An almost Idiot's Guide (Post. GIS 2. 2) Comments Rss. What Is Post. GIS? Post. GIS is an open source, freely available, and. OGC compliant spatial database extender for the Postgre. SQL. Database Management System. In a nutshell it adds spatial functions. Post. GIS is very similar in functionality to SQL Server Spatial support, ESRI Arc. SDE. Oracle Spatial, and DB2 spatial extender except it has more functionality and generally better performance than all of those (and it won't bankrupt you). The latest release version. Postgre. SQL DBMS installs as an optional. Shiny at its simplest. In its simplest form, a Shiny application requires a server function to do the calculations and a user interface. Below we have the simplest. Things to Try: Spatially Enable an Existing Database An object-relational database (ORD), or object-relational database management system (ORDBMS), is a database management system (DBMS) similar to a relational database. How can I connect to a PostGIS database from ArcMap using ArcGIS Desktop 9.3 and later? I would like to be able to perform spatially enabled queries and receive the. The rest of this chapter goes into detail each of the above installation steps. As of PostGIS 2.0.6, out-of-db rasters and all raster drivers are disabled by default. Module: Forestry Application. If you are interested in learning. I know, but we had to make a decision to support older versions vs. So for each new version of PostGIS we support only 2 or 3 PostgreSQL versions. As of this writing Post. GIS 2. 2. 0 is the latest stable release. Noteable features in this release: now packages along new 3. D measurement functions, 3. D spatial index support and 3. D surface area typesseamless raster/vector analysis support including an easy to use command line raster database loader that supports various types and can load whole folders of raster files with one commandline statement, and really jazzy image export functions to output both raster and geometries as PNG/TIFF and other raster formats. SQL/MM topology support: now improved using native C functions. Windows Application Stack builder and some other desktop distros, now includes batch file uploading as well as exporting. We will also be using. Massachusetts/Boston data for these examples. For desktop users, the Enterprise. The following instructions describe how to install PostgreSQL and PostGIS on Linux and Windows, create the appropriate spatial databases, and tune database parameters. Section 3: Creating a Spatial Database This is the magical moment Node.js and Express get to work generating a project template for you. You should see a series of lines that begin with DB one- click installer exists as well for Mac/OSX and Linux desktops, so you should be able to follow along without too much fuss. Installing Postgre. SQL with Post. GIS Functionality. We will not go into too much detail here since the. Below are the. basic steps. Download the install for your specific platform. Postgre. SQL Binary Download ( http: //www. As of. this writing the latest version is Postgre. SQL 9. 5. 0beta. 1 and we will be assuming Post. GIS 2. 2. The minimum support Postgre. SQL for Post. GIS 2. Postgre. SQL 9. 1 (for windows we only build installers for 9. KNN true distance indexable operators (prior versions are bounding box distance only) you need Postgre. SQL 9. 5. So use 9. Launch exe to install Postgre. SQLOnce Postgre. SQL is installed, launch Application Stack Builder from (Start- > Programs- > Postgre. SQL 9. 5- > Applciation Stackbuilder and pick the version of Postgre. SQL you want to install Post. GIS on and the version of Post. GIS to install. NOTE: Post. GIS 2. 1, 2. 2, 1. The dumper,loader commandline and GUI tools in Postgre. SQL bin folder will get overwritten by the last Post. GIS you installed so be careful. Generally speaking Post. GIS 2. 2. 0 should work just fine everywhere you were using Post. GIS 2. 0- 2. 1 before, but you may need install the legacy. GUC raster features Post. GIS GDAL Enabled Raster Drivers GUC, that can either be set using ALTER SYSTEM (for 9. ALTER DATABASE for specific databases.- - Enable Out of database rasters. In 2. 0. 6, 2. 1. If you need them, say yes to this prompt. Enable Out of Database rasters GUCFor those of you who want to try experimental builds - - e. We have experimental Windows builds made weekly or as frequently as anything interesting happens in the Post. GIS code base. Your psql steps would look something like this: To install a bunch of extensions, just open up the pg. Admin SQL Query window (which we'll cover shortly) or psql and run this including only the extensions you want. If you are a newbie or not sure what extensions you want, it's best just to use that. On windows Pg. Admin III is under. Start- > Programs- > Postgre. SQL 9. 5- > Pg. Admin III Login with the super user usually postgres and the. If you forgot it, then go into. Set the line host all all 1. If you are on a newer windows (say 2. Windows 7), you may see an additional option host all all : :1/1. The : :1/1. 