USU GEOG 2800 Midterm

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36 Terms

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Definition of GIS

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Definition of Spacial Thinking

Find meaning in the shape, size, orientation, location, direction or trajectory, of objects, processes, or phenomena.

<p>Find meaning in the shape, size, orientation, location, direction or trajectory, of objects, processes, or phenomena. </p>
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Types of Spacial Patterns

Radom, Clustered, Dispersed

<p>Radom, Clustered, Dispersed </p>
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Why is spacial data important?

In order to solve problems and better understand the world, we need to ask questions, develop hypotheses, and question assumptions.

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Small vs Large Scale

Small scale is zoomed out with little detail. Large Scale is zoomed in with a lot of detail

<p>Small scale is zoomed out with little detail. Large Scale is zoomed in with a lot of detail </p>
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Vector data:

Lines, points, and polygons. Has attribute, locational, and topological data.

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Topological Data

Shows spacial relationships and describes how spatial data share geometric attributes

<p>Shows spacial relationships and describes how spatial data share geometric attributes </p>
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Types of Topology information:

Adjacency: info about neighborhoods of different objects.

Enclosure: info about spatial features that enclose other features.

Connectivity: info about the links between spatial objects.

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Vector Advantages:

Precise location of features, store attributes, flexible and easy to edit, smaller files, suitable for anaysis or areas, lenths, and networks.

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Vector Disadvantages:

Features seem homogenous, difficult to show gradients, imply discrete division that might not exist, and accuracy depends on scale.

<p>Features seem homogenous, difficult to show gradients, imply discrete division that might not exist, and accuracy depends on scale. </p>
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Raster Data:

Divides space into grid cells or pixels, each cell is spacial locations, size is constant, each cell has a value/attribute.

<p>Divides space into grid cells or pixels, each cell is spacial locations, size is constant, each cell has a value/attribute.  </p>
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Raster Data Types:

Continuous rasters: Shows gradual changes / cell values vary continuously to for surface. Ex: elevation, temp., density.

Discrete rasters: classifies data into categories. Ex: land cover, soil types, species comp.

<p>Continuous rasters: Shows gradual changes / cell values vary continuously to for surface. Ex: elevation, temp., density.</p><p>Discrete rasters: classifies data into categories. Ex: land cover, soil types, species comp.</p>
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Raster vs Vector Data Models

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Rasterization:

Creating a raster from vector data. You superimpose a grid over vector data, its sensitive to raster resolution (cell size), and information is lost.

<p>Creating a raster from vector data. You superimpose a grid over vector data, its sensitive to raster resolution (cell size), and information is lost. </p>
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Vectorization:

Creating vector data from raster data. Combine areas with similar values into polygons or locate similar areas with lines. Its sensitive to raster resolution and information is lost.

<p>Creating vector data from raster data. Combine areas with similar values into polygons or locate similar areas with lines. Its sensitive to raster resolution and information is lost. </p>
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Map Projections:

How to transform coordinates on the earth into a flat 2-D surface.

<p>How to transform coordinates on the earth into a flat 2-D surface. </p>
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Aspect in Map Projections, Normal, Transverse, and Oblique Aspect.

Aspect: the orientation of the developable surface.

Normal Aspect: the standard line is the equator.

Transverse Aspect: the standard line is a meridian.

Oblique Aspect: the standard line is a great circle other than the equator or prime meridian.

<p>Aspect: the orientation of the developable surface.</p><p>Normal Aspect: the standard line is the equator.</p><p>Transverse Aspect: the standard line is a meridian.</p><p>Oblique Aspect: the standard line is a great circle other than the equator or prime meridian. </p>
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Types of Distortion/Accuracy:

Equal-area: accurately represents areas/relative sizes.

Conformal: accurately represents shapes / intersecting lines, and maintains the angles

Equidistant: accurately represents distances along certain straight lines on the map

No map can be both equal-area and conformal

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Indicatrix

Small circles on the globe placed at the intersection of grid lines to visualize distortion.

<p>Small circles on the globe placed at the intersection of grid lines to visualize distortion. </p>
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Conformal Projections  

Shapes and angles are accurate, but size is distorted. Can be a Mercator or Conic Conformal projections.  

<p>Shapes and angles are accurate, but size is distorted. Can be a Mercator or Conic Conformal projections.&nbsp;&nbsp;</p>
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Cylindrical Mercator 

Conformal Map, tangent to Equator 

<p>Conformal Map, tangent to Equator&nbsp;</p>
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Lambert Conformal Conic

Accurately represents shapes around mid-latitudes. Often used for regional or continental maps.

<p>Accurately represents shapes around mid-latitudes. Often used for regional or continental maps. </p>
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Equal Area (Equivalent)

Sizes and ratios throughout the map are consistent, which is useful for comparing the size and extent of geographic areas. Can be Albers Equal Area Conic, Gall-Peters, or Mollweide.

<p>Sizes and ratios throughout the map are consistent, which is useful for comparing the size and extent of geographic areas.&nbsp;Can be Albers Equal Area Conic, Gall-Peters, or Mollweide. </p>
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Great Circle

The intersection of the surface of a sphere with a plane that passes through the center of the sphere.

