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- https://phys.libretexts.org/Courses/Prince_Georges_Community_College/PHY_1030%3A_General_Physics_I/10%3A_Fluids/10.1%3A_IntroductionThere are four states of matter: solid, liquid, gas, and plasma.
- https://phys.libretexts.org/Courses/Joliet_Junior_College/Physics_201_-_Fall_2019/Book%3A_Physics_(Boundless)/11%3A_Temperature_and_Kinetic_Theory/11.08%3A_Phase_ChangesDuring a phase transition, certain properties of the medium change, often discontinuously, as a result of some external condition.
- https://phys.libretexts.org/Courses/Prince_Georges_Community_College/PHY_2030%3A_General_Physics_II/12%3A_Temperature_and_Kinetic_Theory/12.6%3A_Phase_ChangesDuring a phase transition, certain properties of the medium change, often discontinuously, as a result of some external condition.
- https://phys.libretexts.org/Bookshelves/Astronomy__Cosmology/Astronomy_2e_(OpenStax)/15%3A_The_Sun-_A_Garden-Variety_Star/15.02%3A_The_Structure_and_Composition_of_the_SunThe Sun, our star, has several layers beneath the visible surface: the core, radiative zone, and convective zone. These, in turn, are surrounded by a number of layers that make up the solar atmosphere...The Sun, our star, has several layers beneath the visible surface: the core, radiative zone, and convective zone. These, in turn, are surrounded by a number of layers that make up the solar atmosphere. In order of increasing distance from the center of the Sun, they are the photosphere, with a temperature that ranges from 4500 K to about 6800 K; the chromosphere, with a typical temperature of 104 K; the transition region, a zone that may be only a few kilometers thick.
- https://phys.libretexts.org/Bookshelves/University_Physics/Physics_(Boundless)/10%3A_Fluids/10.1%3A_IntroductionThere are four states of matter: solid, liquid, gas, and plasma.
- https://phys.libretexts.org/Learning_Objects/A_Physics_Formulary/Physics/11%3A_Plasma_physicsPlasma physics, Boltzmann transport equation, collisional dynamics
- https://phys.libretexts.org/Courses/Grossmont_College/ASTR_110%3A_Astronomy_(Fitzgerald)/09%3A_The_Sun/9.01%3A_The_Structure_and_Composition_of_the_SunThe Sun, our star, has several layers beneath the visible surface: the core, radiative zone, and convective zone. These, in turn, are surrounded by a number of layers that make up the solar atmosphere...The Sun, our star, has several layers beneath the visible surface: the core, radiative zone, and convective zone. These, in turn, are surrounded by a number of layers that make up the solar atmosphere. In order of increasing distance from the center of the Sun, they are the photosphere, with a temperature that ranges from 4500 K to about 6800 K; the chromosphere, with a typical temperature of 104 K; the transition region, a zone that may be only a few kilometers thick.
- https://phys.libretexts.org/Bookshelves/Astronomy__Cosmology/Astronomy_1e_(OpenStax)/15%3A_The_Sun-_A_Garden-Variety_Star/15.01%3A_The_Structure_and_Composition_of_the_SunThe Sun, our star, has several layers beneath the visible surface: the core, radiative zone, and convective zone. These, in turn, are surrounded by a number of layers that make up the solar atmosphere...The Sun, our star, has several layers beneath the visible surface: the core, radiative zone, and convective zone. These, in turn, are surrounded by a number of layers that make up the solar atmosphere. In order of increasing distance from the center of the Sun, they are the photosphere, with a temperature that ranges from 4500 K to about 6800 K; the chromosphere, with a typical temperature of 104 K; the transition region, a zone that may be only a few kilometers thick.
- https://phys.libretexts.org/Courses/Joliet_Junior_College/Physics_201_-_Fall_2019v2/Book%3A_Custom_Physics_textbook_for_JJC/12%3A_Temperature_and_Kinetic_Theory/12.08%3A_Phase_ChangesDuring a phase transition, certain properties of the medium change, often discontinuously, as a result of some external condition.
- https://phys.libretexts.org/Courses/Georgia_State_University/GSU-TM-Introductory_Physics_II_(1112)/zz%3A_Back_Matter/10%3A_13.1%3A_Appendix_J-_Physics_Formulas_(Wevers)/1.11%3A_Plasma_physicsPlasma physics, Boltzmann transport equation, collisional dynamics
- https://phys.libretexts.org/Bookshelves/University_Physics/Physics_(Boundless)/12%3A_Temperature_and_Kinetic_Theory/12.6%3A_Phase_ChangesDuring a phase transition, certain properties of the medium change, often discontinuously, as a result of some external condition.
