Sunday, November 10, 2019

Are Mobile Phones a Necessity?

Mobile phones take a big part in our lifes nowadays. Although they are very useful, some people are beginning to ask if they are good for us or we really need them. In my opinion, we can’t talk about an easy life without mobile phone. In the first place, as their reason to be invented, we can connect with other people whenever and wherever we want. We can send messages to people and sometimes it can be very important. Especially at deathlines your saviors are mobile phones. Furthermore, as technology is improved, we can do more than just sending messages or talking with someone with mobile phones. We can save our files, listen music and we can connect to internet. We can receive and share a lot of things. And mobile phones’ cameras are very improved, we can catch very good scenes from life†¦ Nevertheles, there are so many people who say that mobile phones are making our lifes â€Å"short†. I mean mobile phones have a weak point: Radition. As many doctors say, mobile phones spread radition, which can be very dangerous for human life. Also, people say that mobile phones kill face to face relationship, basically people do not go to see their relatives, just call them. All in all, despite their weak points, mobile phones are making the life easier. I believe in future radition problem will be solved and mobiles phones will be exactly safe. And we have not to forget this: People make inventions good or bad†¦

Thursday, November 7, 2019

The Election of 1956 essays

The Election of 1956 essays The election of 1956, 48 states were in the union at that time and Dwight Eisenhower was president. Even though Eisenhower had not made and major changes during his first term he was still the publics for choice for the next election. In a poll taken in 1954, 65% of Americans had approved of the job he was doing. Some critics reflected his as lazy. Saying he rather be golfing, one of his own speech writers once described his as an oaf. But never the less he was unanimously nominated for the Republican ticket in 1956 along with Richard Nixon for vice president, who won with 457 electoral votes and 57.6% of the popular vote. For the Democrats Adlai E. Stevensons was anomously nominated and excepted the nomination. This campaign was won of the calmest in American history, for the same candidates ran in the election of 1952. Not many people thought the democrats even had a chance against Eisenhower. at a picnic at Eisenhowers farm in Gettysburg, where he officially began his campaign, He addressed the leaders attending on the top two issues: his health and Richard Nixons place on the ticket. He assured them he felt fine. And Richard Nixon assured them he would be able to fulfill the duties of president.Dwight Eisenhower was one of the most popular American leaders. British General Bernard C. Montgomery, who had fought in the war with Eisenhower is quoted saying He merely had to smile at you and you trusted in him at once. As a great World War II General people saw him as a sign of hope for peace in the post war era. He was elected in to office in 1952 by and overwhelming margin and an even greater one in 1956. In the 1956 election people were sure he would be re-elected, but they were not sure if he would accept the Republican parties nomination. Eisenhower suffers some medical ...