28 is usually the controlling one and is what localhost resolves to in IPV6 so you'll want to set this one. This will allow any person logging locally to the computer that. Postgre. SQL is installed on to access all databases without a password. Note you can. add additional lines to this file or remove lines to allow or block. The lines highest in the file take precedence. This feature is only available if you have installed the adminpack. C: \Program Files\Postgre. SQL\9. x\share\contrib) (Admin Pack) in the postgres database . Call. it gisdb or whatever you want. It's generally a good idea to create a user too that. UPDATE: - The remaining steps in this section are not needed if you created a spatial database using the Create spatial database checkbox for your new database. Expand your database and you should see an extensions section , right- mouse click on that and select the New Extension option. Note the many options highlighted in yellow - - ain't that a beaut. The ones highlighted in yellow are the ones packaged in the Post. GIS 2. 2. 0 windows bundle. Using Pg. Admin will list all extensions available on your Postgre. SQL server even if your Postgre. SQL server is not on Windows. So you might see much less than we have highlighted if your distribution doesn't offer these or you didn't do the binary installation for them on the server. Also note the Definition tab, which allows you to install postgis in the non- default schema. Post. GIS 2. 3. 0 when that comes out by changing the version number from drop down or to upgrade to Post. GIS 2. 2. 0 from an earlier version. If Post. GIS Bundle install, you should see the Post. GIS Shapefile and DBF loader in the plugins menu. C: \Program Files\Postgre. SQL\9. 5\bin) and click the .. So to do some neat stuff, we need to get some data to. Get the Data. Download data from the Mass. GIS site. For this simple exercise just download Towns. Extract the files into some folder. We will only be using the . A . prj is often included with ESRI shape files and. We'll need to match this. SRID (the id field of a spatial ref record. Open up the . prj file in a text editor. You'll see. something like NAD. This will bring up about 1. Note the srid of the closest match. In this case. its 2. NOTE: srid is not just a Post. GIS term. Most of the common. So 2. 69. 86. always maps to NAD8. Most if not all Mass. GIS data is in this particular projection. Loading the Data. The easiest data to load into Post. GIS is ESRI shape. Post. GIS comes packaged with a nice command line tool called. ESRI shape files into Post. GIS specific SQL. Post. GIS database. This file is located in the Postgre. SQL bin folder. which default location in Windows is Program. Files/Post. Gre. SQL/9. Make a Post. GIS mini toolkit. Since these files are so embedded, it is a bit. To create yourself a self- contained toolkit. Cd to the folder you extracted the towns data Run the following command: c: \pgutils\shp. BOUNDARY. Also you may get. For the above I used the default superuser. Alternatively you can use the gui to load the data and when you do, your screen will look something like this. In this case we replaced the default table name boundary. This particular dataset is only polygons. There is also a downside to indexes and. Indexes slow down the updating of indexed fields. Indexes take up space. You can think of an index as. Given the above, it is often times tricky to have a. The reason for this is. A gist basically. For large complex. The most common queries we will be doing on this query. So we will create 2. NOTE: The loader has an option to create the spatial index which we took. CREATE INDEX idx. Verify. that you have a towns database now. An OL3 map with Node. Post. GIS – denelius. This is the second post in my Node. In this post I decided to show some love to Open. Layers 3 and Post. GIS, looking at the Node. Node. js Leaflet Mongo. DB post. Once you have the Postgre. SQL/Post. GIS database hooked up you are in good shape and, for the most part there is not too much difference between the approaches used for Mongo. DB or Postgre. SQL. The main item I needed to adjust was my way of thinking about the Java. Script content and how to structure this to best respond to the Node. The idea behind this simple introduction to Node. Node. js is a great platform and can accommodate many different combinations – so, mix up the stack, use your favorite database – or try something new. As mentioned in my other Node. I would love to hear from you. Here is what I would like to achieve from my Node. OL3 Post. GIS application: Build something similar to the Mapbox Toggling layers example Add point line and polygon layers to an Open. Layers 3 map. Store layers as Geo. JSON in Post. GISUse the Node. JSON and Geo. JSONUse the Jade template to build HTML based on layers. In the example I will only have three layers but the design is intended to be scalable and should be able to accommodate more content without the need to build custom HTML. Installation. If you use Windows or OS X you can get the latest version of Node. Node. js website it should be a pretty straight forward install and comes with the Node Package Manager, NPM which is really useful for installing a wide range of packages. You will be using NPM a lot but don’t worry it’s quite simple to use. For Debian based distributions like Ubuntu, Node. On Ubuntu 1. 