1943 Poetry Response free essay sample

Desiree Adams The Poem â€Å"1943† by Donald, Hall was a very good poem. When I looked at the title I thought the poem was going to be about WWII because the year 1943 was during the time of WWII. When I read the poem it was about a bunch of teenagers who are getting prepared for war and trained on how to act and be tough. This poem talks about how teen boys are getting taught in school and other places on how to be men in the army and go to war. It also talks about how they have to realize that war is bloody in brutal ,so they have to have tough skin if they want to make it into the military. This poem reminds me of the story my grandfather told me about when he enlisted to the marines and had to go to Paris, Island for basic training. He told me that back home they made war sound like something a young boy should do in order to become a man. We will write a custom essay sample on 1943 Poetry Response or any similar topic specifically for you Do Not WasteYour Time HIRE WRITER Only 13.90 / page When he got to basic training he told me he was very nervous and as soon as he got there they trained them and toughened them up for the war that was happen in Vietnam. My grandfather would tell me about how the Marines made him into a fine man because it taught him to put away all the childish things and it toughened him up , so he could be able to face the challenges of the real adult world and life. The poem makes me feel glad that young boys are getting taught back then about how to be real men. I think that some of the boys we have in our society need a harder class other than ROTC to teach them how to become real men and grow up. This poem talks about how they were teaching boys in high school how to prepare for the war and becoming better men in life.

Free Essays on Sonic Case Study

Executive Summary Beginning with one restaurant, Sonic has become the largest drive-in chain in the United States. While they are smaller than their competitors, they are still leading in sales growth, customer loyalty and customer satisfaction. Sonic restaurants saturate the southern U.S. This gives them the opportunity to expand to other area. However, Sonic is reluctant due to the colder climates and their basis as a drive-in restaurant. Sonic should look at adding or combining capabilities to it’s restaurants to increase competitiveness and make it easier for them to expand into other areas without limiting themselves. Situational Analysis In 1953, Troy Smith, the founder of SONIC and World War II veteran, was living in Shawnee, Oklahoma. Troy dreamed of owning his own restaurant business. In fact, he had already tried twice. Troy first owned a small diner called the Cottage Cafà ©. The income he received was barely enough to make a living for himself and his family. Troy sold the Cottage Cafà © and bought a bigger restaurant. His next business, the Panful of Chicken, was so successful that he tried opening more. Unfortunately, fried chicken didn't do well in early 1950s Oklahoma and Troy closed his Panful of Chicken restaurant. Troy then owned a steak house that had a root beer stand attached. This root beer stand, called The Top Hat proved more profitable and eventually outlasted the steak house. While traveling to Louisiana, Troy saw some homemade intercom speakers in use at a local hamburger stand. He contacted the innovator in Louisiana and asked him to make an intercom for the Top Hat. He then hired some local electronics wizards to install the system. He then added a canopy for cars to park under and servers to deliver the food right to customers’ cars. During the first week after the intercom was installed, the Top Hat took in $1750. With his new partner, Charlie Pa... Free Essays on Sonic Case Study Free Essays on Sonic Case Study Executive Summary Beginning with one restaurant, Sonic has become the largest drive-in chain in the United States. While they are smaller than their competitors, they are still leading in sales growth, customer loyalty and customer satisfaction. Sonic restaurants saturate the southern U.S. This gives them the opportunity to expand to other area. However, Sonic is reluctant due to the colder climates and their basis as a drive-in restaurant. Sonic should look at adding or combining capabilities to it’s restaurants to increase competitiveness and make it easier for them to expand into other areas without limiting themselves. Situational Analysis In 1953, Troy Smith, the founder of SONIC and World War II veteran, was living in Shawnee, Oklahoma. Troy dreamed of owning his own restaurant business. In fact, he had already tried twice. Troy first owned a small diner called the Cottage Cafà ©. The income he received was barely enough to make a living for himself and his family. Troy sold the Cottage Cafà © and bought a bigger restaurant. His next business, the Panful of Chicken, was so successful that he tried opening more. Unfortunately, fried chicken didn't do well in early 1950s Oklahoma and Troy closed his Panful of Chicken restaurant. Troy then owned a steak house that had a root beer stand attached. This root beer stand, called The Top Hat proved more profitable and eventually outlasted the steak house. While traveling to Louisiana, Troy saw some homemade intercom speakers in use at a local hamburger stand. He contacted the innovator in Louisiana and asked him to make an intercom for the Top Hat. He then hired some local electronics wizards to install the system. He then added a canopy for cars to park under and servers to deliver the food right to customers’ cars. During the first week after the intercom was installed, the Top Hat took in $1750. With his new partner, Charlie Pa...

