Tag: atmosphere

  • Why Is the Sky White in the Winter?

    Why Is the Sky White in the Winter?

    The cooler air and lower humidity in winter contribute to the sky’s purportedly whiter appearance compared to other seasons. Clouds are made up of small ice crystals, which develop when the moisture in the air freezes. The sky seems white in winter because the ice crystals reflect light in all directions. In contrast, since the air is warmer and more humid in the summer, it is the water droplets rather than the ice crystals that produce the clouds. The sky seems bluer in summer since these water droplets scatter light in a manner distinct from that of ice crystals.

    White Sky: The Essential Aspects

    • When it’s very chilly outside, the sky might seem white instead of the typical summertime blue.
    • There is a simple scientific explanation for the blue sky and the evening glow.
    • One reason for this is because, despite its white appearance, sunlight really contains a wide spectrum of electromagnetic radiation. The colors of a rainbow are an illustration of how they may be seen by humans.
    • Yet, there is still a chance of being deceived; not all strange phenomena in the sky can be explained physically. Some colors we see in the sky could be the consequence of our own imaginations, just like a low full Moon is not actually bigger than the usual Moon.
    A color prism. (Credit: Lucas Vieira)

    Using a prism, you can see that white light is really made up of many different colors (wavelengths). A white beam of light passing through a piece of triangular glass will emerge from the other side in a variety of hues. After seeing how amazing the effect was, Pink Floyd decided to use it as the central theme for their classic album, “The Dark Side of the Moon.”

    It’s not the season, but rather the amount of moisture in the air that determines whether or not the sky looks bluer or whiter.

    Why Does the Sky Seem Whiter in the Winter?

    There is no significant difference in the sky’s color in the summer and winter. The winter sky is just as blue as the summer one (including the white skies in summer). However, some days, even in apparently clear weather, the sky might look “whiter” than others due to certain circumstances. This effect is mostly determined by the humidity, or how foggy the air is.

    High fog is more common in the fall and winter than in the summer because of the increased humidity. The sky appears white because of light diffraction from the tiny water droplets. In the winter, when the sun takes longer to burn off dense fog, the color effect may last into the day.

    atmosphere light scattering
    The effect of light diffraction sets the color of the sky.

    It’s the same with aerosols. Dust and soot are two common examples of such minute airborne particles. The sky seems whiter in the winter because of the increased concentration of aerosols caused by increased heating.

    But, without clouds or fog, the winter sky can still look brighter and whiter: After entering Earth’s atmosphere, the blue portion of the sun’s rays disperses in all directions. In a normal world, this would make the sky above you seem brilliant blue. But the winter provides a longer route for the sunrays through the atmosphere since the sun is lower. The blue light is so diffused that it can hardly reach your eyes and the sky appears whiter.

    The area close to the horizon especially turns brighter than the remaining parts of the sky, creating a similar white impression. The sun’s rays coming in from the horizon are dispersed so many times by the air molecules that the resulting spectrum is (nearly) white. Overall, the sky will be whiter because of the various wavelengths of light mixing together to form white. This impact, however, is not seasonal, occurring both in the winter and the summer.

    In the winter, when there is a lot of snow, some of the sunlight will be reflected back into the sky. This also adds to the effect.

    Why Is the Sky Blue?

    Sunlight has a wide variety of colors. From red to blue, that’s where you’ll find the visible light spectrum. When all combined, it’s just white. When this spectrum of light reaches Earth’s atmosphere, the molecules of oxygen and nitrogen, as well as the water droplets and dust particles, deflect (or “diffract”) some of the light.

    In this mechanism, blue light is dispersed in all directions to a considerably greater extent than red light. The atmosphere (the “sky”) appears blue because of this scattering effect, regardless of your point of view. The air itself acts as a “carrier” for the color, but in reality, it is just the reflected blue light that hits your eye.

