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IONIZATION INSTABILITY

  • Ionization instability
  • ionization instability occurs from a feedback effect, when electrons produced by ionization go on to produce still more electrons through ionization in

    Ionization instability

    Ionization_instability

  • Electrothermal instability
  • The electrothermal instability (also known as ionization instability, non-equilibrium instability or Velikhov instability in the literature) is a magnetohydrodynamic

    Electrothermal instability

    Electrothermal_instability

  • Magnetohydrodynamic generator
  • Magnetohydrodynamic converter that transforms thermal and kinetic energy into electricity

    Conference on Ionization Phenomena in Gases. Belgrade, Yugoslavia. Shapiro, G. I.; Nelson, A. H. (12 April 1978). "Stabilization of ionization instability in a

    Magnetohydrodynamic generator

    Magnetohydrodynamic_generator

  • Plasma (physics)
  • State of matter

    temperatures are usually needed to sustain ionization, which is a defining feature of a plasma. The degree of plasma ionization is determined by the electron temperature

    Plasma (physics)

    Plasma (physics)

    Plasma_(physics)

  • Magnetohydrodynamic converter
  • Electromagnetic machine with no moving parts

    Shipuk, I. Ya (1965). Ionization instability of a plasma with hot electrons (PDF). 7th International Conference on Ionization Phenomena in Gases. Belgrade

    Magnetohydrodynamic converter

    Magnetohydrodynamic converter

    Magnetohydrodynamic_converter

  • Mass spectrometry
  • Analytical technique based on determining mass to charge ratio of ions

    formation. For example, ionized NF3 contains F−, which abstracts proton. Electrospray ionization (ESI) and thermospray ionization (TSI) are suited for high

    Mass spectrometry

    Mass spectrometry

    Mass_spectrometry

  • Instability strip
  • Region of an astronomical diagram

    temperature reaches 25,000–30,000 K, begins the He II layer (first He ionization). Second ionization of helium (He III) starts at depths where the temperature is

    Instability strip

    Instability strip

    Instability_strip

  • Ion
  • Particle, atom or molecule with a net electrical charge

    with less net electric charge is called the ionization potential, or ionization energy. The nth ionization energy of an atom is the energy required to

    Ion

    Ion

    Ion

  • Jeans instability
  • Star formation process

    The Jeans instability is a concept in astrophysics that describes an instability that leads to the gravitational collapse of a cloud of gas or dust. It

    Jeans instability

    Jeans instability

    Jeans_instability

  • Plasma stability
  • Degree to which disturbing a plasma system at equilibrium will destabilize it

    (drift) instability (in the Critical ionization velocity mechanism) Magnetic drift instability, Slow Drift Instability Electrothermal instability Fan instability

    Plasma stability

    Plasma stability

    Plasma_stability

  • Ice giant
  • Type of giant planet

    magnetically is likely to have magnetic dead zones, due to varying degrees of ionization, where mass moved by magnetic forces could pile up, eventually becoming

    Ice giant

    Ice giant

    Ice_giant

  • F-center
  • Type of crystallographic defect

    to move also. c)  Multiple ionization. This process requires the most energy. A photon interacts with a halide ion, ionizing it twice, leaving it positively

    F-center

    F-center

    F-center

  • Robert D. Richtmyer
  • American mathematician

    Richtmyer, Robert Davis (1935). Quantum Mechanical Study of Multiple-Ionization Collisions of a Fast Electron with an Atom. Massachusetts Institute of

    Robert D. Richtmyer

    Robert D. Richtmyer

    Robert_D._Richtmyer

  • Isotope-ratio mass spectrometry
  • Usage of mass spectrometry to measure remaining isotopes

    depend on IRMS using thermal ionization of a solid sample loaded into the source of the mass spectrometer (hence thermal ionization mass spectrometry, TIMS)

    Isotope-ratio mass spectrometry

    Isotope-ratio mass spectrometry

    Isotope-ratio_mass_spectrometry

  • Plasmoid
  • Plasma and magnetic field structure

    820–825. ISSN 0004-637X. Bostick, Winston H (1956). "Experimental Study of Ionized Matter Projected across a Magnetic Field". Physical Review. 104 (2): 292–299

    Plasmoid

    Plasmoid

    Plasmoid

  • Francium
  • Chemical element with atomic number 87 (Fr)

    refinement of the value for francium. Francium has a slightly higher ionization energy than caesium, 392.811(4) kJ/mol as opposed to 375.7041(2) kJ/mol

