Clouds and blowing snow (BLSN) occur frequently over Antarctica, where it is critical to understand their feedbacks to surface and atmospheric boundary layer processes. Dome C, an elevated East Antarctic station, dominated by lengthy periods of surface longwave (LW) radiative cooling, is selected to reveal cloud and BLSN impacts within a largely stable environment. The sky condition is classified as clear, cloudy, or BLSN, using 3 years of Cloud‐Aerosol Lidar and Infrared Pathfinder Satellite Observations satellite data. Co‐located and contemporaneous in situ observations are used to investigate the relationship of sky condition with surface and atmospheric boundary layer thermal structure, focusing on seasonal variability. Results show that increased downwelling LW radiation from clouds abate surface radiative cooling losses, contributing to warming during all seasons. An increase of 3°C in the mean surface air temperature is observed during spring, whereas, a more dramatic rise (around 10°C), due to accompanying large‐scale subsidence, is observed during fall and winter in association with clouds. For all seasons, the wind speed and wind speed shear are strongest during BLSN events, and the surface‐based inversion is weakened by cooling which peaks in a shallow above‐surface turbulent layer. The stronger background stability during fall and winter seasons, restricts turbulence and BLSN depths generally to the lowest tens of meters. The Earth's cryosphere is among the most rapidly evolving yet least well‐observed regions, and knowledge of clouds and BLSN interactions with the typical stable atmospheric boundary layer can help further understand energy and moisture exchanges. Plain Language Summary: The sky‐condition over Antarctica can be cloudy, clear, or characterized by blowing snow (BLSN) which is a phenomenon where snow is lifted, sometimes up to few hundreds of meters, and transported across the continent by winds. Knowing the impact of clouds and BLSN on the surface and the atmospheric boundary layer, which is the lower portion of the atmosphere that is directly linked to the surface, is crucial for understanding Antarctic climate. Dome C, an elevated dome‐shaped peak in East Antarctica, is chosen to study these impacts. In this location, an investigation covering a 3 year period using satellite observations and in situ measurements reveals that clouds can warm the surface and atmospheric boundary layer by increasing the downwelling longwave radiation. BLSN is accompanied by relatively stronger winds, and the wind‐driven atmospheric turbulence tends to weaken the strong positive temperature gradient in the atmospheric boundary layer, which is known as the temperature inversion. Temperature inversions are common at Dome C, and are most intense in the fall and winter seasons during which time they seemingly restrict the atmospheric turbulence and BLSN layer depth to a few tens to several tens of meters. Key Points: Cloud‐Aerosol Lidar and Infrared Pathfinder Satellite Observations and co‐located in situ observations allow study of cloud and blowing snow (BLSN) impacts on Antarctic atmosphereAt Dome C, clouds abate surface longwave radiative cooling losses, causing warming in all seasonsBLSN, accompanied by intense winds, weakens the temperature inversion, and is vertically restricted by strong background stability [ABSTRACT FROM AUTHOR]