Doppler effects 1970-01-01
The Doppler effect is a phenomenon that occurs when there is a change in frequency or wavelength of a wave in relation to an observer who is moving relative to the wave source. This effect is commonly associated with sound waves, but it also applies to electromagnetic waves, such as light. ### Key Points of the Doppler Effect: 1. **Source and Observer Movement**: - If the wave source moves toward the observer, the waves are compressed, resulting in a higher frequency (or shorter wavelength).
Earth phenomena 1970-01-01
Earth phenomena refer to natural processes and events that occur on Earth and are often characterized by their impact on the environment, weather, geology, and ecosystems. These phenomena can encompass a wide range of occurrences, including but not limited to: 1. **Weather Events**: Hurricanes, tornadoes, thunderstorms, heatwaves, and blizzards are examples of atmospheric phenomena that can have significant effects on the climate and human activities.
Electrical phenomena 1970-01-01
Electrical phenomena refer to various effects and behaviors associated with electricity, which includes electric charge, electric fields, currents, and voltage. These phenomena can manifest in several ways and can be observed in various contexts, from simple static electricity to complex electrical circuits and electromagnetic waves. Here are some key components and concepts associated with electrical phenomena: 1. **Electric Charge**: This is a fundamental property of matter that causes it to experience a force when placed in an electromagnetic field.
Ionization 1970-01-01
Ionization refers to the process in which atoms or molecules gain or lose electrons, resulting in the formation of charged particles known as ions. This can occur through various mechanisms, including: 1. **Loss of Electrons (Cation Formation)**: When an atom or molecule loses one or more electrons, it becomes positively charged, forming a cation. This often occurs in chemical reactions, where an atom donates an electron to another atom.
Optical phenomena 1970-01-01
Optical phenomena refer to the various behaviors and effects of light as it interacts with different materials and media. These phenomena can include a wide range of visual effects that result from the properties of light, such as reflection, refraction, diffraction, interference, polarization, and scattering. Here are some common optical phenomena: 1. **Reflection**: The bouncing back of light when it strikes a reflective surface, such as a mirror or calm water.
Physical properties 1970-01-01
Physical properties are characteristics of a substance that can be observed or measured without changing the substance's chemical composition. These properties help in identifying and describing materials. Some common physical properties include: 1. **Color**: The color of the material. 2. **Odor**: The smell associated with the substance. 3. **Density**: The mass per unit volume of a substance, typically expressed in grams per cubic centimeter (g/cm³) or kilograms per cubic meter (kg/m³).
Stellar phenomena 1970-01-01
Stellar phenomena refer to various events and characteristics associated with stars, including their formation, evolution, and eventual death. These phenomena can encompass a wide range of activities that occur in and around stars. Some key examples include: 1. **Star Formation**: The process by which gas and dust in molecular clouds collapse under gravity to form new stars.
Weather 1970-01-01
Weather refers to the atmospheric conditions in a specific place over a short period of time, typically hours to days. It encompasses various elements, including temperature, humidity, precipitation (such as rain or snow), wind speed and direction, atmospheric pressure, and cloud cover. Weather can change rapidly and is influenced by several factors, including geographic location, time of year, and local atmospheric conditions.
Ferromagnetism 1970-01-01
Ferromagnetism is a fundamental magnetic property of certain materials, primarily metals, characterized by a strong attraction to magnetic fields and the ability to retain magnetization even after the external magnetic field is removed. This behavior is due to the alignment of magnetic moments of atomic or molecular dipoles within the material.
Heat treating 1970-01-01
Scattering 1970-01-01
Scattering is a physical phenomenon that occurs when waves (such as light, sound, or other types of electromagnetic radiation) encounter an obstacle or inhomogeneity in the medium through which they are traveling. The interaction causes the waves to be deflected or spread out in different directions. Scattering can occur with various types of waves, such as electromagnetic waves (light), acoustic waves (sound), and matter waves (like electrons).
Superfluidity 1970-01-01
Superfluidity is a phase of matter characterized by the ability of a fluid to flow with zero viscosity. This means that a superfluid can flow without dissipating energy, allowing it to move through small openings and along surfaces without friction. The phenomenon is most commonly observed in liquid helium at very low temperatures, specifically in helium-4 (He-4) and helium-3 (He-3).
Vacuum 1970-01-01
A vacuum is a space that is essentially devoid of matter, meaning it has very low pressure and density, and contains very few particles, such as atoms or molecules. In an ideal vacuum, there would be no air or any other substances; however, achieving a perfect vacuum is practically impossible. In physics, vacuums are often described in terms of pressure, with standard atmospheric pressure at sea level being about 101,325 pascals (or 1 atmosphere).
Aharonov–Bohm effect 1970-01-01
Aharonov–Casher effect 1970-01-01
Andreev reflection 1970-01-01
Antiferromagnetism 1970-01-01
Arago's rotations 1970-01-01
Askaryan radiation 1970-01-01
Biefeld–Brown effect 1970-01-01