Tuesday, November 5, 2019

What Redshift Reveals About an Object

What Redshift Reveals About an Object When stargazers look up at the night sky, they see light. Its an essential part of the universe that has traveled across great distances. That light, formally called electromagnetic radiation, contains a treasury of information about the object it came from, ranging from its temperature to its motions. Astronomers study light in a technique called spectroscopy. It allows them to dissect it down to its wavelengths to create whats called a spectrum. Among other things, they can tell if an object is moving away from us. They use a property called a redshift to describe the motion of an objects moving away from each other in space. Redshift occurs when an object emitting electromagnetic radiation recedes from an observer. The light detected appears redder than it should be because it is shifted toward the red end of the spectrum. Redshift is not something anyone can see. Its an effect that astronomers measure in light by studying its wavelengths.   How Redshift Works An object (usually called the source) emits or absorbs electromagnetic radiation of a specific wavelength or set of wavelengths. Most stars give off a wide range of light, from visible to infrared, ultraviolet, x-ray, and so on. As the source moves away from the observer, the wavelength appears to stretch out or increase. Each peak is emitted farther away from the previous peak as the object gets recedes. Similarly, while the wavelength increases (gets redder) the frequency, and therefore the energy, decreases. The faster the object recedes, the greater its redshift. This phenomenon is due to the doppler effect. People on Earth are familiar with Doppler shift in pretty practical ways. For example, some of the most common applications of the doppler effect (both redshift and blueshift) are police radar guns. They bounce signals off of a vehicle and the amount of redshift or blueshift tells an officer how fast its going. Doppler weather radar tells forecasters how fast a storm system is moving. The use of Doppler techniques in astronomy follows the same principles, but instead of ticketing galaxies, astronomers use it to learn about their motions.   The way astronomers determine redshift (and blueshift) is to use an instrument called a spectrograph (or spectrometer) to look at the light emitted by an object. Tiny differences in the spectral lines show a shift toward the red (for redshift) or the blue (for blueshift). If the differences show a redshift, it means the object is receding away. If theyre blue, then the object is approaching. The Expansion of the Universe In the early 1900s, astronomers thought that the entire universe was encased inside our own  galaxy, the Milky Way. However, measurements made of other galaxies, which were thought to be simply nebulae inside our own, showed they were really  outside of the Milky Way. This discovery was made by astronomer Edwin P. Hubble, based on measurements of variable stars by another astronomer named  Henrietta Leavitt.   Furthermore, redshifts (and in some cases blueshifts) were measured for these galaxies, as well as their distances. Hubble  made the startling discovery that the farther away a galaxy is, the greater its redshift appears to us. This correlation is now known as Hubbles Law. It helps astronomers define the expansion of the universe.   It also shows that the farther away objects are from us, the faster they are receding. (This is true in the broad sense, there are local galaxies, for instance, that are moving towards us due to the motion of our Local Group.)   For the most part, objects in the universe are receding away from each other and that motion can be measured by analyzing their redshifts. Other Uses of Redshift in Astronomy Astronomers can use redshift to determine the motion of the Milky Way. They do that by measuring the Doppler shift of objects in our galaxy. That information reveals how other stars and nebulae are moving in relation to Earth. They can also measure the motion of very distant galaxies - called high redshift galaxies.   This is a rapidly growing field of astronomy. It focuses not just on galaxies, but also on other other objects, such as the sources of  gamma-ray bursts. These objects have a very high redshift, which means they are moving away from us at tremendously high velocities. Astronomers assign the letter z to redshift. That explains why sometimes a story will come out that says a galaxy has a redshift of z1 or something like that. The earliest epochs of the universe lie at a z of about 100.   So, redshift also gives astronomers a way to understand how far away things are in addition to how fast they are moving.   The study of distant objects also gives astronomers a snapshot of the state of the universe some 13.7 billion years ago. Thats when cosmic history began with the Big Bang. The universe not only appears to be expanding since that time, but its expansion is also accelerating. The source of this effect is dark energy,  a not-well-understood part of the universe. Astronomers using redshift to measure cosmological (large) distances​ find that the acceleration has not always been the same throughout cosmic history. The reason for that change is still not known and this effect of dark energy remains an intriguing area of study in cosmology (the study of the origin and evolution of the universe.) Edited by Carolyn Collins Petersen.

