宇宙線観測アプリ[宙豆]そらまめ
Soramame


Consumer Devices with CMOS camera image sensors
as Pocket-Sized Particle Detectors

Soramame: A Cosmic Ray Observation App for iOS and Android

Cosmic rays are important targets of observation that can provide insights into the origins of the universe and high-energy astrophysical phenomena. Traditionally, their detection has required specialized and expensive equipment. Focusing on the characteristics of CMOS image sensors installed in smartphones and tablets, we developed the app “Soramame”, which enables simplified cosmic ray detection using general consumer devices.

When high-energy charged particles from space strike the CMOS sensor, they generate tiny amounts of electrical charge. The Soramame app captures these signals as images and visualizes them in real time. The detected data is also transmitted to a cloud server, allowing users to view events detected by others via a shared web platform.

Because Soramame allows cosmic ray detection without specialized equipment, it is highly suitable for educational use. Since detection relies on rare and spontaneous events, long-term observation is important. We encourage the use of unused smartphones or tablets to enable continuous data collection.

From an educational perspective, the ability to detect and observe invisible cosmic rays with one's own hands deepens understanding of physical phenomena and fosters scientific curiosity. By altering conditions such as altitude, shielding, and time of day, students can collect and compare data, making the app suitable for inquiry-based learning and data-driven science education.

The app also includes a data sharing feature, allowing users to compare observations from different regions. This enables collaborative learning and supports citizen science activities. In the future, we plan to enhance detection accuracy, integrate more closely with educational curricula, and improve data analysis features to further increase the app's educational value.

Soramame is developed by the Hibino Laboratory, Department of Applied Physics, Faculty of Engineering, Kanagawa University. We hope it will serve as a tool that bridges research and education, and that it helps deepen public understanding and interest in science.

Repurposing Unused Smartphones for Scientific Exploration

Globally, there are now over 19 billion internet-connected devices, including tablets, laptops, and smartphones. With new models released nearly every year, many devices are replaced within just a few years. But what happens to these devices once they are no longer in everyday use?

Despite their compact size, these devices are highly advanced computers, equipped with a range of valuable components. One of the most important is the camera sensor—found in nearly all smartphones and tablets. This silicon-based semiconductor, known as a CMOS image sensor, plays a key role in the development of the Soramame cosmic ray detection app.

Why not breathe new life into an old smartphone or tablet by using it for scientific discovery? With Soramame, you can contribute to cosmic ray observation and turn an unused device into a tool for space science exploration.

App Screen

  • Tracks from charged particles are displayed in real time as images.
  • Track candidate locations are shown as rings on the screen.
  • Each ring represents a detection position on the sensor.
  • Uneven ring distribution may indicate noise or edge-related bias.
  • Detected events are uploaded to the cloud server in real time.
  • Rings gradually shrink and disappear over a period of 12 hours.

About Threshold Setting

When the app is launched for the first time, it enters a learning phase to determine the noise level and automatically sets the detection threshold. During this phase, the detection rate may temporarily appear very high.
To ensure accurate calibration, please keep the app running for at least 3 hours after the initial launch.
Once the threshold is established, the ,“Keep the current threshold value”, option will be checked.
After that, you can begin observations in different environments, such as on airplanes or in high-latitude regions.

Interactive Icons

  • 📈: Open the detection graph site
  • Orange UFO: App updates and FAQ

Observation point

Location information is blurred. Leaflet Map


Android

iOS

Harnessing 19 billion CMOS sensors worldwide to pursue global-scale observation of cosmic rays

Among cosmic rays are particles with energies far beyond what Earth-based accelerators can achieve. The highest-energy cosmic rays are thought to carry energies up to ten million times (over seven orders of magnitude) greater than artificial accelerators. How they are accelerated and where they originate remain among the biggest unsolved problems in modern physics.

These ultra–high-energy cosmic rays are extremely rare, making them difficult to observe. Large numbers of sophisticated detectors must be deployed over vast areas, which entails high operating costs. Even so, researchers around the world continue to take on this challenge. Multiple international collaborative projects are underway, installing numerous detectors across sites spanning thousands of square meters to observe particles that rain down from space every day.

We are exploring a more economical way to expand the effective observation area by using smaller detectors such as CMOS sensors. To date, there have been very few attempts to observe air showers with CMOS camera image sensors. We believe CMOS sensors hold new potential for observing the “core region” of air showers—where particle density is especially high and conventional instruments struggle. The compactness and thinness of these sensors, counterintuitively, make them well-suited to measurements in such high-density regions.

It may also be possible to detect very weak signals from charged particles—signals that have previously been treated as noise—using CMOS sensors. This could enable higher-resolution measurements of variations in particle density within air showers.

We are currently working to establish an entirely new method for observing cosmic-ray air showers using CMOS sensors. Through this effort, we aim to get closer to the true nature of cosmic rays.

Updated: September 26, 2025

Contact: Kazuniko Takano (r201970105fg_at_jindai.jp)
*Please replace “at” with “@” in the email address.