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0. Quick start

This getting started manual is intended to help you, the end-user of our system, to get up and running as quickly as possible. In other words - how to mount the spectrometer on your measurement platform, what power do you need to supply and how do you actually do a measurement. 

Before starting

As a start, we would like you to take note of the fact that you have a delicate instrument in your hands. Our gamma-ray spectrometers contain a (relatively) fragile scintillation crystal at their core. Both this crystal and the electronics in the device should always be handled with care. Dropping, hitting or significant impact on the detector may result in the breaking of this crystal. Medusa has taken care to optimise the weight of the spectrometer systems while implementing a shock-absorbing layer that keeps the crystal stable. However improper use could still lead to the breaking of an element in the system. Therefore it is crucial that handling the detector is done with care and proper preparation have been taken before working with this system.

UAV warning: You can use the small detectors as drone detectors. However, it is advised to confirm that the UAV platform is suitable for this weight by testing with a dummy weight. Depending on the type of UAV you are using the weight of this detector may be at the limit of what the UAV can handle. We have had many successful measurements with our detectors, however, we always tested the platform with a dummy before mounting the real detector. There are reports of drones that crashed when carrying their maximum load. This can have various causes among which the (weak) stiffness of the drones' frame (causing the IMU's to overcompensate) or magnetic interference (such as from little magnets incorporated in GPS antennas). Always take proper preparations when using the medusa spectrometer under a drone.

If you are in doubt about the mounting, handling or other handling issues, please contact Medusa. Our support section is always happy to help you out and give advice on the use of spectrometer systems. 

Mounting the detector

The end caps of the detector are equipped with mounting points. These mounting points are sufficient to support the weight of the detector if fastened properly. The dimensions and mounting points differ between the different systems. Our technical section lists all the dimensions of the various Medusa detector systems. The MS-2000 detector can be mounted by using the MSB-20x mounting brackets, whereas the smaller systems usually have an application-specific mounting.

Gamma-ray detectors in general are sensitive to radiation from all directions. Therefore there is no "preferred" mounting direction - a sensor can as well be mounted parallel to the direction of movement as perpendicular. Gamma-radiation is, attenuated by materials placed between the detector and the source of the radiation. Therefore the detector should be mounted in such a way that there is the least possible obstruction between the source (the soil) and the sensor. 

More information and examples of mounting the spectrometer on a platform can be found on the Theory page.

Powering the device

Medusa supplies the systems with a variety of cables that are specifically tailored for each application. Information on the specifications of all available cables can be found in the Cables and connectors section. The table below lists which cables come standard with each detector type. Always use medusa certified cables on the system, these cables are specifically designed to be used with our spectrometer systems.

DetectorCableInput voltage rangeConnectors
MS-4000/MS-2000MDC-40x cable9-18 or 9-35VEthernet and flying leads for power
MS-1000-/MS-700/MS-350MDC-50x cable3-35VUSB for power

Spectrometers have a nominal power usage of 3W and a peak power usage of 6W

Configuring the measurement

When the system is powered it will automatically start the spectrometer. All data is logged and automatically saved to the project which was active before.

System startup

The detector has four LEDs embedded in the top cap. The orientation of the LEDs relative to the connector depends on the detector series. Some detectors are mounted with the fastening wings down such as the MS-2000, and some are mounted with the fastening wings up such as the MS-350 or the MS-1000. The position described below is with the connector oriented below the LEDs. The table below lists the colour coding for the mDOS V3.0 systems. For the older systems, such as the mDOS V2.x system, check out the mDOS manual page.

PWRGreenPower is ok and in the right input range

RedPower is too low or high

PurplePower line has large fluctuations, please check the power supply
ETHGreenEthernet cable is connected
SCNGreenThis LED will blink if a spectrum is collected.
AUXGreenThis LED will blink if auxiliary sensor data is received (GPS, PTH, etc.)

If both the SCN and AUX LEDs blink in red this means that the internal storage is almost full. The default action when all storage space is taken is to overwrite the oldest data! At a typical data logging rate of 1Hz and storage capability of 4GB this means that you can store around 20 days of data.

Accessing the mDOS interface through the built-in website

When an ethernet cable is connected

The detector can be accessed either by directly connecting the detector to a computer or by connecting it to a network using a router. The detector will check if it receives an IP address from a router. If no IP address is provided by your router, e.g. when the detector is connected directly to a computer, the detector will initialize with its default IP address. If there is a router in the network that provides the detector with an IP address, this address has to be determined by checking the router settings. Most routers have the option to set a unique IP address based on the connected device. Detectors in the network can also be found by using the Medusa detector finder tool which can be downloaded from the Medusa Software section under software downloads and updates.

Additionally, if your network supports multicast DNS (mDNS), the detector can be accessed by using the detector hostname.

To access the built-in website, navigate to the IP address.

Standard IP-address192.168.2.150
Hostname<Model>-<Series number>.localMS-2000-0054.local

When the detector is connected directly to the computer by using the ethernet cable the website of your detector can be accessed by navigating to the address: (mDOS V2) or (mDOS V3)

Through WIFI

One of the functions of the (internal or external) PUCK is to provide a WIFI access point. By connecting your computer, tablet or phone to the PUCKs network, it is possible to access the webserver through its standard IP-address as described in the section above.

SettingDescription Internal puck (PUCK-300)
PUCK SSIDMS<version>-<serial>
PUCK PW@Radiometrics123
When you encounter difficulties accessing the spectrometer by using a phone or a tablet it might be necessary to turn off your data connection.

The landing page of the web-interface

Selecting or downloading a project

When connected to the interface it is possible to inspect the measurement through the available pages. The dashboard gives basic information on the current measurement and selected project.

Project management (projects page)
The projects on the system are automatically 'chunked' in sub-projects with a maximum size of 300MB. When the project exceeds this size the project name is appended with an underscore and three incrementing digits.

New projects can be created or old projects can be selected or deleted. Selecting means that data will be logged to this project. Deletion of the project is permanent and cannot be undone.

When the option "overwrite oldest files when full" is selected measurement system will overwrite the oldest files. This does not mean that a whole project is deleted at once. However, the project size will gradually go down when new data is written to the device. When a project folder is empty it will automatically be deleted.

Starting a measurement

After selecting a project the measurement is started. Because the spectrometer is designed to be "always on", the data is stored automatically on the device. Once a project has been created all data is subsequently logged to this project. The Medusa Gamman software provides the tools to make selections on the project. This can be done either by timestamp or by geometric position. 

By checking the LEDs during the measurement it can be confirmed that the measurement is still running. The SCN LED will blink for every stored spectrum and the AUX LED will blink for every auxiliary data entry.

Retrieving the data

After the measurement is done or even during measurement, you can download the recorded data from the device. This has to be done through the web interface by navigating to the projects page. A project can be downloaded by first clicking on the project name and then using the download button.  When downloading a project it will be compressed to a .zip file before it is being sent to the user. A progress bar shows the progress of the compression. Once this is finished a pop-up will appear with the project file. You can now save the data to your PC or other devices. When a phone or tablet is used the user should remember that all data needs to be transferred to a (Windows) computer where the data can be analysed using GAMMAN or other software.

Turning the device off

Powering down or restarting the system can either be done by pressing the button on the power off-page of the webserver or by removing the power. Doing it through the webserver is advised when settings have been changed because it ensures proper saving of the settings.

When pressing the shutdown button it the webserver the system will turn itself off. If all four LEDs are ON the system is fully powered down and power can be removed.

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