  • Divides the sphere into two equal halves

  • The shortest distance between any two points on the surface of the Earth is always along a great circle

<p>The intersection of the surface of a sphere with a plane that passes through the center of the sphere.</p><ul><li><p>Divides the sphere into two equal halves</p></li><li><p>The shortest distance between any two points on the surface of the Earth is always along a great circle</p></li></ul><p></p>
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Small Circle

Small circle: the intersection of the surface of a sphere with a plane that does not pass through the center of the sphere

<p><strong>Small circle</strong>: the intersection of the surface of a sphere with a plane that does not pass through the center of the sphere</p><p></p>
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Meridians

Meridians, lines of equal longitude, are also great circles with a plane parallel to the axis of rotation of the earth. All meridians intersect at the poles, there are an infinite number of meridians

<p><strong>Meridians</strong>, lines of equal longitude, are also great circles with a plane parallel to the axis of rotation of the earth. All meridians intersect at the poles, there are an infinite number of meridians</p>
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Parallels

Parallels, lines of equal latitude, are all small circles (except the equator)

<p><strong>Parallels</strong>, lines of equal latitude, are all small circles (except the equator)</p>
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Latitude

Latitude, or north-south (y)

Angular position between the equator and the North or South Pole, 180 degrees: angle between 90º N and 90º S

 Parallels: lines of constant latitude - Small circles that run east-west, parallel to the equator

<p>Latitude, or north-south (y)</p><p>Angular position between the equator and the North or South Pole, 180 degrees: angle between 90º N and 90º S</p><p>&nbsp;Parallels: lines of constant latitude - Small circles that run east-west, parallel to the equator</p>
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How to determine Latitude

In the northern hemisphere, you can find your latitude by measuring the angle between Polaris (the North Star) and the horizon

Historically, a sextant or astrolabe would be used to measure the angle

<p>In the northern hemisphere, you can find your latitude by measuring the angle between Polaris (the North Star) and the horizon</p><p>Historically, a <strong>sextant</strong> or <strong>astrolabe </strong>would be used to measure the angle</p><p></p>
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Longitude 

Angular position on the earth’s surface between the intersection of plane that passes through the North and South Pole and the prime meridian (0º)

360 degrees: 180º W to 180 ºE

All lines of longitude (meridians) are great circles

<p>Angular position on the earth’s surface between the intersection of plane that passes through the North and South Pole and the prime meridian (0º)</p><p>360 degrees: 180º W to 180 ºE</p><p>All lines of longitude (meridians) are great circles</p>
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Prime Meridian

Prime meridian is arbitrarily located at the Royal Observatory in Greenwich, UK.

Because the technology for longitude was created in Britain

<p>Prime meridian is <strong>arbitrarily l</strong>ocated at the Royal Observatory in Greenwich, UK.</p><p>Because the technology for longitude was created in Britain </p>
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How to measure Longitude

There was no accurate way to measure longitude until the invention of the marine chronometer, a clock that could keep time at sea.

The Earth spins 15 degrees per hour (360*/24hrs), so (12 noon - current time) x 15*/hr = longitude

If it is 8:00 AM at the prime meridian and noon where you are = 4 hours later than prime meridian x 15º per hour = 60º East longitude

<p>There was no accurate way to measure longitude until the invention of the marine <strong>chronometer</strong>, a clock that could keep time at sea.</p><p>The Earth spins 15 degrees per hour (360*/24hrs), so (12 noon - current time) x 15*/hr = longitude</p><p>If it is 8:00 AM at the prime meridian and noon where you are = 4 hours later than prime meridian x 15º per hour = 60º East longitude</p>
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The Graticule 

Web of latitude lines (parallels) and longitude lines (meridians) is called the graticule

- Meridians & parallels always meet at right angles

- Distance between parallels is constant (about 69 mi)

- Distance between meridians varies by latitude (about 69 mi at equator, zero at poles)

- Meridians all intersect at the poles; parallels never intersect

<p>Web of latitude lines (parallels) and longitude lines (meridians) is called the graticule</p><p>- Meridians &amp; parallels always meet at right angles</p><p class="p1">- Distance between parallels is constant (about 69 mi)</p><p class="p1">- Distance between meridians varies by latitude (about 69 mi at equator, zero at poles)</p><p class="p1">- Meridians all intersect at the poles; parallels never intersect</p>
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Earth’s true shape:

Oblate spheroid or ellipsoid: the rotation of the earth causes polar flattening due to centrifugal force. This affects distance measurements on maps. 

The truest shape is a geoid, which means the the surface is not smooth, it has “Bumpiness” caused by variations in density of the Earth’s crust (which also causes variabilities in gravity). 

<p>Oblate spheroid or ellipsoid: the rotation of the earth causes polar flattening due to centrifugal force. This affects distance measurements on maps.&nbsp;</p><p>The truest shape is a geoid, which means the the surface is not smooth, it has “Bumpiness” caused by variations in density of the Earth’s crust (which also causes variabilities in gravity).&nbsp;</p>
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Geodetic Surveys 

Geodetic surveys: detailed measurements of the globe that take into account the curvature and variations in gravity of the Earth. 

Geodetic surveys are used to create a set of points in a control network with very accurate and precise locations

Markers (monuments) are often set up at control points

<p>Geodetic surveys: detailed measurements of the globe that take into account the curvature and variations in gravity of the Earth.&nbsp;</p><p>Geodetic surveys are used to create a set of points in a control network with very accurate and precise locations</p><p>Markers (monuments) are often set up at control points</p>
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