The Aerodynamics of Future Electric Cars Research Paper

The Aerodynamics of Future Electric Cars - Research Paper Example The researcher states that changes in global demand patterns, market forces, environmental concerns and the ever present danger of fleeting fossil fuel reserves are forcing automobile manufacturers and research scientists to look for alternative means to fuel automobiles. One facet of these developments has been electric vehicles that are powered exclusively through electric batteries. The emergence of electric vehicles has put in motion a number of new design challenges such as the aerodynamics of such vehicles because aerodynamics represent a large loss during normal functioning of all kinds of automobiles. Drag created by a moving vehicle represents one of the largest losses of energy created by an automobile’s engine. Conventional automobiles may lose as much as 40% of the total power to air drag. As with other conventional bodies, the aerodynamic drag exerted by air on a vehicle is directly proportional to the square of the velocity of the vehicle. For typically aerodynam ic automobiles the coefficient of drag and the accompanying area need to be as small as possible in terms of design considerations in order to minimize the drag encountered. There has been an ongoing struggle to create vehicles with as low a coefficient of drag as possible. Typically well designed vehicles display coefficients of drag of the order of 0.13 while a coefficient of drag of 0.1 is achievable through special design considerations.... Moreover considerations of an acoustical nature are also reduced through the use of electric engines that produce far less noise than conventional engines. However this has been criticized for increasing danger to blind people because the incoming vehicle would not possess a sound. (The Week, 2010) Based on these considerations it can be seen that the design of electric vehicles is an altogether different domain from conventional automobile design. The inclusion of new components such as the electric engines places new constrains on design that require solutions through out of the box thinking. This paper will attempt to describe the various major challenges being posed in terms of design and their current solutions along with their future outlook. 2. Conventional Automobile Packaging and Acoustics Conventional automobiles have been built and packaged in nearly the same way for decades. The early pioneering research into automobiles has created a stable platform that is dogmatically used as per vehicle class and usage. For example most passenger cars created along conventional design philosophy house the engine in the front and use a front wheel drive system while load carriers such as trucks use front mounted engines with rear wheel drive. Moreover recent advances in computational fields have allowed designers to create more light weight and singular construction frames better known as monocques. While some of these design elements such as a light weight bodies, four wheels and singular construction have been applied to building electrical vehicles but other packaging constraints have changed altogether. The design configuration and considerations for conventional automobiles are being

Changes in market power Research Paper Example | Topics and Well Written Essays - 250 words

Changes in market power - Research Paper Example Hence, despite the decreasing values of hotel prices, the market power can still be strengthened through the use of advertising strategy (Tung et al., 2010). The market power of hotel industries has gained an incremental value especially when hotel management lowered down their room rates. Celen and Thomas (2009) implicated that the changes of the market power within hotel industries are increasing towards a better profit because lowered priced rooms are mostly booked and occupied. In addition, Eden (1990) and Dana (1999) explicated that hotel industries can gain a change in market power when the distribution of room rates is equal and lowered to an affordable price. Consequently, market power is important within hotel industries in order to cope up with the increasing industrial competition (as cited in Celen & Thomas, 2009). Accordingly, the market power is determined through the market structure of the hotel industry, in which this will influence the changes of the market power held by the particular firm. Moreover, the vertical integration can benefit the market power of hotel industries and be able to manage their services despite increasing competition. Hence, the market power depends on how the hotel industries market their low priced rooms in order to sustain and regulate their market structure (Celen & Thomas, 2009; Tung et al., 2010). Tung, G.-S., Lin, C.-Y., & Wang, C.-Y. (2010). The market structure, conduct and performance paradigm re-applied to the international tourist hotel industry. African Journal of Business Management, 4 (6),