Sunday, November 3, 2019

Commercial Law Essay Example | Topics and Well Written Essays - 2250 words

Commercial Law - Essay Example The ability of Ellen to sue the council for damages not only to her business but also to her health offers particular advantages in protecting the reputation of her business because it can be proven that the council was negligent in its providing approval to start her business in the location that she did. Furthermore, the court will also presume that there was damage to the business or trading reputation of Ellen’s business and that she will need to be compensated by the council to ensure that its good reputation in the market is restored. If Ellen does not sue the council immediately on these grounds, then the reputation of her will be damaged further because council will be able to get away with not being able to fulfil its responsibility of ensuring that it provides accurate advice to her before she started her business. Establishment of claims The first thing that Ellen must do is to establish her claim for damages from the council is to prove that it is indeed the counci l was the negligent party, and that the latter had a duty to ensure that the information concerning her business location was accurate so that she would be able to establish it. Ellen’s claim against the council is one that cannot be disputed because it is as a direct result of the council’s employee’s negligence that Ellen came to be faced with all the problems she had after the disruption of her business as well as the development of her health problems.2 Therefore, in order for her case to go to court, she should make sure that her stand is not in any way disputed. Ellen would want to be able to prove that the council breached its duty and she has to do this in order to prove that it was negligent. Ellen must also be able to prove that it was as a direct result of the false information given by the council employee that brought about all the commercial and health damages that she sustained. It will be Ellen’s responsibility to prove that it was the fai lure in the council’s duty to provide legitimate information to her that led to the damages suffered by her.3 The third thing that Ellen will need to prove is that it was the negligent action of the council that was the cause of the damages that she is claiming compensation for and she will need to show proof of the medical records of the nervous breakdown she sustained as well as the photos of the renovation work being done in the neighbouring premises which came about as a result of the inaccurate approval that came about because of the council’s negligence.4 This will ensure that justice will be carried out in her favour and that she gets compensated for all the damages she sustained. The Plaintiff’s desired business environment It is the availability of a quiet space for meditation that would have provided Ellen with the opportunity to work effectively in order to not only achieve the goals of her business but also to provide satisfactory services to her cus tomers. It should be understood that in the type of business that Ellen is

Thursday, October 31, 2019

Aristotles View on the Natural of Teleology Essay

Aristotles View on the Natural of Teleology - Essay Example In this first argument, Aristotle draws to the comparison of rainfall and existent of animal parts which seems to be the most disputed contents in Aristotelian Corpus. In his argument, Aristotle tries to develop a final causation with regard to nature. Aristotle discusses the subject of natural teleology as a result of his predecessors trying to trace the final causation. The predecessors believe that things exist the way they as a result of necessity. This necessity includes the material elements that exist on their own natures and potentials. However, according to Aristotle, his predecessors describe natural phenomena with a focus on necessity. For Aristotle, his main focus is to establish the existence of other causes other than the material necessity. Since nature is a source of change, it acts to serve something; therefore, Aristotle is on the view that teleology and necessity tend to be related (Asanuma, 2011). Regarding how Aristotle distinguishes his teleological view concerning nature and the views associated with his opponents, it is clear that Aristotle considers his view and those of his opponents to be incompatible. As such, Aristotle disagrees with the view material necessity operates in nature and does not require operations associated with teleology. On another note, these two forces associated with nature could be compatible; however, operations associated with material necessity may not be sufficient when it comes to producing positive results. The natural phenomena may not come about with the absence of a final cause, as such, explanations related to formal and final causation should not be reduced to explanations focusing on efficiency and material causation. While there is a school of thought that concur necessity and teleology seems compatible with regard to Aristotle’s view, this can only happen with the absence of ontological consequences (Krbalek & Vacek, 2013).  Ã‚  

Tuesday, October 29, 2019

Crime and punishment Essay Example | Topics and Well Written Essays - 1250 words

Crime and punishment - Essay Example Absence of punishments in a criminal justice system not only makes the criminals brave and fearless but also encourages them to commit crimes repeatedly. Here, I would like to say that punishment alone is not a very effective method for reducing the number of crimes because where it injects a sense of fear into the minds of the criminals; it also injects a sense of revenge in them, which is very harmful for the peace of whole society. A good method is to make use of reformation along with punishment because reformation changes the behavior and attitude of a criminal. Professional psychologists attempt to alter the behaviors of criminals by doing their psychotherapies and guiding them towards the right path. Therefore, I would say that although punishment is effective in reducing the number of crimes but it should be accompanied with reformation process in order to transform the criminals into peaceful citizens. To What Degree Punishment is Effective? The effectiveness of punishments depends on the type of punishment and the motive behind the punishments, which are given by the judges to the criminals. There are different types of punishments for different types of crimes. ... Punishments are very effective because they not only stop the criminals from committing crimes without any fear but also play a vital role in establishing and maintaining peace in a society. Punishments are very effective in reducing the number of crimes because it injects a sense of fear in the minds of the criminals, which stops them from committing any form of crime in future. The goals of punishments and one’s belief about the purpose of sentencing play a critical role in making punishments an effective tool for crime reduction. Decisions for punishments are only effective when they are based on merit because if a judge punishes a person without any solid proofs or by ignoring the ground realities, it injects a sense of revenge in the mind of that person, which makes him/her a real criminal once he/she comes out of jail. Therefore, I would say that the efficacy of punishments is deeply related with the merit-based decisions and with the purpose behind the punishments. Is C orporal Punishment Or The Death Penalty Justifiable In Any Sensible Way? Before going to describe whether corporal punishment and death penalty are sensible ways of punishments or not, let us get a better understanding of what corporal punishment and death penalty actually are. Corporal punishment means using physical force on a person as a form of punishment for a crime, whereas death penalty means sentencing a criminal to death because of some form of crime, which he/she commits. Both forms of punishments are given to the criminals in almost every country depending on the nature of crimes. I personally think that although corporal punishment is a harsh punishment, still it is a much better way to punish the criminals as compared to death

