# Stargazer Photos Reveal New Insights Into Red Northern Lights

Amateur photography provides critical data on the mechanisms behind rare red auroral displays.

- **Source:** [All Articles | Discover Magazine](https://www.discovermagazine.com/rss/all)
- **Published:** 2026-11-03
- **Topic:** [Business](https://brifing.si/c/business)
- **Original article:** <https://www.discovermagazine.com/aurora-images-taken-by-stargazers-may-help-explain-elusive-red-northern-lights-49893>
- **On Brifing:** https://brifing.si/s/8d0377a8-7e9c-4790-b724-28ce9d16d777

## Rare Auroral Event Analysis

On May 10, 2024, a massive magnetic storm pushed auroras far from polar regions, reaching Göttingen, Germany. Sami Solanki, director of the Max Planck Institute, captured images of this rare display. These photos, originally intended as a hobbyist project, became the primary data source for a new study published in Annales Geophysicae.

## Unprecedented Visual Evidence

Researchers identified unique light rays connecting red auroral glows to green ones below. Philipp Schulz captured these streaks using a Google Pixel 7, while Solanki utilized a tripod-mounted camera. According to lead author Bruce Tsurutani, these continuous rays connecting different atmospheric layers have never been documented in previous scientific literature until this specific event.

## Oxygen Atom Emission Mechanics

Auroral colors originate from oxygen atoms reacting to electron impacts at varying altitudes. Green light typically forms between 50 and 80 miles high, while red light occurs in thinner air between 125 and 500 miles. The red glow persists because lower air density prevents collisions from quenching the light emission process prematurely.

## Challenging Existing Scientific Theories

The unbroken streaks observed in the photos provide evidence against older theories, such as heat flow from space. Since electrons travel along Earth's magnetic field lines, the alignment of these streaks suggests that fast electrons are the primary cause for both colors. This observation simplifies the physical model of the auroral light production.

## Citizen Science Data Collection

The study relies entirely on ground-based photography because few scientific instruments measure these high-altitude phenomena directly. Yasuhito Narita, who coordinated the international team, emphasizes that this is a citizen science report. The researchers are actively requesting more high-quality images from the public to further validate their findings regarding red auroral variations.

## Technical Requirements for Submissions

To contribute useful data, the research team specifies that photographs must be taken with a shutter speed of six seconds or less. This duration ensures that the light streaks remain visible while stars appear as distinct points rather than trails. Such precision is necessary for the team to analyze the structural details of rays.

## Solar Cycle Contextual Factors

The May 10 event was the second strongest magnetic storm recorded since 1958, triggered by intense solar activity. Although the sun is currently moving away from the peak of its 11-year cycle, researchers note that strong eruptions remain possible. This ongoing solar activity provides further opportunities for gathering data on rare atmospheric light displays.

## Future Research Implications

The study suggests that multiple types of red auroras likely exist, as evidenced by earlier photos from the same night showing patches without streaks. By integrating amateur photography into formal research, scientists can bridge gaps left by limited instrumentation. This collaborative approach is essential for understanding complex, high-altitude atmospheric interactions during intense storms.

## Sources covering this story

- https://www.discovermagazine.com/aurora-images-taken-by-stargazers-may-help-explain-elusive-red-northern-lights-49893 — 

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_Summary written by Brifing from the original reporting. Copyright in the original article belongs to its publisher; read the full piece at the link above._
