Lagboltz
Well-Known Member
Before we leave the topic of my original "3 statements" in post 56, I really need to make it clearer. The universe is full of stuff with varying amounts of internal energy. The first two following statements are simple atomic physics.
1. (Atomic physics) Each piece of stuff radiates EM energy at all wavelengths everywhere. For some particular object, the maximum possible amount of radiation at each wavelength it can emit is given by it's temperature and Plank's radiation law (Black Body (BB) radiation curve.) It almost never radiates the maximum. (emissivity is not 100%). It always emits radiation by the same BB curve no matter what stuff surrounds it.
2. (Atomic physics) Each piece of stuff absorbs any radiation that hits it, with an efficiency given by the same BB curve modified by that same emissivity. It doesn't matter how high or low the temperature of the surrounding stuff is, it still absorbs what hits it according to it's BB curve.
All the stuff creates a field of radiant energy, or lots of photons with various wavelenghs. Each piece of stuff continuously absorbs and emits radiation.
What else can we say about this space of stuff and radiation? This is where the laws of thermodynamics comes in.
3a. (First law) The total energy of the stuff is conserved (can't change.) No problem. Everyone knows that.
3b. (Second law) A hotter piece of stuff always radiates more energy to a colder piece, than the colder piece radiates to the hotter piece. Or conversely, a colder piece of stuff absorbs more energy from a hotter piece than it emits. (No mystery there. The BB curves shows that at a glance.) Thereby, colder stuff warms up and hotter stuff cools down.
(Aside remark) The above points are only about the transfer of radiant energy. Of course there are other ways heat energy can be created or transferred: Convection, conduction, heat of fusion, heat of vaporization, chemical energy (fire), nuclear energy (sun), kinetic energy (hurricane) etc... Study of the atmosphere includes many of them to various degrees, and the importance of each is different with different models of atmospheric science. Hence the controversy.
1. (Atomic physics) Each piece of stuff radiates EM energy at all wavelengths everywhere. For some particular object, the maximum possible amount of radiation at each wavelength it can emit is given by it's temperature and Plank's radiation law (Black Body (BB) radiation curve.) It almost never radiates the maximum. (emissivity is not 100%). It always emits radiation by the same BB curve no matter what stuff surrounds it.
2. (Atomic physics) Each piece of stuff absorbs any radiation that hits it, with an efficiency given by the same BB curve modified by that same emissivity. It doesn't matter how high or low the temperature of the surrounding stuff is, it still absorbs what hits it according to it's BB curve.
All the stuff creates a field of radiant energy, or lots of photons with various wavelenghs. Each piece of stuff continuously absorbs and emits radiation.
What else can we say about this space of stuff and radiation? This is where the laws of thermodynamics comes in.
3a. (First law) The total energy of the stuff is conserved (can't change.) No problem. Everyone knows that.
3b. (Second law) A hotter piece of stuff always radiates more energy to a colder piece, than the colder piece radiates to the hotter piece. Or conversely, a colder piece of stuff absorbs more energy from a hotter piece than it emits. (No mystery there. The BB curves shows that at a glance.) Thereby, colder stuff warms up and hotter stuff cools down.
(Aside remark) The above points are only about the transfer of radiant energy. Of course there are other ways heat energy can be created or transferred: Convection, conduction, heat of fusion, heat of vaporization, chemical energy (fire), nuclear energy (sun), kinetic energy (hurricane) etc... Study of the atmosphere includes many of them to various degrees, and the importance of each is different with different models of atmospheric science. Hence the controversy.