Sunday, October 27, 2019

Sensor Technology for Mineral Exploration

Sensor Technology for Mineral Exploration 1. Introduction Significant contribution is done by satellite remote sensing in the field of mineral exploration viz. Geological faults, fractures and mapping, which are associated with the ore deposits based on spectral signature, (Farooq and Govil 2013; Magendra and Sanjeevi 2014; Murphy and Monteiro 2011, Le Yo et al., 2011) the spectral signature helps in the recognizes hydrothermal altered rocks (Sabins, 1999). The multispectral remote sensing exhibits differences in spectral signatures which are insufficient spectral resolution for the hydrothermal altered mineral mapping (Clark, 1999). The Multispectral sensors viz. Landsat TM, ETM+, ASTER image processing helps in iron oxides mapping, the spectral ranges 1.55-1.75 Â µm and 2.08-2.35 Â µm is important for iron mapping (Gupta, 2003). The hyperspectral images provide a higher spectral resolution the the multispectral images (Clark et al., 1990; Magendra and Sanjeevi 2014; Van der Meer 2012). The discovery of new hyperspectral sensor technology in terms of both sensor and technical development has provided the opportunity to revisit previous remote sensing approaches for the mineral exploration as well as for the development of improved methods. Hyperspectral sensors have hundreds of channels, aircraft and satellite platforms which provide unique spectral datasets, and which are helpful in analyzing the surface mineralogy mapping (Goetz et al., 1985; Kruse et al., 2003; Debba et al., 2005, Vaughan et al., 2003). The airborne sensors like AVIRIS, HYDICE and Satellite sensor like Hyperion are used for mapping geology, snow etc. Hyperspectral remote sensing aims at providing the requirements like spectral, spatial and radiometric empower, measuring in terms of range, sampling, response, stability, uniformity, precision and accuracy. With the help of hyperspectral remote sensing we can find different minerals viz iron oxides, micas, chlorites, amphiboles, talc, serpentines, c arbonates, quartz, garnets, pyroxenes, feldspars and sulphates (Eva Papp and Cudahy 2002; Magendran and sanjeevi 2014; Hubbard and Crowley 2005). EO-1 Hyperion is the first Space based hyperspectral sensor, and it was launched on 21 November 2000 (Ungar et al., 2003). The Hyperion image has 30m spatial resolution, 242 channels and 7.7 km swath. The hyperspectral (Hyperion) sensor with 0.4-2.5Â µm spectral range, i.e. visible-near infrared (VNIR) spectrometer (approxmeterly0.4-1.0Â µm) and one short-wave infrared (SWIR) spectrometer (approximately 0.9-2.5Â µm) (EO-1 User guide) in which some minerals and rocks show good absorption and reflectance, due to variation in physicochemical properties, which help in their exploration mapping (Clark et al., 1990; Hunt et al., 1971). The spectral reflectance one can detect and identify the Earth surface and atmospheric constituents to measure the reflected spectra’s component concentration. We can find the distribution of the component and validate by improving models. The processing of Hyperion image is a challenging task as it consists hundreds of channels. The selection of required channels with its good apparent reflection requires good skills. The direct measurements of atmospheric properties are rarely available, and there are some techniques which surmise them from their imprint on hyperspectral radiance data. These properties are used to constrain highly accurate models of atmospheric radiation transfer to produce an estimate of the true surface reflectance. Moreover, atmospheric corrections of this type can be applied on a pixel by pixel basis since each pixel in a hyperspectral image contains an independent measurement of atmospheric water vapor absorption bands. There are different models available viz QUAC, 5S, 