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How Do We Learn Objects of Interest to Intelligence Through Matter or Energy Interaction

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How do we learn about objects of interest to intelligence through matter/energy interaction: emission, reflection, refraction, and absorption?
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Use these References, plus the ones attached:
https://www(dot)satimagingcorp(dot)com/services/resources/characterization-of-satellite-remote-sensing-systems/
https://seos-project(dot)eu/remotesensing/remotesensing-c03-p01.html

Essay Sample Content Preview:

INTELLIGENCE THROUGH MATTER/ENERGY INTERACTION
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Technological advancements allow for the adoption of newer forms of military intelligence. Such progress arises from the persistent endeavor of the forces to improve their operations. For instance, the introduction of the satellite, among other imaging technologies, has enabled the literal depiction of a bird’s-eye view of the universe. The primary output of geospatial intelligence is imagery which experts interpret according to the laws of physical sciences. On the other hand, Geospatial information exclusively presents meaningful data, unlike imagery that captures the general outlook. The Geospatial information provides details such as roads, transport networks, location and shape of buildings, and elevation data. These data outputs are often integrated to generate an impressively detailed depiction. Therefore, proper interpretations are indispensable. The scientific concepts of emission, reflection, refraction, and absorption are crucial to deciphering geospatial data as they illustrate the influence of energy and matter on registered observations.
The scientific concept of emission is an intersection of the ideas of energy and matter. Experts define matter as anything that occupies space and has mass, while energy demonstrates work capability. It may exist in many different uniquely identifiable forms. Emissions occur when tiny particles of matter are released on the acquisition of sufficient energy leading to dislodgement and subsequent transmission. Although the particles may be too small to be seen, a convenient system can be constructed to allow for human visualization for ensuring they make sense for humans. The process is detection, and sensors depict the incident particles. As already implied, matter can either acquire or release energy. One can also define emission in the context of radiated energy. Unlike particles that are not easily detectable, the energy released can occur in forms that are readily discernable by humans, such as heat and light. The emission of light has been significant to astronomy because it can be mathematically evaluated to deduce the properties of the spatial bodies. The essential properties include their surface temperature, chemical composition, radial velocity, and spin through the IR spectrum. Thus, the concept of emission has enabled scientists to determine the properties of spatial bodies that are practically inaccessible to humans either due to extreme temperatures or lack of oxygen.
Notably, not every perceived incident particle or energy should be attributed to emissions. The laws of reflection allow for matter and particles to be deflected by appropriate bodies. Misinterpretation will occur if approaching matter-energy are treated as emissions when they are reflected. The error is very costly as it would lead to a false deduction of the properties of the respective spatial bodies. For instance, the planet’s mass is red because most red light is reflected while most blue light is absorbed. The planet’s chemical composition can be determined by shortlisting the chemical compounds that absorb the blue light and reflect the red light. Since the incidence of matter and energy may be indistinguishable between the concepts of emission and reflection, critical scientific evaluation is necessary to draw appropriate conclusions. The production of energy and matter is indicative of the background processes and reactions within a spatial body. Reflection may be facilitated by an inert body as long as it possesses a suitable surface. Introduction to Remote Sensing indicates that IR is significant in reflection, just as in emission. In this context, the incident IR is referred to as the reflective IR. The amount of the reflection similarly depicts some properties of the reflecting body. The reflections generate imagery for analysis.
The concept of refraction is crucial to the accurate interpretation of geospatial data. The laws of refraction have been utilized to construct lenses that are essential in imagery platforms. Galileo used the telescope, a product of refraction, to lay the foundation of the field of space exploration. The laws of refraction can be exploited to achieve the most effective imaging. The laws of refraction are also ideal to evaluate the incid...
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