Climate Change and Astronomy: A Look at Long-Term Trends on Maunakea

TL;DR

This study analyzes 40 years of climate data at Maunakea to assess how changing conditions may impact its suitability for astronomy, finding stable meteorological parameters but increased wind speeds that could affect observational quality.

Contribution

It provides a comprehensive climatology of Maunakea over four decades, highlighting trends and stability in key parameters affecting astronomical observations.

Findings

Meteorological conditions remained relatively stable over 40 years.

Maximum wind speeds have increased, with more frequent gusts above 15 m/s.

The Fried parameter has not changed, indicating stable optical turbulence.

Abstract

Maunakea is one of the world's primary sites for astronomical observing, with multiple telescopes operating over sub-millimeter to optical wavelengths. With its summit higher than 4200 meters above sea level, Maunakea is an ideal location for astronomy with an historically dry, stable climate and minimal turbulence above the summit. Under a changing climate, however, we ask how the (above-) summit conditions may have evolved in recent decades since the site was first selected as an observatory location, and how future-proof the site might be to continued change. We use data from a range of sources, including in-situ meteorological observations, radiosonde profiles, and numerical reanalyses to construct a climatology at Maunakea over the previous 40 years. We are interested in both the meteorological conditions (e.g., wind speed and humidity), and the image quality (e.g., seeing). We find that meteorological conditions were, in general, relatively stable over the period with few statistically significant trends and with quasi-cyclical inter-annual variability in astronomically significant parameters such as temperature and precipitable water vapour. We do, however, find that maximum wind speeds have increased over the past decades, with the frequency of wind speeds above 15~m~s$^{-1}$ increasing in frequency by 1--2%, which may have a significant impact on ground-layer turbulence. Importantly, we find that the Fried parameter has not changed in the last 40 years, suggesting there has not been an increase in optical turbulence strength above the summit. Ultimately, more data and data sources-including profiling instruments-are needed at the site to ensure continued monitoring into the future and to detect changes in the summit climate.