    Francium

    Francium

  • Genome instability
  • High frequency of mutations within the genome of a cellular lineage

    Genome instability (also genetic instability or genomic instability) refers to a high frequency of mutations within the genome of a cellular lineage. These

    Genome instability

    Genome instability

    Genome_instability

  • Magnetohydrodynamic drive
  • Vehicle propulsion using electromagnetic fields

    fluid is the air (a gas instead of a liquid) ionized to become electrically conductive (a plasma). Air ionization is achieved at high altitude (electrical

    Magnetohydrodynamic drive

    Magnetohydrodynamic drive

    Magnetohydrodynamic_drive

  • Firehose instability
  • Dynamical instability of thin or elongated galaxies

    The firehose instability (or hose-pipe instability) is a dynamical instability of thin or elongated galaxies. The instability causes the galaxy to buckle

    Firehose instability

    Firehose instability

    Firehose_instability

  • Kappa–mechanism
  • Cause of changes in luminosity in pulsating variable stars

    Technology, 2010 Cox, John P. (1963). "On Second Helium Ionization as a Cause of Pulsational Instability in Stars". The Astrophysical Journal. 138: 487. Bibcode:1963ApJ

    Kappa–mechanism

    Kappa–mechanism

  • Critical ionization velocity
  • Critical ionization velocity (CIV), or critical velocity (CV), is the relative velocity between a neutral gas and plasma (an ionized gas), at which the

    Critical ionization velocity

    Critical ionization velocity

    Critical_ionization_velocity

  • Hypocalcemia
  • Low calcium levels in one's blood serum

    electrical instability (and this is therefore a more critical condition than constant QTc prolongation). This type of electrical instability puts the person

    Hypocalcemia

    Hypocalcemia

    Hypocalcemia

  • Cepheid variable
  • Type of variable star that pulsates radially

    threshold is reached at which point double ionization cannot be sustained and the layer becomes singly ionized hence more transparent, which allows radiation

    Cepheid variable

    Cepheid variable

    Cepheid_variable

  • Streaming instability
  • Hypothetical formation of planetesimals

    the ionization rate is too low to sustain the magnetorotational instability. In the inner Solar System the formation of streaming instabilities requires

    Streaming instability

    Streaming instability

    Streaming_instability

  • Neutron radiation
  • Ionizing radiation that presents as free neutrons

    nucleus recoiling from a neutron interaction is ionized and causes more traditional subsequent ionization in other atoms. Because neutrons are uncharged

    Neutron radiation

    Neutron radiation

    Neutron_radiation

  • Alpha decay
  • Type of radioactive decay

    and ionizing photons. However, the recoil of the parent nucleus (alpha recoil) gives it a significant amount of energy, which also causes ionization damage

    Alpha decay

    Alpha decay

    Alpha_decay

  • Streamer discharge
  • Type of transient electric discharge

    electron loses the corresponding energy. Impact ionization, where the neutral particle becomes ionized, with the incident electron losing the energy. Attachment

    Streamer discharge

    Streamer discharge

    Streamer_discharge

  • Effects of ionizing radiation in spaceflight
  • Cancer causing exposure to ionizing radiation in spaceflight

    radiation from nuclear reactions from spacecraft parts or tissue. The ionization patterns in molecules, cells, tissues and the resulting biological effects

    Effects of ionizing radiation in spaceflight

    Effects of ionizing radiation in spaceflight

    Effects_of_ionizing_radiation_in_spaceflight

  • Pinch (plasma physics)
  • Compression of an electrically conducting filament by magnetic forces

    S2CID 250763028. Kruskal, M D; Schwarzschild (1954). "Some Instabilities of a Completely Ionized Plasma". Proc. R. Soc. Lond. A. 223 (1154): 348–360. Bibcode:1954RSPSA

    Pinch (plasma physics)

    Pinch (plasma physics)

    Pinch_(plasma_physics)

  • Chromosome instability
  • Type of genomic instability

    Chromosomal instability (CIN) is a type of genomic instability in which chromosomes are unstable, such that either whole chromosomes or parts of chromosomes

    Chromosome instability

    Chromosome_instability

  • Acetone peroxide
  • Chemical compound

    peroxide explosives by desorption electrospray ionization and desorption atmospheric pressure chemical ionization". Analytical Chemistry. 80 (5): 1512–9. doi:10