4. 0. Node. js is nodejs instead of node, on Debian 7 nodejs is not available. The global installation of Node. Packages have to be run as root, so must be run with sudo. Creating a project. We are now ready to crate a project. If you are not already there, cd into the directory you made and think of a name for your new project, I am going with pg. It appears to only applies to Trusty (1. This is the magical moment Node. Express get to work generating a project template for you. You should see a series of lines that begin with . Take a look at the contents of your parent directory, you will notice there is now a directory with the name of your project. Take a look inside your project folder, you should see the following: app. HTML output is constructed. If you take a look in your views directory you will see a few files with a . HTML. To learn more about the Jade template engine take a look at jade- lang. Jade is a little weird at first but if you know some HTML you should be up and running in no time – the key to Jade is indentation. Add Dependencies. Open the package. JSON file with a short description of the app and a list of the dependencies. Since we will be working with Postgre. SQL/Post. GIS we need to add two dependencies. In your package. json file type in the pg and postgeo dependencies seen below – don’t forget the trailing comma on all dependency lines apart from the last. When working with JSON or Geo. JSON there are some useful syntax checkers like http: //jsonlint. JSON syntax, these are useful resources. Another handy JSON resource is the command line tool. The asterisks in the lines we have added instruct NPM to get the latest version of that dependency. To install the dependencies we have added we need to tell NPM to review our package. To do this, execute the following command from inside your project folder. The cogs will start turning and in a few seconds your new dependencies should be officially hooked up. At this stage you can run your application in the browser – execute the following line then navigate to http: //localhost: 3. If you are using a server, adjust local host to reflect your remote IP. The index. js file receives a request from the URL http: //localhost: 3. This is the text that displays in the browser, but lets see how that’s done by looking at the views/index. Welcome to #. The first line imports anything in the layout. The block content line is telling Jade where the content from the layout file needs to go. Next the title variable passed from routes/index. If you like, make some changes to the routes/index. Up till now we have pretty much covered what you are likely to find in initial stages of most Node. OL3, Postgre. SQL mapping application. Postgre. SQL/Post. GISI am not going to cover the details of the Postgre. SQL and Post. GIS install so lets jump directly to adding the data. Create a table to store your spatial data, I am going to call mine . This table will store our point line and polygon layers. For this tutorial the table will have only three fields: id, name and geometry. I have used the same Manhattan point line and polygon sample layers I did in my previous post and have provided the insert statements below to save you some time. This router item does not handle the request for. Next comes our query, we want to return all the layer names from the geo. The final section should look familiar to you from what we went over earlier with the index. We are declaring that we wish to use a map. The next few lines setup the variables we will be sending into the map. Postgre. SQL query result containing our list of layers, a title, which was . Of course we could get the last three variables from Postgre. SQL if we wanted to. We can setup another router item that makes our layer list available to us – wait haven’t we just done this? Yes, if you recall, in the router item above we made a list of layers and some other variables available to our map. Java. Script – This router item will allow us to get immediate access to our layer list using http: //localhost: 3. Very much the same as the handler above except we are not sending our variables to the map. This handler is very similar to the handler above except we want to base the response on an argument we append to the end of the URL which will be our layer name which happens to be the geometry type too. This handler will return the Geo. JSON associated with the layer name. Before I go on, a slight detour – the SQL in this handler requires Postgre. SQL 9. 