Online Marketing For Airline Industry Literature review

Online Marketing For Airline Industry - Literature review Example The use of online marketing is quite advantageous for the airline industry because it provides access to potential customers even in the most remote areas of the world. The internet is currently one of the most accessed tools of marketing in the world and because of this; online marketing carries with it a higher possibility of having access to more customers than other traditional means of marketing. Among the biggest advantages of online marketing for the airline industry is that it is not only done at a local level, its marketing campaigns are also done at a regional, national, and international level and this is one of the reasons why this means of marketing is one of the most successful of its kind worldwide. Online marketing is so efficient that it is able to compete effectively against other marketing strategies and in fact, it has an edge over them. When compared to other means of marketing, one is likely to find that online marketing is probably more popular than the others hence more returns to those companies that invest in it. This is means of marketing which most airline industries in the world should aspire to invest in because it is a guarantee of their success not only in the present, but also in the future. The online marketing of an airline company can be used as a means through which it can be able to attract the best talent to seek jobs within it. With some of the best people working for it, not only will such a company be able to offer excellent services, but its reputation is likely to grow, since the internet has become a means through which news travels fast. Making excellent job offers through the internet and acquiring good staff through it is a means to make the public more aware of the company. Because online marketing is one of the leading marketing strategies, this is where most companies and other institutions go to when they need to acquire people in to work for them. In addition, marketing online ensures that a company’s clients stay up to date with the current knowledge about it as well as ensuring that they take advantage of all offers that the company has to give, hence giving the company a competitive edge over other airlines. Online marketing ensures that an airline is able to make adjustments quickly, according to the changes in the marketing scene in the world and it does this for assisting its clients keep up to speed of things so that they do not lose any opportunities if there are any unexpected changes in the market. Online marketing provides a swift means through which individuals can easily be able to make connections with people and resources which they have need of in order receive the services they want from the airline companies. Context This paper discusses the need for companies in the airline industry to turn to the online marketing in order to reach more customers in the process of marketing their products. It deals with how these companies are moving from the old mode of market ing and relying heavily on new sources such as social networks. Instead of the impersonal marketing modes of the past, these companies have now realized that it is better to deal with potential customers on a more personal basis so that data that is more reliable can be collected. Due to the availability of a lot of data that is brought about by social networks and consumer websites, online marketing