    Acetone peroxide

    Acetone peroxide

    Acetone_peroxide

  • Radiation-induced cancer
  • Cancer caused by ionizing radiation exposure

    not ionization, which is usually dissipated as heat with relatively little chemical damage. Ultraviolet light is usually categorized as non-ionizing, but

    Radiation-induced cancer

    Radiation-induced_cancer

  • Hall-effect thruster
  • Type of electric propulsion system

    preferred because its high atomic mass and relatively low ionization energy reduce ionization losses and support efficient thrust production. Lower-cost

    Hall-effect thruster

    Hall-effect thruster

    Hall-effect_thruster

  • Conditional symmetric instability
  • Conditional symmetric instability, or CSI, is a form of convective instability in a fluid subject to temperature differences in a uniform rotation frame

    Conditional symmetric instability

    Conditional symmetric instability

    Conditional_symmetric_instability

  • Atmospheric science
  • Study of the atmosphere, its processes, and its interactions with other systems

    the study of the upper layers of the atmosphere, where dissociation and ionization are important. Atmospheric science has been extended to the field of planetary

    Atmospheric science

    Atmospheric science

    Atmospheric_science

  • Aurora
  • Atmospheric effect caused by the solar wind

    precipitate into the upper atmosphere (thermosphere/exosphere). The resulting ionization and excitation of atmospheric constituents emit light of varying colour

    Aurora

    Aurora

    Aurora

  • Interchange instability
  • The interchange instability, also known as the Kruskal–Schwarzschild instability or flute instability, is a type of plasma instability seen in magnetic

    Interchange instability

    Interchange_instability

  • Molecular cloud
  • Type of interstellar cloud

    suggested by astronomers. Cloud growth by collision and gravitational instability in the gas layer spread throughout the galaxy. Models for the collision

    Molecular cloud

    Molecular cloud

    Molecular_cloud

  • Isotopes of thorium
  • energy is on the same order of magnitude as electron ionization energy (for reference, the ionization energy of hydrogen is 13.6 eV), the decay rate of 229mTh

    Isotopes of thorium

    Isotopes_of_thorium

  • Isotopes of americium
  • nuclear waste. It is the isotope used in normal ionization smoke detectors, which work as an ionization chamber. It is a potential fuel for long-lifetime

    Isotopes of americium

    Isotopes_of_americium

  • Orion Nebula
  • Diffuse nebula in the constellation Orion

    showed six unresolved high-ionization sources near the Trapezium Cluster. These sources were interpreted as partly ionized globules (PIGs). The idea was

    Orion Nebula

    Orion Nebula

    Orion_Nebula

  • Fluorine nitrate
  • Chemical compound

    linked to higher ionization potential due to the centrality of fluorine. This higher ionization potential is indicative of electron ionization of deeper shell

    Fluorine nitrate

    Fluorine nitrate

    Fluorine_nitrate

  • Neoplasm
  • Tumor or other abnormal growth of tissue

    usually has genome instability. This instability is likely due to reduced DNA repair or excessive DNA damage. Because of such instability, the cancer continues

    Neoplasm

    Neoplasm

    Neoplasm

  • Atomic radius
  • Measure of the size of an atom

    Ionic radius: the nominal radius of the ions of an element in a specific ionization state, deduced from the spacing of atomic nuclei in crystalline salts

    Atomic radius

    Atomic radius

    Atomic_radius

  • Electrospray
  • Apparatus that employs electricity to disperse a liquid into fine aerosol

    Fenn (2002 Nobel Prize in Chemistry) and others discovered electrospray ionization for mass spectrometry. To simplify the discussion, the following paragraphs

    Electrospray

    Electrospray

  • Rapidly oscillating Ap star
  • Type of variable star

    instability strip, it has been suggested that the driving mechanism may be similar, i.e. the opacity mechanism operating in the hydrogen ionization zone

    Rapidly oscillating Ap star

    Rapidly_oscillating_Ap_star

  • Plasma oscillation
  • Rapid oscillations of electron density

    the electromagnetic spectrum. The oscillations can be described as an instability in the dielectric function of a free electron gas. The frequency depends

    Plasma oscillation

    Plasma_oscillation

  • Causes of cancer
  • Genetic changes leading to uncontrolled cell growth and tumor formation

    basic cause of sporadic (non-familial) cancers is DNA damage and genomic instability. A minority of cancers are due to inherited genetic mutations. Most cancers

    Causes of cancer

    Causes_of_cancer

  • Proplyd
  • Dust ring surrounding large stars thousands of solar radii wide

    unresolved high-ionization sources near the Trapezium Cluster. These sources were not interpreted as proplyds, but as partly ionized globules (PIGs).

