Abstract The Extreme Ultraviolet (EUV) monitor is an instrument on the NASA Mars
Atmosphere and Volatile EvolutioN (MAVEN) mission, designed to measure the variability of …

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 …

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 …

Photoionization heating from ultraviolet (UV) radiation incidents on the atmospheres of hot
Jupiters may drive planetary mass loss. Observations of stellar Lyman-α (Lyα) absorption …

We report on the results of the Sun in Time multiwavelength program (X-rays to UV) of solar
analogs with ages covering∼ 0.1–7 Gyr. The chief science goals are to study the solar …

The lack of long and reliable time series of solar spectral irradiance (SSI) measurements
makes an accurate quantification of solar contributions to recent climate change difficult …

The Solar EUV Experiment (SEE) is one of four scientific instruments on the NASA
Thermosphere Ionosphere Mesosphere Energetics Dynamics (TIMED) spacecraft, which …

We present evidence for a correlation between the observed properties of hot Jupiter
emission spectra and the activity levels of the host stars measured using Ca ii H & K …

The Sun is the main energy source to Earth, and understanding its variability is of direct
relevance to climate studies. Measurements of total solar irradiance (TSI) exist since 1978 …

Abstract The Flare Irradiance Spectral Model (FISM) is an important tool for estimating solar
variability for a myriad of space weather research studies and applications, and FISM …