Dr Peter R. Young


Dr Young is a Research Astrophysicist at NASA Goddard Space Flight Center. His field of research is the study of ultraviolet spectra from the Sun and other stars. Links to Dr Young's publications and projects he is involved with are given below.

Publications
Lectures & talks CHIANTI
Hinode/EIS SOHO/CDS IRIS
Data analysis guides Research Projects Solar Orbiter/SPICE
NASA/GSFC activities
Observing programs HelioIndex

News

10-Dec-2025
New article in Eos: "Shining a Light on the People Behind Solar Science." This article is about my HelioIndex project, written for the broader science community.
6-Nov-2025
New co-author paper published: Ryan et al., 2025, Sol. Phys., "Solar Orbiter's 2024 Major Flare Campaigns: An Overview."
27-Oct-2025
New co-author paper published: Namekata et al., 2025, Nature Astronomy, "Discovery of multi-temperature coronal mass ejection signatures from a young solar analogue."
10-Sep-2025
New co-author paper published: Milanović et al., 2025, A&A, "Thermal structuring of the quiet solar corona."
1-Sep-2025
New co-author paper published: Wallace et al., 2025, ApJ, "Connecting Solar Orbiter and L1 Measurements of Mesoscale Solar Wind Structures to Their Coronal Source Using the ADAPT-WSA Model."

Older news items

Gallery


This movie is from my recent paper. It shows a set of coronal loops at a temperature of around 7 million degrees. The loops brighten due to a solar flare and show a complex pattern of motion, brightening and fading. By the end of the sequence, the cooling loops are notably straighter than they were at the beginning. This indicates a release of magnetic energy during the flare. The white lines show the location of the Solar Orbiter/SPICE spectrometer slit.

Images are from the Atmospheric Imaging Assembly of NASA's Solar Dynamics Observatory. The sequence lasts 60 minutes (see time in top-left corner). The box has a size of 87,000 km x 33,000 km. For comparison, the Earth's diameter is 8000 km.

More images


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