Montana Aurora Detector Network


Operated by the Optical Remote Sensor Laboratory, Dr. Joseph Shaw,
Montana State University, Electrical and Computer Engineering Department

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Live Aurora Status

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Current Aurora Status Help

This page displays the current status of the network represented by the icons on the map. Each of these icons can be clicked to display more information about the current status.

College Icons

The numbers in the icons for each college represent the current brightness level of the aurora at that location. For more information about these brightness levels, use the "About Our Detectors" link in the navigation bar on the left side of the page.

Map Display Settings

Shows full college names
This button toggles the length of the colleges' names between full and abbreviated. By default the full names are displayed.
Shows the auroral oval
This button toggles the display of the auroral oval. This is enabled by default. Please note that even when this is displayed, it may not be visible from your current map view. For more information about the auroral oval, use the link in the navigation bar.

Map View Shortcuts

This button adjusts the map so that the entire Montana Aurora Detector Network is in view.

When the auroral oval is displayed this button adjusts the map so that the northern auroral oval is in view.

The buttons in this dialog are for demonstration only. The states of these buttons will not effect the content on the map.

Information About Our Detectors

What causes the Aurora?

Excited Particles in our Atmosphere cause the Aurora to become visible. Energy from the sun strikes our atmosphere, causing causes abundant Nitrogen and Oxygen to become excited, meaning that their electrons jump up to a higher energy state. These electrons eventually fall back to their ground state and they release the stored energy as light. This is the light that we see and recognize as the visible Aurora.

How Do We Detect the Aurora?

The Light is Released from the particles in our atmosphere at a specific wavelength. In the case of Oxygen emissions this light is approximately 557.7nm. This light is fed through a lens into our detector, and we measure its intensity. We then also measure the total light from the sky, and compare the relative strengths. If the Aurora Green is more intense than the general light from the sky, we know that an Aurora is likely occuring!

Pictured is the aurora detector located at MSU Bozeman on the roof of Cobleigh Hall. Skylight passes through a 10-nm interference filter and is focused by a lens onto a photomultiplier tube (PMT) detector whose output is sampled with a microcontroller and transmitted via Ethernet to a server at MSU. Once the data arrives, a data processing algorithm determines whether an alarm signal should be sent.

Information About The Auroral Oval

The Auroral Oval is generated with information gathered by the National Oceanic and Atmospheric Administration (NOAA). Data is generated through measurements of solar winds, which indicate the likelyhood of an Auroral storm occuring at the hemispheres. Though the Aurora is primarily in high-latitude environments, high intensity solar storms can cause the Auroral Oval to extend down into Montana. The image below was taken by Dr. Joseph Shaw in Bozeman on May 3rd, 2010.

The Auroral Oval indicates where the Aurora is likely visible. Darker regions indicate higher higher probability of seeing the Aurora, while lighter and clear regions indicate little to no chance of seeing the Aurora. Data used to generate the Auroral Oval is updated every 5 minutes, so be sure to refresh your browser to see the most recent Auroral Oval.

The Optical Remote Sensor Laboratory