Solar Radio Emissions: Investigating Reactivated Prominences

Solar Radio Emissions: Investigating Reactivated Prominences Madeleine Eve Andrew Johnston Solar Radio Emissions in Investigating Reactivated Prominences Literature Review Abstract Astronomical objects that have a changing magnetic field can produce radio waves, which are the longest waves in the electromagnetic spectrum. By studying the radio waves emitted by the Sun, astronomers can acquire information about its composition, structure and motion. This aim of the present project is to use solar radio emissions produced during the re-activation of prominences in order to investigate possible energy sources for the activation. The purpose of this literature review is to analyse relevant papers on the subject matter that will be covered in this project, and give a summary of the literature in the field, whilst covering the history and importance of the topic, along with what types of instruments can be used to measure radio waves, and how radio waves are useful in studying prominences and their reactivation. 1 Introduction Radio waves are a type of electromagnetic radiation, which is a form of energy produced whenever charged particles are accelerated. They have frequencies from 3kHz to 300GHz, with corresponding wavelengths ranging from just 1mm to 100km. The understanding of solar radio emissions began in 1942, when an English physicist and radio astronomer, James Hey, was tasked to work on radar anti-jamming methods for the military. He had several reports of severe noise jamming of radars signals in the 4-8 meter wavelength range, and after examination, he realised that the direction of maximum interference was coming from the Sun, and concluded that the Sun radiates radio waves (M. Pick, 2008). The observation of solar radio emissions has proved to be a useful tool in our efforts to understand solar physics., In particular solar radio emissions can be used to study local plasma density and magnetic reconnection, which relates to the release, over periods of a few minutes, of magnetic energy stored in the corona and which accompany solar eruption events like prominences which this project will be focusing on. In addition, radio wave emissions from solar flares offer several unique diagnostic tools which can be used to investigate energy release (A. O. Benz; 2005), plasma heating, particle acceleration, and particle transport in magnetized plasmas. A Solar flare is an observed sudden flash of brightness over the Sun’s surface or the solar limb, powered by magnetic reconnection. Scientists study the Sun through radio emissions and other electromagnetic emissions and this has an additional advantage in that it provides a better understanding other stars, and the important processes they have to offer, such as nuclear fusion, which is a potential alternative energy source scientists have been trying to recreate on Earth for decades. The study of prominences and other eruptive events is important for providing an insight into the mechanics of the interior of the Sun, and also to assist us in the prediction of ‘space weather,’ which can effect satellites, and the Earth’s atmosphere and magnetic field. A solar prominence is a large, bright, gaseous feature that is anchored to the surface of the Sun in the photosphere, and extends outwards into the Sun’s corona in a loop shape. Solar prominences are made from plasma that is roughly 100 times cooler and denser than the plasma in the corona and so, when viewed with the sun as a backdrop, they appear dark, and are referred to as ‘filaments.’ They can last for several months, and are held in place above the Suns surface by strong magnetic fields. The exact composition of prominences is currently unknown, but it has been proposed that they are made up of roughly 10% helium and 90% hydrogen. Solar prominences, like other erupting projectiles, are useful to observe as they are good indicators of the magnetic field pattern of the sun, since they lie above the magnetic neutral lines. There are two basic types of prominences: quiescent and active-region prominences. Quiescent prominences are typically larger than active-region prominences, and also extend further into the corona, often reaching up to and over 30 000 kilometres above the Sun’s corona (T. E. Berger, 2012). In addition, quiescent prominences have a magnetic field of roughly 0.5-1mT, allowing them to extend further from the surface of the Sun than active-region prominences, which are much smaller, have much larger magnetic fields of around 2 – 20mT, and mostly do not travel over 30 000km. This project will largely be focusing on Quiescent prominences, as, extending further away from the Sun, they are easier to study using radio waves. Prominences are always projected from filament channels, which are along polarity inversion lines; where the magnetic field is highly non-potential (J. Chaf, 2005). These channels are the source of all major solar eruptions, such as coronal mass ejections and flares. The temperature of a prominence that hasn’t erupted, is typically , and these often appear as a long horizontal sheet of plasma. Several different models have been proposed in order to explain how cool, dense objects like prominences can be supported and thermally isolated from the surrounding hot coronal plasma. It is generally accepted that these models can generally be placed into one of two main categories: dip models, and flux rope models (for example: D. H. Mackay, 2010, D. J. Schmit, 2013, P. F. Chen; 2008). The main similarity between dip models and flux rope models is the suggested existence of concave-upward directed magnetic fields to support the prominence plasma against the downward gravitational force. Following this mechanism, it can be assumed that the plasma in a prominence is frozen to the magnetic field lines. Prominence plasma, however, is actually only partially ionised, and so it is not entirely clear how the non-ionized portion of plasma is supported, and how rapidly the neutral material might drain across the magnetic field lines. Scientists are still researching how and why prominences are formed, and the cause for their reactivation. The models proposing how prominences are supported are vital in understanding their formation and reactivation. 