This overview paper highlights the successes of the Ozone Monitoring Instrument (OMI) on
board the Aura satellite spanning a period of nearly 14 years. Data from OMI has been used …

The Sun and other stars are magnetic: magnetism pervades their interiors and affects their
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …

We present the final Sloan Digital Sky Survey IV (SDSS-IV) quasar catalog from Data
Release 16 of the extended Baryon Oscillation Spectroscopic Survey (eBOSS). This catalog …

This paper describes the recommended solar forcing dataset for CMIP6 and highlights
changes with respect to CMIP5. The solar forcing is provided for radiative properties, namely …

The brightness of the Sun varies on all timescales on which it has been observed, and there
is increasing evidence that this has an influence on climate. The amplitudes of such …

We assess the importance of factors that determine the intensity of UV radiation at the
Earth's surface. Among these, atmospheric ozone, which absorbs UV radiation, is of …

We present a new solar irradiance reference spectrum representative of solar minimum
conditions between solar cycles 24 and 25. The Total and Spectral Solar Irradiance Sensor …

We present an overview of state-of-the-art chemistry–climate and chemistry transport models
that are used within phase 1 of the Chemistry–Climate Model Initiative (CCMI-1). The CCMI …

An accurate solar-irradiance spectrum is needed as an input to any planetary atmosphere or
climate model. Depending on the spectral characteristics of the chosen model, uncertainties …

This brief introductory review of some recent developments in atmosphere–ionosphere
science is written for the “Vertical Coupling Special Issue” that is motivated by the 5th …