6S, ATCOR, ATREAM, HATCH, EFFORT Polishing, FLAASH etc (ITTVis, 2010). FLAASH is a MODTRAN4-based atmospheric correction software package, which provides accurate, physics-based derivation of apparent surface reflectance, through derivation of atmospheric properties such as surface albedo, surface altitude, water vapor column, aerosol and cloud optical depths, surface and atmospheric temperature from hyperspectral imaging data. FLAASH uses the most advanced techniques for handling particular stressing atmospheric conditions, such as the presence of clouds, cirrus and opaque cloud classification map adjustable spectral polishing for artifact suppression. The Hyperion image consists of a huge number of data sets which are supposed to be reduced dimensionally. The techniques like Minimum Noise Fraction (MNF) transform are used to reduce the number of spectral dimensions to be analyzed. The pure pixels are the most spectrally extreme pixels (Broadman et al., 1995), which spectrally correspond to the mixing end members. These end members form the base for the n-Dimensional visualization, and each selected end members are spectrally matched with USGS spectral library. The near visible near infrared image (VNIR) and shortwave infrared (SWIR) spectral range cover the features of iron bearing minerals, hydroxyl bearing minerals sulphates and carbonates. The iron ores and iron bearing minerals have characteristic spectra in the 850nm to 950 nm wavelength (Magendran and Sanjeevi, 2014). The ferric iron minerals hematite (Fe203) has distinct spectral curves in the visible near-infrared image (VNIR), which is caused by absorptions and induced by crystal field transitions at about 465 nm, 650 nm and 850–950 nm (Townsend, 1987). The paper presents an attempt for mapping iron oxides in Chitradurga Schist belt by using the Hyperion image. The iron distribution mapping is made with the standardized hyperspectral methodologies. An attempt is also made by taking the spectra of iron in-vitro and compared it with the USGS spectral libraryfor mappingiron distribution. The Spectral Angle Mapper Classification (SAM) is an automated method of comparing the image spectra with the individual spectra, or a spectral library (Boardman 1992; Kruse et al 1993). SAM treats both individual spectra, spectral library spectra and calculates as vectors and its spectral angle. Since the SAM algorithm uses the only vector direction and not the vector length. The result of the SAM classification is an image showing the best match at each pixel. This method is typically used for determining the mineralogy and works better in the areas of identical regions. The USGS maintains a large spectral library composed of mineral and soil types, which has image spectra and can be compared directly. 1.1 Study Area and image data The lithology of the Chitradurga schist belt 13036’25’’N and 760 35’49’’E belongs to both Bababudan and Chitradurga Groups. (Figure 1) The Bababudan Group of rocks represented by metabasalt-quartzite formations and NNW trending synclinal Kibbanahalli BIF formation, wrapping around the Chikkanayakanahalli (CN Halli) gneiss and joining the main CN Halli belt near Dodguni (Radhakrishna, 1967; Srinivasan and Sreenivas, 1975; Seshadri et al., 1981; Ramakrishnan and Vaidynadhan, 2008). Chitradurga Group covers most of the CN Halli schist belt, represented by quartz-sericite-chlorite schist, quartzite, carbonates, Mn formations and BIF overlies Bababudan Group (Devaraju and Anantha Murthy, 1976, 1977). EO-1 Hyperion level 1 radiometric (L1R) product having 242 bands covering CN Halli area acquired on 14 April 2011 was used. The image covers the spectral range of 0.4 to 2.5Â µm at 10 nm bandwidth. However, only 155 of them are calibrated from visible-to-infrared (VNIR) and short wave-infrared (SWIR) regions. (Table 1) (EO-1 User Guide, 2003).