The Doppler CLI requires an API key for authentication. Access can be granted via the login flow for local development or using a Service Token for production environments as it restricts access to a specific config within a Project.

The Doppler CLI supports multiple workplaces by allowing you to scope your login to a specific directory. Any applications inside your chosen directory (and its sub-directories) will automatically use the correct API key.

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When using the --command flag, the Doppler CLI will determine what shell to use based on the SHELL environment variable. The CLI currently supports sh, bash, zsh, dash, fish, ksh, tcsh, and csh. If you are using an alternative shell, the CLI will fall back to sh. You can manually specify your preferred shell.

The below is a list of the top-level commands available in the Doppler CLI. To get additional information about any given command, use the built-in CLI help by passing in the -h flag like this: doppler run -h.

These are some commonly used commands that you'll likely find yourself using pretty regularly. There are more advanced ways to use the CLI, so we recommend exploring the available commands, but this should help jump start your usage!

You can perform an operation that assigns a specific directory (and its subdirectories) to a particular config. This allows you to run commands without specifying the project (-p) and config (-c) flags.

NEXRAD (Next Generation Radar) obtains weather information (precipitation and wind) based upon returned energy. The radar emits a burst of energy (green in the animated image). If the energy strikes an object (rain drop, snowflake, hail, bug, bird, etc), the energy is scattered in all directions (blue). Note: it's a small fraction of the emitted energy that is scattered directly back toward the radar.

This reflected signal is then received by the radar during its listening period. Computers analyze the strength of the returned pulse, time it took to travel to the object and back, and phase, or doppler shift of the pulse. This process of emitting a signal, listening for any returned signal, then emitting the next signal, takes place very fast, up to around 1300 times each second!

NEXRAD spends the vast amount of time "listening" for returning signals it sent. When the time of all the pulses each hour are totaled (the time the radar is actually transmitting), the radar is "on" for about 7 seconds each hour. The remaining 59 minutes and 53 seconds are spent listening for any returned signals.

The ability to detect the "shift in the phase" of the pulse of energy makes NEXRAD a Doppler radar. The phase of the returning signal typically changes based upon the motion of the raindrops (or bugs, dust, etc.). This Doppler effect was named after the Austrian physicist, Christian Doppler, who discovered it. You have most likely experienced the "Doppler effect" around trains.

As a train passes your location, you may have noticed the pitch in the train's whistle changing from high to low. As the train approaches, the sound waves that make up the whistle are compressed making the pitch higher than if the train was stationary. Likewise, as the train moves away from you, the sound waves are stretched, lowering the pitch of the whistle. The faster the train moves, the greater the change in the whistle's pitch as it passes your location.

The same effect takes place in the atmosphere as a pulse of energy from NEXRAD strikes an object and is reflected back toward the radar. The radar's computers measure the phase change of the reflected pulse of energy which then convert that change to a velocity of the object, either toward or from the radar. Information on the movement of objects either toward or away from the radar can be used to estimate the speed of the wind. This ability to "see" the wind is what enables the National Weather Service to detect the formation of tornados which, in turn, allows us to issue tornado warnings with more advanced notice.

In the image above, the grey line is the transmitted signal. You can see how

the returned energy changes its wavelength characteristics when it hits

a target moving away or toward the radar (red and green line, respectively)

Reflectivity data shows us the strength of the energy that is returned to the radar after it bounces off precipitation targets. Other non-precipitation targets will return energy, but for now, we will only deal with the precipitation. In general, the stronger the returned energy, the heavier the precipitation. Learn more about Reflectivity here.

Velocity data is derived from the phase, or doppler shift of the returned energy. The radar's computers will calculate the shift and determine whether the precipitation is moving toward or away from the radar, and how fast, then apply a corresponding color to those directions and speeds. Red is typically a target moving away from the radar, while green is applied to targets moving toward the radar. The intensity of these colors determines its estimated speed. Learn more about Velocity here.