    Proplyd

    Proplyd

    Proplyd

  • Variable star
  • Star whose brightness fluctuates, as seen from Earth

    two layers where hydrogen and helium ionization occurs, respectively. These are referred to as partial ionization zones. The location of these layers determine

    Variable star

    Variable star

    Variable_star

  • Q-machine
  • emission, and ions are created through contact ionization of atoms of alkali metals that have low ionization potentials. The hot plate is made of a metal

    Q-machine

    Q-machine

  • Plasma railgun
  • Linear accelerator

    plasma armature in that case is subject to the "blow-by" instability. This is an instability in which the magnetic pressure front can out-run or "blow-by"

    Plasma railgun

    Plasma_railgun

  • Ataxia–telangiectasia
  • Rare neurodegenerative disease

    DSBs are defective. The result is genomic instability, which can lead to the development of cancers. Ionizing radiation (such as X-rays and gamma rays)

    Ataxia–telangiectasia

    Ataxia–telangiectasia

  • Stellar classification
  • Classification of stars based on spectral properties

    a theory of ionization by extending well-known ideas in physical chemistry pertaining to the dissociation of molecules to the ionization of atoms. First

    Stellar classification

    Stellar classification

    Stellar_classification

  • Plutonium-241
  • Isotope of plutonium

    immediately precedes actinium (89) and follows a three-element gap of instability after polonium (84) where no nuclides have half-lives of at least four

    Plutonium-241

    Plutonium-241

  • Radiobiology evidence for protons and HZE nuclei
  • in cancer cells can result in instability in multiple chromosomes. These recent results suggest that telomere instability could be an important early event

    Radiobiology evidence for protons and HZE nuclei

    Radiobiology_evidence_for_protons_and_HZE_nuclei

  • Outline of astrophysics
  • Subfield of astronomy

    self‑consistent electric and magnetic fields. Critical ionization velocity – Threshold limiting plasma ionization in cosmic shocks and aurorae. Dissociative recombination

    Outline of astrophysics

    Outline_of_astrophysics

  • Field-emission electric propulsion
  • Type of electric spacecraft propulsion system

    propulsion (FEEP) is an electrostatic propulsion method based on field ionization of a liquid metal, and subsequent acceleration of the ions by a strong

    Field-emission electric propulsion

    Field-emission_electric_propulsion

  • Solar corona
  • Outermost layer of the Sun's atmosphere

    a specialized coronagraph. Spectroscopic measurements indicate strong ionization in the corona and a plasma temperature in excess of 1000000 kelvins, much

    Solar corona

    Solar corona

    Solar_corona

  • Ultraviolet
  • Form of electromagnetic radiation

    harmful interactions of non-ionizing radiation in living organisms, conventionally demarcated around 10 eV, the first ionization energy of oxygen. UV ranges

    Ultraviolet

    Ultraviolet

    Ultraviolet

  • Sonoluminescence
  • Luminescence induced by sound waves

    (even a small drop in temperature causes a large drop in ionization, due to the large ionization energy relative to photon energy). This description is

    Sonoluminescence

    Sonoluminescence

    Sonoluminescence

  • Structure formation
  • Astrophysical models for the formation of galaxies and clusters of galaxies

    containing few galaxies. Structure formation applies models of gravitational instability to small ripples in mass density to predict these shapes. The modern

    Structure formation

    Structure formation

    Structure_formation

  • Zap Energy
  • American nuclear fusion energy company

    United Kingdom. At first, it appeared these designs were free from the instabilities of the earlier devices. However, further investigation showed that new

    Zap Energy

    Zap_Energy

  • Evgeny Velikhov
  • Russian physicist (1935–2024)

    Bibcode:1959JETP....9..995V. E.P. Velikhov (1962). "Hall instability of current-carrying slightly-ionized plasmas". Newcastle-upon-Tyne, England. 1st International

    Evgeny Velikhov

    Evgeny Velikhov

    Evgeny_Velikhov

  • Engine knocking
  • Problem in internal combustion engines

    Combustion and knock in a spark-ignition engine (Archived) NACA Report 774 - Ionization in the knock zone of an internal combustion engine (Archived) NACA Report