    The Impact of Altitude on Sky Color

    sky cloud
    (Image: Freepik)

    At noon, the sun travels a relatively short distance through the air envelope before reaching the border with space, which is just 60 miles (100 km) away. The sun appears yellow on Earth because only a small fraction of the blue light it emits can get through the atmosphere. At higher altitudes, the filtering effect is lowered. Therefore, the sky seems slightly whiter to those flying at an altitude of 6 miles (10 km) than it does to those on the ground.

    Rayleigh Radiation

    scattering
    The sky color and Rayleigh scattering (Credit: Gsu.edu)

    This intriguing phenomenon, named after its discoverer, Baron Rayleigh, determines the degree to which the light is dispersed. An intense deflection occurs when a particle is smaller than the wavelength of the incident light. This implies that the atmosphere scatters sunlight’s shorter-wavelength blue rays around four times more powerfully than its longer-wavelength red rays.

    Why Does the Sky Become Red During Sunset?

    The problem with sunset is that light has to travel through the atmosphere for 40 times longer at night than it does during the day, especially when the sun is at its optimal position just above the equator.

    As during the day, the blue light is still scattered during sunsets. But the blue light from sunlight is nearly entirely filtered away during sunset as it travels through the Earth’s atmosphere, so the sky is no longer illuminated by it.

    In addition, ozone (O3) and water molecules in the upper atmosphere absorb part of the blue wavelengths.

    Sunsets on the beach are nearly entirely composed of the long-wave red light that penetrates the atmosphere due to the position of the sun in the sky.

    The sun’s rays are not only weaker in the evening, but they also no longer include any short-wave UV radiation, which is why sunburns are no longer common.

    When additional particles, such as ash from a volcanic eruption, dust from a sandstorm, smoke from forest fires, and, sadly, fine dust from air pollution, are also floating in the air, the sky may become a spectacular crimson in turn.

    The Sky in Space

    This picture of the ISS space station also doesnt show any stars

    No matter how high the Earth is in the sky, the sky on the Moon will always be completely dark. Even though the Moon looks to be encased in a blue sky here on Earth during the day, the space doesn’t light blue. There are no particles in a vacuum to reflect light of any color, hence, a vacuum cannot emit any colors. Transparency permeates all of space. It’s dark everywhere else in the universe except for the stars, which shine in a rainbow of colors based on their composition.

    References

    1. David K. Lynch; William Charles Livingston (2001). Color and light in nature. Cambridge University Press. p. 31. ISBN 978-0-521-77504-5.
    2. Gibbs, Philip (May 1997). “Why is the sky Blue?” Usenet Physics FAQ.
    3. Craig F. Bohren & Eugene Edmund Clothiaux (2006). Fundamentals of Atmospheric Radiation: An Introduction with 400 Problems.
  • A new structure found in the Sun’s corona

    A new structure found in the Sun’s corona

    A hitherto unseen structure in the Sun’s corona, a dynamic network of interwoven plasma filaments, has been discovered by astronomers. Researchers claim in Nature Astronomy that a structure only observable in ultraviolet light could be found in the solar atmosphere’s middle layer, and that it contains key information about the slow solar wind’s origins. Scientists found that solar wind particles are accelerated by magnetic energy released when this plasma network interacts.

    As the solar system’s driving force, the solar wind could strip planets of their atmospheres, change their surface chemistry, and distort their magnetic fields. At the same time, the heliosphere, which is a protective bubble encircling our solar system, is formed by the constant flux of charged particles and the solar magnetic field. However, the genesis of the solar wind is poorly understood despite its significance for our cosmic home.

    new corona structure 2

    New studies and calculations suggest that the fast, energetic portion of the solar wind originates from very hot, magnetic areas in the chromosphere, the lower solar atmosphere. The solar corona looks darker in UV light in these regions. Up until recently, however, the origin of the solar wind’s slower, steadier component remained unknown.