In the image above, you can see the velocity data that is associated with a strong storm depicted in the reflectivity data. This is a great example of what a tornado looks like in the velocity display. Click on the image for better detail. The radar is located to the southeast, or to the bottom right of the computer screen. Note the bright red, or strong outbound velocities right next to the bright green, or inbound velocities. This indicates a strongly rotating column of air. When coupled with a reflectivity pattern that exhibits a hook signature, as in this case, there is often a tornado occurring or about to occur. 

If there is a "target" out there and it reflects radar energy back to the radar, the radar will display it as if it was precipitation. The radar does have some logic built in to help it discriminate between precipitation and non-precipitation targets. But, sometimes we see curious things on our radar display. Here are a few:

Bird Roost Rings. These are most common in the fall around bodies of water that typically have temperatures warmer than the surrounding land at night. It is also the time birds are gathering for the seasonal migration. At night, birds rest/nest in and around the lakes. Just before sunrise, there is often a coordinated lift off and dispersion of the birds out into the surrounding fields for feeding during the day. Click on the image to the left for a quick animation of the bird rings.

Sun Interference. Twice a day, at sunrise and sunset, the radar experiences interference from the electromagnetic energy emitted by the sun. There is a point at sunrise and sunset where the radar dish points directly at the sun and is hit with this energy. This is then displayed as a spike of returned energy on our display. It is brief, typically only occurring during one volume scan. Notice in the image to the left that sunset is slightly south of due west. The date is March 11, 2009. In less than 2 weeks, we will be at the Spring Equinox. The sun will set due west of the radar. 

Smoke Plumes. During dry periods, when there is controlled burning or uncontained wildfires going on, our radar will detect smoke plumes associated with the fires. Many of the big smoke plumes are from prescribed, or controlled burns. These are fires intentionally set by Federal/State/Local officials for land management purposes. Other fires may be on private lands. The two plumes in this example (click on image for an animation) were prescribed burns by the Wisconsin DNR. 

The Doppler Ultrasound Flow Phantom, when used with the Doppler Flow Pump, provides a complete solution for QA testing of doppler ultrasound devices. The two most common tests are sensitivity and velocity accuracy.

As any object moves through the air, the air near the object is disturbed.The disturbances aretransmitted through the air at a distinct speed calledthe speed of sound.Sound is a sensation created in the humanbrain in response to small pressure fluctuations in the air.Sound moves through the air as a series of waves. When the wavespass our ears, a sound is detected. The distance between any twowaves is called the  wavelength  and the time interval between wavespassing is called the  frequency .The wavelength and the frequency are related by the speed of sound; highfrequency implies short wavelength and low frequency implies a long wavelength.The brain associates a certainmusical  pitch  with each frequency; the higher the frequency, thehigher the pitch. Similarly, shorter wavelengths produce higher pitches.The speed of transmission of the sound remains a constant regardless ofthe frequency or the wavelength. The speed of sound only depends on thestate of the air(or gas) not on the characteristics of the generatingsource.

Because the speed of sound depends only on the state of the gas, some interestingphysical phenomena occur when a sound source moves through a uniform gas. Youcan study some of these phenomena by using the interactivesound wavesimulator. As the source moves it continues to generate sound waveswhich move at the speed of sound. Since the source is moving slower thanthe speed of sound, the waves move out away from the source. Upstream (inthe direction of the motion), the waves bunch up and the wavelengthdecreases. Downstream, the waves spread out and the wavelength increases. Thesound that our ear detects will change in pitch as the object passes.This change in pitch is called adoppler effect.There are equations that describe the doppler effect. Asthe moving source approaches our ear, the wavelength is shorter, the frequencyis higher and we hear a higher pitch. If we call the approachingfrequency fa, the speed of sound a,the velocity of the approaching souce u,and the frequency of the sound at the source f, then 152ee80cbc

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