2 or above and makes use of the built in JSON functions available with this release to compile the Geo. JSON with properties, in our case just the name and id. I will use the properties to display the layer name when a feature is clicked on in the map – this really has nothing to do with Node. Java. Script but I wanted to demonstrate using Node. If your version of Postgre. SQL is less than 9. ST. The following link is a great resource and provides a lot more detail on the format and alternative options. We use the names parameter . Hopefully this is starting to make sense. Lets create our map. Postgre. SQL data. Show me the map. If you are still with me at this point – well done, lets press on and create a map. Here’s where we will get our hands dirty with some Jade templating and build our map content. The views/map. jade file is going to have a similar structure to the the Mapbox Toggling layers example with the exception of the Jade Template iteration and calls to the handler URLs to return our JSON and Geo. JSON data we will also be using Openlayers. Leaflet. We could put everything in one file like the example but let’s rather get our style sheet and Java. Script references setup in the layout. In the views/layout. I have setup the Java. Script and style sheet references for our application. There is not much point in doing this for our example as we only have a one page application but you might use the layout. Let’s edit our views/map. I will try to break down the content into logical parts, the first is the HTML content. If your indentation is not correct, depending on the location of the indentation you might receive the following error: unexpected token “indent”, or simply return a blank screen. The first two lines are where the file will inherit the content from the layout. Next we add an HTML map div element – so the Jade Template Engine translates #map to < div id=’map’> < /div>. We then add HTML div elements for legend title and legend. Notice the line beginning . The full source code is available on Git. Hub. In the second part of our views/map. Open. Layers. 3 content. This is pretty straight forward, we define an osm variable as our base map layer, the map variable and the map arguments. Notice in the view section we have added lat and lng arguments, these are being passed in from the routes/index. A nice feature about the Node. HTML and Geo. JSON content, you are unlikely to run into the situation where you have hard coded an HTML checkbox with no matching spatial data. In the add. Layer() function we check an array called add. Layer. cache, if the layer has already been added we simply return the layer to the request made from the toggle. If the layer is not already in the add. Layer. cache array we request the layer using the handle setup to respond to http: //localhost: 3. Layer. cache array and the map. I have set up an add. Style() function which we will get to shortly but this simply assigns a style to each layer. It is important to note that Open. Layers handles the display of layers on a first come first server basis – so if the first layer you add (request this layer for the first time) is a point layer, you run the risk of subsequent layers being displayed on top of the points layer and possibly covering it. There are many ways to handle this conflict but I’m not going to cover these in this tutorial, the important thing to note is that using the add. Layer() function below, the very first layer you display will be the first layer added to the map and be displayed at the bottom of the layer stack, subsequent requests for the layer will not alter its position they will simply toggle visibility – you can try this out shortly. You might wish to build a function that adds your layers to the map in a logical order then a separate function to handle their visibility.
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We will be happy if you visit our Facebook community https: //www. PSD is set up in 1. Note: Free New Year’s Eve Flyer Template is a guest submission by Dom Design. New Year’s Eve is probably the biggest single party date on the calendar. Each year, NYE is celebrated around the entire globe and almost. Looking for a vibrant PSD pamphlet for your end of the year event? Search no more, this Free New Year Party Flyer Template is the perfect solution for you. With 2 text styles and different color variations, it’s perfect for. New Years Eve Flyer Template. The Free New Years Eve Flyer Template was designed to promote your next New Year and New Years Eve party and club celebration. This print ready premium flyer template includes a 300 dpi print. Explore the best Free New Year Flyer templates for any kind. Save money and time while using our handpicked and collected free new year PSD flyer templates for. Download the Free Free New Year Eve Party Flyer Template. 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This energy source differs from that of mid- latitude cyclonic storms, such as nor'easters and European windstorms, which are fueled primarily by horizontal temperature contrasts. The strong rotating winds of a tropical cyclone are a result of the conservation of angular momentum imparted by the Earth's rotation as air flows inwards toward the axis of rotation. As a result, they rarely form within 5. Cyclone refers to their cyclonic nature, with wind blowing counterclockwise in the Northern Hemisphere and clockwise in the Southern Hemisphere. The opposite direction of circulation is due to the Coriolis effect. In addition to strong winds and rain, tropical cyclones are capable of generating high waves, damaging storm surge, and tornadoes. They typically weaken rapidly over land where