2 Radio Emissions with Prominences Measurable coherent radio emissions occur during flares, and are intermittent and in bursts, driven by the magnetic reconnection process, giving them the term ‘radio burst.’ Previous experiments (J. P. Raulin; 2005, J. P. wild; 1956, R. F. Wilson; 1989, G. Swarup; 1959) in measuring radio emissions produced from prominences have found that Type I bursts are predominantly emitted, Type I being characterised by their long lifespan lasting from hours to days, having a frequency of 80-200mHz with corresponding wavelengths of roughly 2m, and being produced by electrons with a charge of several keV within coronal loops. Moving Type IV radio bursts are also associated with prominence eruptions, these last from half an hour to 2 hours, with a frequency of 20-400MHz, and a corresponding wavelength range of 1 to several meters. As mentioned in the introduction, scientists can use radio waves to gain an insight into how plasmas behave during the prominence eruption process. This can be done through magnetohydrodynamics (MHD), which is the study of the dynamics of electrically conducting fluids. Scientists have previously used MHD equations in investigations to understand the formation and reactivation of prominences (J. A. Linker; 2001, D.J. Schmit;2013, G. P. Zhou;2006, A. K. Srivastava; 2013). An investigation using SDO/AIA (T. E. Berger; 2012) on the formation of prominences produced a series of images that showed the reactivation of a prominence. The sequence showed that after a prominence has completed its eruptive cycle, it slowly disappears due to drainage and the lateral transport of plasma, and a bright emission cloud forms in the upper regions of the coronal cavity. The cloud descends towards the lower region of the cavity while successively becoming brighter, and a new prominence then forms, rapidly growing in both the vertical and horizontal dimensions. The new prominence is the reactivated old prominence. The coronal cavity core in the image then grows darker as the reactivated prominence continues to grow. The reactivated prominence reaches its maximum size after a number of hours, and the emission cloud in the cavity reduces correspondingly. Using the time sequence of images from this T. E. Bergers paper, an idea of what to search for in data to find reactivat ed prominences can be formed. Work has been performed (by C. Chifor; 2006; D. H. Mackay; 2010, D. J. Schmit, 2013) which also investigates how prominences are formed, concluding that reconnection events trigger different phases in prominence eruption. The flux rope model discussed earlier has been found to be a good model in several investigations (S. E. Gibson; 2006, P. F. Chen; 2008, G. P. Zhou, 2006). Helical field lines provide a support for the mass of the prominence, and are capable of storing the magnetic energy needed to propel the prominence. A coronal flux rope can be interpreted as a magnetic structure which consists of field lines that intricately twist around each other a number of times between the two ends that are anchored to the photosphere. Studies mentioned earlier involving MHD have been found to support the flux rope model, making the model a good investigation point for the project. Further research has been carried out into the cause of reactivated prominences (R. F. Wilson; 1989), producing evidence that suggests that as the initial prominence dissipates, a ‘feed-back’ mechanism occurs, during which interactions of the large scale loops trigger burst activity in lower lying loops. 3 Instruments There are two main types of instruments that can be used to observe objects in the radio wave portion of the electromagnetic spectrum, the type selected for use depending on the strength of the signal and the amount of detail needed. The first type of instrument comprises radio telescopes, which are a form of directional radio antenna. As the range of frequencies in the radio wave portion of the electromagnetic spectrum is very large, there are a variety of different antennae that are used in radio telescopes, differing in their size, design and configuration. When measuring wavelengths of 30-3 meters, the radio telescopes use either directional antenna arrays, or large stationary reflectors with moveable focal points. At shorter wavelengths dish style radio telescopes are more largely used. The second type of instrument comprises radio interferometers, which are made up of arrays of telescopes or mirror segments. The main benefit of using a radio interferometer is that the angular resolution is similar to that of a radio telescope with a large aperture, however, radio interferometers do not collect as many photons as radio telescopes, and they cannot detect objects that are too weak. However, an array of telescopes will provide very good resolution as a result of aperture synthesis. Aperture synthesis is an imaging process that mixes signals from the array of telescopes to produce images with an angular resolution equivalent to that of a single instrument with a diameter equal to the overall size of the array of telescopes. This makes it easy to obtain high resolution images of the Sun. SDO/AIA EUV Several different types of data that can be used to review the radio emissions of the Sun in order to extract information on prominences have been researched. The first is SDO/AIA EUV data; SDO being the Solar Dynamics Observatory, which is a NASA mission that has been observing the Sun since 2010. The goal of the SDO is to understand the influence of the sun on the Earth and close space by studying the solar atmosphere over time and space in many wavelengths at the same time. Currently, investigations are focused on how the Suns magnetic field is generated and structured, and how the stored magnetic energy is converted and released into the heliosphere and geospace in the form of solar wind, energetic particles, and variations in solar radiance, which is the measure of the power per unit area on the Earth’s surface. The SDO uses the Atmosphere Imaging Assembley (AIA), an instrument which provides continuous full-observations of the solar chromosphere and corona in seven extreme ultraviolet channels. The AIA is comprised of four telescopes providing individual light feeds to the instrument. The Extreme Ultraviolet Experiment (EUV) is the instrument that measures the Sun’s extreme ultraviolet irradiance, and incorporates physics based models in order to further understand the relationship between EUV variations and magnetic