavelength selector. In these cases the ends of the plasma tube must be capped with an optical window. To minimize losses, optical windows are angled at

Figure 1.1. Effect of cavity loss on output power in a laser.

the Brewster angle, which polarizes the output of the laser since loss is essentially zero in one polarization and very significant in the other polarization.

     Figure 1.2 shows a Brewster window on a small air cooled argon laser tube. Protruding from the anode of this tube (with attached cooling fins visible in the

Figure 1.2. Brewster window in a gas laser.

Figure 1.3. Brewster window in a gas laser.

photograph) is a metal tube that is fused to a quartz tube sealed with a quartz window. The window is angled at Brewster’s angle. Most tubes contain two windows, one at each end of the tube, and each must be aligned in the same optical axis. As Figure 1.3 shows, where two Brewster windows are used, they should be oriented such that the intracavity beam does not shift overall position as it passes through both windows (as in the top diagram). The optimal angle can be determined from the Fresnel equation as the angle at which reflection (Rp) is reduced to zero. This angle depends on the index of refraction of the window material itself according to

 (1.1)

where n2 is the index of refraction of the window and n1 is the index of refraction of the surrounding media (1.00 for air and most gases). Hence Brewster’s angle is independent of the wavelength of the laser except that the index of refraction of the window may change as a function of wavelength, so for a multiple-wavelength laser such as an argon laser, the angle will be optimal for only one wavelength, with slightly higher losses at other wavelengths (only slightly higher since the index of refraction will not change much). The optimal output coupling can be calculated as a function of the gain of the device and total losses in the cavity. By reducing losses in the cavity such as those at tube windows, power output may be enhanced and weak transitions may be allowed to laser.




هو مجموعة نظريات فيزيائية ظهرت في القرن العشرين، الهدف منها تفسير عدة ظواهر تختص بالجسيمات والذرة ، وقد قامت هذه النظريات بدمج الخاصية الموجية بالخاصية الجسيمية، مكونة ما يعرف بازدواجية الموجة والجسيم. ونظرا لأهميّة الكم في بناء ميكانيكا الكم ، يعود سبب تسميتها ، وهو ما يعرف بأنه مصطلح فيزيائي ، استخدم لوصف الكمية الأصغر من الطاقة التي يمكن أن يتم تبادلها فيما بين الجسيمات.



جاءت تسمية كلمة ليزر LASER من الأحرف الأولى لفكرة عمل الليزر والمتمثلة في الجملة التالية: Light Amplification by Stimulated Emission of Radiation وتعني تضخيم الضوء Light Amplification بواسطة الانبعاث المحفز Stimulated Emission للإشعاع الكهرومغناطيسي.Radiation وقد تنبأ بوجود الليزر العالم البرت انشتاين في 1917 حيث وضع الأساس النظري لعملية الانبعاث المحفز .stimulated emission



الفيزياء النووية هي أحد أقسام علم الفيزياء الذي يهتم بدراسة نواة الذرة التي تحوي البروتونات والنيوترونات والترابط فيما بينهما, بالإضافة إلى تفسير وتصنيف خصائص النواة.يظن الكثير أن الفيزياء النووية ظهرت مع بداية الفيزياء الحديثة ولكن في الحقيقة أنها ظهرت منذ اكتشاف الذرة و لكنها بدأت تتضح أكثر مع بداية ظهور عصر الفيزياء الحديثة. أصبحت الفيزياء النووية في هذه الأيام ضرورة من ضروريات العالم المتطور.