    Engine knocking

    Engine knocking

    Engine_knocking

  • Biological effects of radiation on the epigenome
  • radiation therapy expose the individual to ionizing radiation. Irradiated cells can also induce genomic instability in neighboring un-radiated cells via the

    Biological effects of radiation on the epigenome

    Biological_effects_of_radiation_on_the_epigenome

  • Cancer
  • Group of diseases involving cell growth

    in the progression to cancer and are a possible cause of the genetic instability characteristic of cancers. Reduced expression of DNA repair genes disrupts

    Cancer

    Cancer

    Cancer

  • CI
  • Topics referred to by the same term

    interferometry, a radio and optical communication coding technology Chemical ionization, a technique used in mass spectrometry Configuration interaction, a post-Hartree–Fock

    CI

    CI

  • Helium-4
  • Isotope of helium

    estimate of the key atomic properties of helium-4, such as its size and ionization energy. The size of the 4He nucleus has long been known to be in the order

    Helium-4

    Helium-4

    Helium-4

  • Magnetosphere of Jupiter
  • Magnetic field around the Jovian system

    of plasma diffusion due to interchange instability. The process is similar to the Rayleigh-Taylor instability in hydrodynamics. In the case of the Jovian

    Magnetosphere of Jupiter

    Magnetosphere of Jupiter

    Magnetosphere_of_Jupiter

  • Argon flash
  • Single-use source of very short and extremely bright flash of light

    processes, while noble gases are monatomic and can only undergo ionization; the ionized gas then produces the light. The low specific heat capacity of

    Argon flash

    Argon_flash

  • Extended periodic table
  • Periodic table of the elements with eight or more periods

    Hence, its first ionization energy would be smaller than thorium's (Th: 6.3 eV; element 122: 5.6 eV) because of the greater ease of ionizing unbibium's 8p1/2

    Extended periodic table

    Extended periodic table

    Extended_periodic_table

  • Pickup ion
  • heliosphere are ionized by either solar ultraviolet radiation, charge exchange with solar wind protons or electron impact ionization. Pickup ions are

    Pickup ion

    Pickup ion

    Pickup_ion

  • Filament propagation
  • Diffractionless propagation of a light beam

    self-focusing is not possible. Multiphoton ionization, inverse Bremsstrahlung and electron avalanche ionization are three major results of gas and laser

    Filament propagation

    Filament_propagation

  • Downwinders
  • Persons exposed to nuclear test fallout

    "Non-targeted and Delayed Effects of Exposure to Ionizing Radiation: II. Radiation-Induced Genomic Instability and Bystander Effects Clastogenic Factors and

    Downwinders

    Downwinders

  • Astrophysical plasma
  • Plasma outside of the Solar System

    Terminology, 5th ed. (the "Gold Book") (2025). Online version: (2006–) "Ionization". doi:10.1351/goldbook.I03183 Lazarian, A.; Boldyrev, S.; Forest, C.;

    Astrophysical plasma

    Astrophysical plasma

    Astrophysical_plasma

  • Iris Nebula
  • Reflection nebula in the constellation Cepheus

    first is gravitational instabilities occurring on small scales forming dense shells and chains of YSOs along fronts of ionization. The sections scenario

    Iris Nebula

    Iris Nebula

    Iris_Nebula

  • Fusion power
  • Electricity generation by nuclear fusion

    once it is heated past its ionization energy. The resultant bare nucleus is a type of ion. The result of this ionization is plasma, which is a heated

    Fusion power

    Fusion power

    Fusion_power

  • Protoplanetary disk
  • Gas and dust surrounding a newly formed star

    proplyd 177-341W in the Orion Nebula observed with VLT MUSE, showing an ionization front, protoplanetary disk, and tail HOPS-315, a still-forming planetary

    Protoplanetary disk

    Protoplanetary disk

    Protoplanetary_disk

  • Tokamak
  • Magnetic confinement device used to produce thermonuclear fusion power

    of magnetic confinement had attempted this, but demonstrated serious instabilities. The safety factor (labelled q in mathematical notation) guided tokamak

    Tokamak

    Tokamak

    Tokamak

  • Chronology of the universe
  • History and future of the universe

    possible to study the state of ionization at many different times in the past. Reionization began as "bubbles" of ionized hydrogen which became larger over

    Chronology of the universe

    Chronology of the universe

    Chronology_of_the_universe

  • Unbibium
  • Theoretical chemical element with atomic number 122 (Ubb)

    first ionization energy of 5.651 eV and second ionization energy of 11.332 eV are predicted for unbibium; this and other calculated ionization energies