variation changes in the Sun (N. Labrosse, 2011). Fig 1. This image is an example of SDO/AIA data, taken from (T. E. Berger; 2012) from a time sequence which investigates the radio emissions from the Sun leading up to the reactivation of a prominence event. Using the data produced by the two, an image can be created of the Sun that combines physical processes such as prominences, with information on the magnetic field at the time. An example is shown in ‘Fig 1’ above, which shows a reactivated prominence eruption and its corresponding radio emission in the form of a cross-sectional image of the surface of the Sun. Data collected from the AIA has been made public through online databases, providing a ready set of images and films that can be analysed in order to observe prominences and their reactivation for this project. NoRH The second type of data that will be focused on in order to infer radio emissions from the Sun is Nobeyama Radioheliograph data. The Nobeyama Radioheliograph is an array of 84 antennas dedicated for solar observation at the Nobeyama Radio Observatory, located in the Japanese Alps, and was constructed with the purpose of observing the Sun, using non-thermal emissions in particular. The Nobeyama Radioheliograph is a radio interferometer, and the original data comprises sets of correlation values of all the combination of antennas. The antennas correspond to the spatial Fourier components of the brightness distribution of the solar disk. The Nobeyama Radioheliograph is particularly useful in studying prominences (M. Shimojo, 2005), as due to its large daily observation window, combined with the low time resolution of 1 second, and a spatial resolution of roughly 13†, it can produce highly dynamic images. Even though the NoRH is ground based, the consequences of the surrounding weather conditions are minimal compared to that of other ground based observations, and observations can take place even in turbulent unclear weather. NoRH has also developed an automatic detection method, the most important factor in using the instrument to detect prominences, as data will be recorded automatically when there is an eruptive projectile. However, due to the limited time resolution and the field of view, NoRH cannot detect vary fast or very slow eruptive events, simultaneous events, and events where the structure has a weak brightness. Fig 2 This is an image taken by the NoRH (M. Shimojo) which is an example of a prominence eruption, recorded by the automatic limb detection method. The panels are negative images, so the dark region indicates the high temperature. NoRH uses the radio interferometer to create images of the Sun such as in ‘Fig 2,’ which is an example of use of the automatic limb detection method to record images of prominence eruption. Data recorded from the NoRH automatic limb detector has also been made public through online databases, giving a further set of images that can be analysed in order to extract information on prominences and their reactivation. 4 Conclusion The topics covered in the papers that were researched lead to an adequate proposal of how to investigate the reactivation of prominences. Using NoRH and AIA data from SDO, the radio bursts emitted during the collapse and reformation of a prominence, an idea of what causes the reformation can be found. The investigation will centre on the different models, primarily the magnetic flux rope model, and the magnetohydrodynamics behind them that have been proposed for the formation of prominences, and how these models could support the ‘feed-back’ theory. 5 References J. P. Wild, H. Zirin. On the Association of Solar Radio Emission and Solar Prominences (1956) 320, 322, 323 G. Swarup, P. H. Stone, A. Maxwell. The Association of Solar Radio Bursts With Flares and Prominences. Radio Astronomy Station of Harvard College Observatory (1959) 725,726 R. F. Wilson, K. R. Lang. Impulsive Microwave Burst amd Solar Noise Storm Emission Resolved with the VLA. Department of Physics and Astronomy (1989) 856, 864, 866 J. A. Linker, R. Lionello, Z. Mikic. Magnetohydrodynamic Modeling of Prominence Formation with a Helmet Streamer. Science Applications International, California (2001) A. O. Benz, H. Perret, P. Saint-Hilaire, P. Zlobec. Extended Decimeter Radio Emission After Large Solar Flares. Institute of Astronomy, Switzerland (2005) 954, 955 J. Chaf, Y. Moon, Y. Park. The Magnetic Structure of Filament Barbs. (2005) 574-578 J. P. Raulin, A. A. Pacini. Solar Radio Emissions. Universidade Presbiteria Mackenzie (2005) 741-745 M. Shimoji, T. Yokoyama, A.Asai, H. Nakajima, K. Shibasaki. One Solar-Cycle Observations of Prominence Activities Using the Nobeyama Radioheliograph 1992-2004. University of Tokyo, School of Science (2005) 85, 86 S. E. Gibson, Y. Fan. Coronal Prominence Structure and Dynamics: A Magnetic Flux Rope Interpretation (2006) 1-5 G. P. Zhou, J. X. Wang, J. Zhang. Two Successive Coronal Mass Ejections Drivin by the Kink and Drainage Instabilities of an Eruptive Prominence (2006) 1244 C. Chifor, H. E. Mason, D. Tripathi, H. Isobe, A. Asai. The Early Phases of a Solar Prominence Eruption and Associated Flare: a Multi-Wavelength Analysis. Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences (2006) 966-968 P. F. Chen, D. E. Innes, S. K. Solanki, SOHO/SUMER Observations of Prominence Oscillations Before Eruption. Department of Astronomy, Nanjing University (2008) 4,5 M. Pick, N. Vilmer. Sixty-five years of Solar Radioastronomy: Flares, Coronal Mass Ejections and Sun-Earth Connection. Astron Astrophys Rev (2008) 6,7 D.H. Mackay, J.T. Karpen, J.L. Ballester, B. Schmieder, G. Aulanier. Physics of Solar Prominences: II – Magnetic Structure and Dynamics. Springer Science and Business Media (2010) 335-338 N. Labrosse, K. McGlinchey. Plasma Diagnostics in Eruptive Prominences from SDO/AIA Observations at 304 A. University of Glasgow (2011) 2-4 T. E. Berger, W. Liu, B. C. Low, SDO/AIA Detection of Solar Prominence Formation Within a Coronal Cavity. National Solar Observatory (2012) 1-4 D. J. Schmit, S. Gibson, M. Luna, J. Karpen, D. Innes. Prominence Mass Supply and the Cavity. Max Planck Institute for Solar System Research (2013) 1-5 A. K. Srivastava, B. N. Dwivedi, M. Kumar. Observations of Intensity Oscillaations in a Prominence-Like Cool Loop System as Observed by SDO/AIA: Evidence of Multiple Harmonics of Fast Magnetoacousic Waves (2013) 31