they are cut off from their primary energy source. For this reason, coastal regions are particularly vulnerable to damage from a tropical cyclone as compared to inland regions. This bibliography lists both monographs and journal or magazine articles about comic books, comic strips and animation. Some of these materials have NOT YET been verified for accuracy or content; please contact the authors if. Using other people’s research or ideas without giving them due credit is plagiarism. En physique des particules comme en chimie quantique, la configuration Serafin, “Tromba moderna: a digitally augmented medieval instrument,” in Proceedings of the international conference on new interfaces for musical. Furk.net is your personal secure storage that fetches media files and lets you stream them immediately You can use it to stream video or listen to your music from PC, smartphone, HTPC or even a game console (XBOX, PS3). 9/11’s Guided Missiles. 9/11’s GUIDED MISSILES By Brother Nathanael Kapner, Copyright 2008-2011. Articles May Be Reproduced Only With Authorship of Br Nathanael Kapner & Link To Real Jew News. 8.1 illustrates some key things about the global distribution of tropical cyclones: Tropical cyclones do not form very close to the equator and do not ever cross the equator; The western North Pacific is the most active. Heavy rains, however, can cause significant flooding inland, and storm surges can produce extensive coastal flooding up to 4. Though their effects on human populations are often devastating, tropical cyclones can relieve drought conditions. They also carry heat energy away from the tropics and transport it toward temperatelatitudes, which may play an important role in modulating regional and global climate. Physical structure. Tropical cyclones are areas of relatively low pressure in the troposphere, with the largest pressure perturbations occurring at low altitudes near the surface. On Earth, the pressures recorded at the centers of tropical cyclones are among the lowest ever observed at sea level. At the outer edge of the storm, air may be nearly calm; however, due to the Earth's rotation, the air has non- zero absolute angular momentum. As air flows radially inward, it begins to rotate cyclonically (counter- clockwise in the Northern Hemisphere, and clockwise in the Southern Hemisphere) in order to conserve angular momentum. At an inner radius, air begins to ascend to the top of the troposphere. This radius is typically coincident with the inner radius of the eyewall, and has the strongest near- surface winds of the storm; consequently, it is known as the radius of maximum winds. However, the wind field often exhibits additional spatial and temporal variability due to the effects of localized processes, such as thunderstorm activity and horizontal flow instabilities. In the vertical direction, winds are strongest near the surface and decay with height within the troposphere. For a sufficiently strong storm, air may sink over a layer deep enough to suppress cloud formation, thereby creating a clear . Weather in the eye is normally calm and free of clouds, although the sea may be extremely violent. The eyewall typically expands outward with height, resembling an arena football stadium; this phenomenon is sometimes referred to as the stadium effect. The heaviest wind damage occurs where a tropical cyclone's eyewall passes over land. Outer rainbands can organize into an outer ring of thunderstorms that slowly moves inward, which is believed to rob the primary eyewall of moisture and angular momentum. When the primary eyewall weakens, the tropical cyclone weakens temporarily. The outer eyewall eventually replaces the primary one at the end of the cycle, at which time the storm may return to its original intensity. This speed is taken as either a 1- minute or a 1. The choice of averaging period, as well as the naming convention for classifying storms, differs across forecast centers and ocean basins. On occasion, tropical cyclones may undergo a process known as rapid deepening, a period in which the minimum sea- level pressure of a tropical cyclone decreases by 4. Water temperatures must be extremely warm (near or above 3. Wind shear must be low; when wind shear is high, the convection and circulation in the cyclone will be disrupted. Usually, an anticyclone in the upper layers of the troposphere above the storm must be present as well. The most common metrics include the radius of maximum wind, the radius of 3. They are largest on average in the northwest Pacific Ocean basin and smallest in the northeastern Pacific Ocean basin. All else equal, a larger storm will impact a larger area for a longer period of time. Additionally, a larger near- surface wind field can generate higher storm surge due to the combination of longer wind fetch, longer duration, and enhanced wave setup. The primary circulation is the rotational part of the flow; it is purely circular. The secondary circulation is the overturning (in- up- out- down) part of the flow; it is in the radial and vertical directions. The primary circulation is larger in magnitude, dominating the surface wind field, and is