    Unbibium

    Unbibium

  • Atmospheric physics
  • Sub-field of physics dealing with the atmosphere's structure, composition, and motion

    concerning the upper layers of the atmosphere, where dissociation and ionization are important. Remote sensing is the small or large-scale acquisition

    Atmospheric physics

    Atmospheric physics

    Atmospheric_physics

  • Magnetosphere of Saturn
  • Cavity in the solar wind created by Saturn

    gradually moves out from the inner magnetosphere via the interchange instability mechanism and then escapes through the magnetotail. The interaction between

    Magnetosphere of Saturn

    Magnetosphere of Saturn

    Magnetosphere_of_Saturn

  • Tetranitrogen
  • Chemical compound

    spectrometry (NRMS). In the synthesis, N+ 4 (which was first formed in the ionization chamber of the mass spectrometer) underwent two high energy collision

    Tetranitrogen

    Tetranitrogen

    Tetranitrogen

  • Livermorium
  • Chemical element with atomic number 116 (Lv)

    reflected in the expected ionization energies of livermorium, where there are large gaps between the second and third ionization energies (corresponding

    Livermorium

    Livermorium

  • Mushroom cloud
  • Cloud of debris and smoke from a large explosion

    volume of lower-density gases at any altitude, causing a Rayleigh–Taylor instability. The buoyant mass of gas rises rapidly, resulting in turbulent vortices

    Mushroom cloud

    Mushroom cloud

    Mushroom_cloud

  • Type II supernova
  • Explosion of a star 8 to 45 times the mass of the Sun

    ISSN 0004-6361. S2CID 253107572. Utrobin, V. P. (1996). "Nonthermal ionization and excitation in Type IIb supernova 1993J". Astronomy and Astrophysics

    Type II supernova

    Type II supernova

    Type_II_supernova

  • B-type main-sequence star
  • Stellar classification distinguished by bright blue luminosity

    B[e] stars are distinct from Be stars in having unusual neutral or low ionization emission lines that are considered to have 'forbidden mechanisms', something

    B-type main-sequence star

    B-type main-sequence star

    B-type_main-sequence_star

  • Pattern formation
  • Study of how patterns form by self-organization in nature

    ISSN 1520-6106. Igor Grabec (1974). "Nonlinear Properties of High Amplitude Ionization Waves". The Physics of Fluids. 17 (10): 1834–1840. Bibcode:1974PhFl..

    Pattern formation

    Pattern formation

    Pattern_formation

  • Quasar
  • Active galactic nucleus (AGN) containing a supermassive black hole

    these lines range from neutral to highly ionized, leaving them highly charged. This wide range of ionization shows that the gas is highly irradiated by

    Quasar

    Quasar

    Quasar

  • Walter Alexander Strauss
  • American mathematician

    Proof of modulational instability of Stokes waves in deep water, submitted, with Huy Q. Nguyen. Steady states of gas ionization with secondary emission

    Walter Alexander Strauss

    Walter_Alexander_Strauss

  • List of plasma physics articles
  • instability Riggatron Ring current Rocket engine nozzle Runaway breakdown Rydberg atom Rydberg matter Safety factor (plasma physics) Saha ionization equation

    List of plasma physics articles

    List_of_plasma_physics_articles

  • RBMK
  • Type of Soviet nuclear power reactor

    void coefficient, the 'positive scram effect' of the control rods and instability at low power levels—which contributed to the 1986 Chernobyl disaster

    RBMK

    RBMK

    RBMK

  • Properties of water
  • Physical and chemical properties of pure water

    and OH− ions. Related to its amphoteric character, it undergoes self-ionization. The product of the activities, or approximately, the concentrations of

    Properties of water

    Properties of water

    Properties_of_water

  • Lithium
  • Chemical element with atomic number 3 (Li)

    chloride and potassium chloride. The nucleus of the lithium atom verges on instability, since the two stable lithium isotopes found in nature have among the

    Lithium

    Lithium

    Lithium

  • Atmosphere of Earth
  • Gas layer surrounding Earth

    includes the mesosphere, thermosphere, and parts of the exosphere. However, ionization in the mesosphere largely ceases during the night. The ionosphere forms