Characteristics Of A Comedy Essay -- essays research papers

Characteristics of Comedy There are many characteristics that make up a comedy. Characteristics such as mistaken identity, battle of the sexes, and jumping to conclusions are what set the comedic story apart from the tragedy. Within a comedy, no matter how much fault, and dismay may appear within the story, there always seems to be the classic ending of â€Å"†¦and they all lived happily ever after†¦Ã¢â‚¬  Comedies capture the viewer with a sense of compassion and love for the characters in the story. Each character has their own essence, to which they pertain a flaw of some sorts, which the audience can relate to. With the relation to characters there is defiantly a certain interest that is grabbed by the actors, which sucks the audience into the show.   Ã‚  Ã‚  Ã‚  Ã‚  Within the comedic play Much To Do About Nothing, Shakespeare portrays many of the characteristics of a comedy. One of these characteristics is mistaken identity. When it is thought that the lady Hero is dead, the offer for Claudio to marry Hero’s cousin is presented, yet Hero is playing a fictional character of her cousin. Claudio had mistaken her identity for that of her cousins. The plan is not known at all until it all unwraps at the end of the play when the supposed cousin takes off her veil. In a modern comedy, mistaken identity is usually more settle, and less drastic then a wedding. Such as in the movie Clerks, when the employee running the store (Dante) steps away from the counter, and asks his friend to watch the store. Then the Dante’s ex-girlfriend comes into the store and asks for him. Dante has been sweating her for so long and wants to get back together, and so does she. His friend (Randal) being ignorant tells her he went home to chan ge or he’s in the back. She goes into the back of the store not to return until a few scenes later. Then she comes out from the dark back bathroom fulfilled, and out of breath to find Dante standing there talking to Randal. When she asks Dante how he got to the front of the store so fast, he replies what are u talking about. It ended up that she was in the bathroom with another man who had gone into the bathroom earlier. She had made love with this stranger thinking it was Dante. Mistaken identity can be quite drastic at times, and then again can be a dream come true.   Ã‚  Ã‚  Ã‚  Ã‚  It seems within every comedy there is a batt... ...e jumps to the wrongful conclusion of this tragedy. Even though it seems like Claudio has much fault in the scandal, it is not at all his fault. Within modern day life it is not uncommon to find someone jumping to conclusions about someone, or a situation. Within the comedic sense it shows the ignorance of man, and how impatient we are to find out the truth. It seems as though through this characteristic of comedy, there is the reflection of man’s impatience, and how we grab the first possible answer without looking into it just to get an answer; the easiest answer.   Ã‚  Ã‚  Ã‚  Ã‚  All aspects and characteristics of comedy from the past can relate into characteristics of comedy form the present. Although stories and plots are different, the general formula to have a comedy remains the same throughout the ages. Relating these characteristics of the comedy Much To Do About Nothing, by Shakespeare, to comedies from the present is simple because every comedic story contains the same characteristics of a comedy. To be a comedy, a story must contain comedic characteristics. Without these characteristics, there would be no comedy, and with no comedy the world would frown.