KnowraAtmospheric windowLinked fromLinked fromThe 21 pages that link to Atmospheric window, each with the reason it gives.All 21Broader topic 2Related 18Compared with 1Radio astronomyRelated: Radio windows allow many observations from the ground, though some frequencies are absorbed or disturbed.Infrared astronomyRelated: Infrared observatories use these transmission bands, while opaque bands require space-based telescopes.Greenhouse gasRelated: Greenhouse gases absorb in parts of the infrared spectrum that would otherwise escape through this window.Space telescopeRelated: These windows allow ground telescopes to observe bands otherwise associated with space missions.Infrared thermographyRelated: Thermal cameras select infrared bands that can pass through air with limited absorption.Radiative coolingRelated: Radiation escaping through this window can carry surface heat directly toward space.Spectral energy distributionRelated: Ground-based observations sample only spectral regions that reach through the atmosphere.OpacityRelated: Low atmospheric opacity in selected bands enables ground-based observation and surface heating.Optical astronomyRelated: Atmospheric transmission determines which optical wavelengths can be observed from the ground.Planetary equilibrium temperatureRelated: Radiation escaping through atmospheric windows helps determine the planet’s effective emission.Ultraviolet-BRelated: Ultraviolet-B transmission varies sharply across its band because atmospheric absorption is wavelength-dependent.Radiative equilibriumRelated: Wavelength-dependent transparency complicates estimates based on a single radiative temperature.South Pole TelescopeRelated: The dry, high Antarctic atmosphere makes key millimeter-wave observing windows unusually transparent.Outgoing longwave radiationRelated: Radiation in this spectral region can escape from near the surface with limited absorption.Atacama Large Millimeter/submillimeter ArrayRelated: ALMA observes from a high, dry plateau to access millimeter and submillimeter atmospheric windows.Infrared techniquesRelated: Infrared instruments often operate in these bands to observe through the atmosphere.Infrared telescopeRelated: Transmission windows determine which infrared wavelengths ground-based telescopes can observe.Submillimetre astronomyRelated: Water vapor absorbs much submillimetre radiation, leaving narrow windows for ground-based observations.
KnowraAtmospheric windowLinked fromLinked fromThe 21 pages that link to Atmospheric window, each with the reason it gives.All 21Broader topic 2Related 18Compared with 1Radio astronomyRelated: Radio windows allow many observations from the ground, though some frequencies are absorbed or disturbed.Infrared astronomyRelated: Infrared observatories use these transmission bands, while opaque bands require space-based telescopes.Greenhouse gasRelated: Greenhouse gases absorb in parts of the infrared spectrum that would otherwise escape through this window.Space telescopeRelated: These windows allow ground telescopes to observe bands otherwise associated with space missions.Infrared thermographyRelated: Thermal cameras select infrared bands that can pass through air with limited absorption.Radiative coolingRelated: Radiation escaping through this window can carry surface heat directly toward space.Spectral energy distributionRelated: Ground-based observations sample only spectral regions that reach through the atmosphere.OpacityRelated: Low atmospheric opacity in selected bands enables ground-based observation and surface heating.Optical astronomyRelated: Atmospheric transmission determines which optical wavelengths can be observed from the ground.Planetary equilibrium temperatureRelated: Radiation escaping through atmospheric windows helps determine the planet’s effective emission.Ultraviolet-BRelated: Ultraviolet-B transmission varies sharply across its band because atmospheric absorption is wavelength-dependent.Radiative equilibriumRelated: Wavelength-dependent transparency complicates estimates based on a single radiative temperature.South Pole TelescopeRelated: The dry, high Antarctic atmosphere makes key millimeter-wave observing windows unusually transparent.Outgoing longwave radiationRelated: Radiation in this spectral region can escape from near the surface with limited absorption.Atacama Large Millimeter/submillimeter ArrayRelated: ALMA observes from a high, dry plateau to access millimeter and submillimeter atmospheric windows.Infrared techniquesRelated: Infrared instruments often operate in these bands to observe through the atmosphere.Infrared telescopeRelated: Transmission windows determine which infrared wavelengths ground-based telescopes can observe.Submillimetre astronomyRelated: Water vapor absorbs much submillimetre radiation, leaving narrow windows for ground-based observations.