    Atmosphere of Earth

    Atmosphere of Earth

    Atmosphere_of_Earth

  • Sun
  • Star at the centre of the Solar System

    ISBN 978-0-935702-64-4. Rast, M.; Nordlund, Å.; Stein, R.; Toomre, J. (1993). "Ionization Effects in Three-Dimensional Solar Granulation Simulations". The Astrophysical

    Sun

    Sun

    Sun

  • Mechanism of sonoluminescence
  • free ions and halt light emission. Light pulse time is dependent on the ionization energy of the noble gas with argon having a light pulse of 160 picoseconds

    Mechanism of sonoluminescence

    Mechanism of sonoluminescence

    Mechanism_of_sonoluminescence

  • Tau Ceti
  • Single yellow-hued star in the constellation Cetus

    Heating Models for the Basal Flux Star τ Ceti Including Time-dependent Ionization: Results for Ca II and Mg II Emission", The Astrophysical Journal, 594

    Tau Ceti

    Tau Ceti

    Tau_Ceti

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Online names & meanings

  • Lavyansh
  • Boy/Male

    Hindu, Indian

    Lavyansh

    Part of Love

  • Balon
  • Surname or Lastname

    English

    Balon

    English : from Old French balon ‘bundle’, ‘roll’, ‘pack’, hence a nickname for a small, rotund man or possibly a metonymic occupational name for a carrier of goods and merchandise.French (Bâlon) : generally regarded as a habitational name from Baalons in the Ardennes, it may however simply be from balon ‘ball’, ‘roll’ (see 1) or a derivative of Bal.

  • Gaultney
  • Surname or Lastname

    English

    Gaultney

    English : habitational name from Gaultney in Rushton, Northamptonshire, probably so named from Old Norse gǫltr ‘boar’ + Old Danish klint ‘steep cliff or bank’ with the later addition of Middle English heye ‘enclosure’. The surname is not found in the U.K. In the U.S., it is concentrated in GA. Compare Gautney.

  • Rikka
  • Girl/Female

    Finnish Teutonic

    Rikka

  • Yahavi | யாகவீ/யஹாவீ 
  • Girl/Female

    Tamil

    Yahavi | யாகவீ/யஹாவீ 

    Bright

  • Riyah | رییاہ
  • Boy/Male

    Muslim

    Riyah | رییاہ

    Comfort

  • Sagari
  • Girl/Female

    Basque, Hindu, Indian, Kannada, Malayalam, Marathi, Sanskrit, Sindhi, Tamil, Telugu

    Sagari

    River; Of the Ocean

  • Ritva
  • Girl/Female

    Australian, Danish, Swedish

    Ritva

    Branch

  • Aaloecana
  • Girl/Female

    Indian, Telugu

    Aaloecana

    To Look Thoroughly

  • Ragavendra | ரகவேந்த்ர
  • Boy/Male

    Tamil

    Ragavendra | ரகவேந்த்ர

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IONIZATION INSTABILITY

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IONIZATION INSTABILITY

  • Ozonation
  • n.

    The act of treating with ozone; also, the act of converting into, or producing, ozone; ozonization.

  • Instability
  • n.

    The quality or condition of being unstable; want of stability, firmness, or steadiness; liability to give way or to fail; insecurity; precariousness; as, the instability of a building.

  • Denizenation
  • n.

    Denization; denizening.

  • Solidity
  • n.

    The state or quality of being solid; density; consistency, -- opposed to fluidity; compactness; fullness of matter, -- opposed to openness or hollowness; strength; soundness, -- opposed to weakness or instability; the primary quality or affection of matter by which its particles exclude or resist all others; hardness; massiveness.

  • Turningness
  • n.

    The quality of turning; instability; tergiversation.

  • Shittleness
  • n.

    Instability; inconstancy.

  • Instableness
  • n.

    Instability; unstableness.

  • Ozonization
  • n.

    Ozonation.

  • Fugacity
  • a.

    Uncertainty; instability.

  • Instability
  • n.

    Lack of determination of fixedness; inconstancy; fickleness; mutability; changeableness; as, instability of character, temper, custom, etc.

  • Fickleness
  • n.

    The quality of being fickle; instability; inconsonancy.

  • Instabilities
  • pl.

    of Instability

  • Denization
  • n.

    The act of making one a denizen or adopted citizen; naturalization.

  • Fugitiveness
  • n.

    The quality or condition of being fugitive; evanescence; volatility; fugacity; instability.

  • Lubricity
  • n.

    Slipperiness; instability; as, the lubricity of fortune.