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    The first view of the corona’s central region

    An observation of the solar corona has now yielded the first hints as to the cause of the sluggish solar wind. This is thanks to the first-ever imaging and analysis of the complete middle corona in UV light, which was made possible by the efforts of a team led by Pradeep Chitta. In the past, this layer, which starts at a height of around 220,000 miles (350,000 km) above the solar surface, went unnoticed since space missions and solar observatories mainly examined layers deeper or higher up.

    To examine the middle solar corona in greater detail for the first time ever, it required the launch of just three new weather satellites of the U.


    S. GOES system. That’s because, in order to foretell space weather, they also carry UV cameras aimed at the Sun. After a particular measuring effort, scientists have examined the data obtained by these sensors.

    Tangled network of plasma filaments

    For the first time, photographs of this layer of the solar corona showed its intricate, dynamic structure. Threadlike, braided plasma structures were seen in the corona above locations where black coronal holes bordered zones of intense magnetic activity. Above their peaks, they discovered highly organized and varied streams of sluggish solar wind, indicating ongoing interactions and enduring remodeling in this coronal network.

    Data from the Solar Dynamics Observatory (SDO) and the Solar Telescope Array (SOHO) showed that the plasma filaments in this coronal web seem to follow magnetic field lines, and that these lines continually cross and interact with each other.

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    Initially disjointed magnetic structures converge and eventually shut into loops. Earlier simulations have indicated that energy is released during such magnetic reconnection processes.

    Solar wind slowing mechanism

    Scientists may have uncovered a key mechanism responsible for the sluggish solar wind. It’s because their research indicates the recently uncovered coronal network aids in the acceleration of charged particles in the solar wind. They postulate that the magnetic field’s structure gets conveyed to the sluggish solar wind and performs a significant function in propelling the solar wind particles into space at high velocities.

    New observations of magnetic “switchbacks” in the solar wind by the Parker Solar Probe and the Solar Orbiter solar probes are consistent with the finding of the coronal network and magnetic reconnections in the core solar corona.


    These transient increases in the coronal magnetic field lines could possibly be the result of ongoing network changes in the corona.

    The findings provide evidence in favor of reconnection-based theories of the weak solar wind.

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    Additional data from the presently operational solar probes, as well as future missions, is needed to provide researchers with a deeper understanding of the processes occurring in the middle solar corona. As part of their mission, several of the future probes will carry sensors designed to study the middle corona.

  • ELVES: When a Lightning Produces Powerful Electromagnetic Pulses

    ELVES: When a Lightning Produces Powerful Electromagnetic Pulses

    Lightning is only one of several electromagnetic phenomena caused by thunderstorms that we can see here on Earth. Pilots have reported seeing red “sprites” and “blue jets” above thunderclouds for decades. Translucent, ring-shaped “ELVES” and gamma-ray bursts that seemed to originate from the clouds have also been reported. The interconnected nature of these radiation events is still poorly understood. But there is a possible connection between the ELVES and the gamma-ray bursts.

    What Is An ELVES?

    The large formation of an ELVES recorded by the International Space Station from 250 miles (400 km) above.
    The large formation of an ELVES recorded by the International Space Station from 250 miles (400 km) above. (Credit: ESA)

    Emissions of Light and Very Low Frequency Perturbations due to Electromagnetic Pulse Sources” is an abbreviation for this singular occurrence called ELVES. The ELVES is a kind of TLE, or “Transient Luminouse Events.” Transient luminous events (TLEs) are atmospheric phenomena that arise as a byproduct of primary thunderstorm lightning.

    The light of an ELVES comes from the excitation of nitrogen molecules brought on by collisions between electrons. The electromagnetic pulse might have energized the electrons due to a discharge from an underlying thunderstorm.