responsible for the majority of the damage a storm causes, while the secondary circulation is slower but governs the energetics of the storm. Secondary circulation: a Carnot heat engine. A tropical cyclone's primary energy source is heat from the evaporation of water from the ocean surface, which ultimately recondenses into clouds and rain when the warm moist air rises and cools to saturation. The energetics of the system may be idealized as an atmospheric Carnot heat engine. Second, the warmed air rises and cools within the eyewall while conserving total heat content (latent heat is simply converted to sensible heat during condensation). Third, air outflows and loses heat via infrared radiation to space at the temperature of the cold tropopause. Finally, air subsides and warms at the outer edge of the storm while conserving total heat content. The first and third legs are nearly isothermal, while the second and fourth legs are nearly isentropic. This in- up- out- down overturning flow is known as the secondary circulation. The Carnot perspective provides an upper bound on the maximum wind speed that a storm can attain. Scientists estimate that a tropical cyclone releases heat energy at the rate of 5. J) per day. This rate of energy release is equivalent to 7. Absolute angular momentum on a rotating planet M. The first term on the right hand side is the component of planetary angular momentum that projects onto the local vertical (i. The second term on the right hand side is the relative angular momentum of the circulation itself with respect to the axis of rotation. Because the planetary angular momentum term vanishes at the equator (where f=0. Similarly, as rapidly rotating air flows radially outward near the tropopause, its cyclonic rotation decreases and ultimately changes sign at large enough radius, resulting in an upper- level anti- cyclone. The result is a vertical structure characterized by a strong cyclone at low levels and a strong anti- cyclone near the tropopause; from thermal wind balance, this corresponds to a system that is warmer at its center than in the surrounding environment at all altitudes (i. From hydrostatic balance, the warm core translates to lower pressure at the center at all altitudes, with the maximum pressure drop located at the surface. Thus, the sea surface lower boundary acts as both a source (evaporation) and sink (friction) of energy for the system. This fact leads to the existence of a theoretical upper bound on the strongest wind speed that a tropical cyclone can attain. Because evaporation increases linearly with wind speed (just as climbing out of a pool feels much colder on a windy day), there is a positive feedback on energy input into the system known as the Wind- Induced Surface Heat Exchange (WISHE) feedback. This upper bound is called the . At equilibrium, the rate of net energy production in the system must equal the rate of energy loss due to frictional dissipation at the surface, i. Win=Wout. Given that a tropical cyclone may be idealized as a Carnot heat engine, the Carnot heat engine efficiency is given by. The first component corresponds to sensible heat and the second to latent heat. There are two sources of heat input. The dominant source is the input of heat at the surface, primarily due to evaporation. The bulk aerodynamic formula for the rate of heat input per unit area at the surface, Qin: k. The second source is the internal sensible heat generated from frictional dissipation (equal to Wout. This derivation assumes that total energy input and loss within the system can be approximated by their values at the radius of maximum wind. The inclusion of Qin: friction. Mathematically, this has the effect of replacing Ts. The ratio of the surface exchange coefficients, Ck/Cd. However, observations suggest that the drag coefficient Cd. However, this quantity varies significantly across space and time, particularly within the seasonal cycle, spanning a range of 0. These processes are modulated by factors including the sea surface temperature (and underlying ocean dynamics), background near- surface wind speed, and the vertical structure of atmospheric radiative heating. On shorter time- scales, variability in the maximum potential intensity is commonly linked to sea surface temperature perturbations from the tropical mean, as regions with relatively warm water have thermodynamic states much more capable of sustaining a tropical cyclone than regions with relatively cold water. This cooling is primarily caused by wind- driven mixing of cold water from deeper in the ocean with the warm surface waters. Furk. net : : Furk. You can use it to stream video or listen to your music from PC, smartphone, HTPC or even a game console (XBOX, PS3). Humor eroteco girl from hex nude pics xxxgerls ringtones free download shekala movie shalane nude tugjobs brooke hogan oral surgery free tutorials panty hose. Dave Matthews Busted Stuff Rapidshare MoviesGirls SeX Porn Videos,3gp mp4 chudai fuck,girls animals dog horse sex,indian sex videos xxx, Desi Sex Video xxx, full free Sex download xxx, Tamil Sex xxx, Punjabi. 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