    The Atmosphere-Space Interactions Monitor (ASIM) captured this animation of a terrestrial gamma-ray flash (TGF) and subsequent ELVES. (Credit: Birkeland Centre for Space Science and Mount Visual)

    The ELVES usually glows for 1 millisecond, and they appear as a ring-shaped light expanding 250 mi (400 km) in diameter. ELVES was originally recorded on an STS-41 Space Shuttle flight in 1990. For a while, nobody knew for sure what color ELVES was, but we now believe it is red.

    Short gamma-ray bursts generated in thunderstorms appear to be responsible for the formation of ELVES.

    How Does ELVES Form?

    Above the thunderclouds, the infographic depicts a variety of electromagnetic events including the ELVES.
    Above the thunderclouds, the infographic depicts a variety of electromagnetic events including the ELVES.

    Some millionths of a second is all that this gamma-ray burst in the atmosphere above a thunderstorm takes. The intense electromagnetic field produced by a lightning strike accelerates electrons in the immediate vicinity. These electrons collide with the nitrogen molecules, exciting them.

    During intense discharges, the electrons gain enough speed to combine with other air particles, producing gamma rays. The gamma flash that is sent into the atmosphere as a consequence usually only lasts for 30–40 millionths of a second (microseconds).

    When Thunderstorms Produce Powerful Electromagnetic Pulses

    Late in March, around 62 miles (100 km) above Ancona, Italy, a red ELVES ring with a radius of approximately 220 miles (350 km) was photographed.
    Late in March, around 62 miles (100 km) above Ancona, Italy, a red ELVES ring with a radius of approximately 220 miles (350 km) was photographed. (Credit: Valter Binotto)

    In addition to the gamma-ray, the lightning from a thunderstorm produces powerful electromagnetic waves that go upwards through the atmosphere as an electromagnetic pulse (EMP). This occurs because lightning supercharges the ions present in the atmosphere. This is where the formation of ELVES comes into play.

    Once the pulse reaches the bottom of the ionosphere, some 50–55 miles (80–90 km) above the earth, it converts its energy to electrons, which in turn hit gas molecules—usually nitrogen—in the atmosphere, stimulating them enough to create the primarily reddish light. This light is known as ELVES, or ELVESs in the plural.

    An ELVES is normally perceptible for a fraction of a second (usually 1 millisecond). Many reported ELVES glows started about the same time as the gamma-ray burst, providing evidence that the two events could be related.

    The Electromagnetic Event of ELVES

    Artist’s impression of TARANIS in orbit with thunderstorms generating ELVES.
    Artist’s impression of TARANIS in orbit with thunderstorms generating ELVES. (Credit: NASA)

    The European Space Agency’s Atmosphere-Space Interactions Monitor (ASIM) captured numerous signals from a thunderstorm reported by ISS astronauts east of the Indonesian island of Sulawesi. Lightning in the cloud was the first visible sign of this electromagnetic phenomenon.

    A gamma-ray burst was likely set off at its onset. Scientists believe gamma rays are created when supersonic electrons collide with airborne atomic nuclei, slow down, and release high-energy photons during a thunderstorm.

    The strong electric field associated with lightning (light blue) results in a terrestrial gamma-ray burst (magenta). The subsequent electromagnetic pulse is what causes ELVES, the widening ring of UV emission (red and white).
    The strong electric field associated with lightning (light blue) results in a terrestrial gamma-ray burst (magenta). The subsequent electromagnetic pulse is what causes ELVES, the widening ring of UV emission (red and white). (Credit: NASA)

    The gamma-ray burst lasted for 30–40 microseconds and was seen to occur at a height of around 7.5 miles (12 km), or 0.60 miles (1 km) below the cloud top. The flare not only emitted gamma rays, but also set off an electromagnetic pulse in the thunderstorm that spread horizontally and vertically for miles. At that height of 50–55 miles (80–90 km), it created an ELVES, which appeared as a ring-shaped light.

    The ISS’s sophisticated detectors picked it up in the electromagnetic spectrum’s reddish and ultraviolet regions. This time the observed ELVES started to glow a little more than 10 microseconds after the gamma-ray burst began.