* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download Hands-on-training: Introduction to emission spectroscopy
Future Circular Collider wikipedia , lookup
Atomic nucleus wikipedia , lookup
Quantum electrodynamics wikipedia , lookup
Bremsstrahlung wikipedia , lookup
Theoretical and experimental justification for the SchrΓΆdinger equation wikipedia , lookup
Field electron emission wikipedia , lookup
Photoelectric effect wikipedia , lookup
Hands-on-training: Introduction to emission spectroscopy Risto Kronholm University of Jyväskylä Department of Physics Contents of emission spectroscopy hands-on-training Introduction to emission spectroscopy Introduction to experimental setup Setting up the experimental setup Optical emission spectrum measurements Analysis: Identification of the most intensive peaks Results: identification of the elements in plasma Contents of introduction to emission spectroscopy Motivation Basics of atomic physics Ionization Excitation Spontaneous emission Spectroscopy Motivation Electron cyclotron resonance ion sources are used for the production of high intensity highly charged ion beams To be able to use and make development to the ECR ion source, the plasma inside the source has to be studied and understood Invasive plasma diagnostic methods cannot be used as they disturb especially the high charge states of interest. Due to the spontaneous emission of excited states, visible light is emitted opening a possibility to study physics of ECR plasma without disturbing it Atomic physics We will concentrate only on atoms and ions Atoms and ions are composed of a massive nucleus and electrons bound to the nucleus potential In quantum mechanical model of atom, electrons can be described as mathematical wave functions These are called atomic orbital which are characterized by unique set of quantum numbers ππ = 1,2,3, β¦ and ππ = 0,1,2, β¦ , ππ β 1 and ππ = βππ, βππ + 1, β¦ , 0, β¦ , ππ β 1, ππ Each orbital can occupy maximum of two electrons with its 1 own quantum number π π = ± (atomic spin orbits) 2 Atomic physics Atomβs energies are quantized, each orbital has its specific energy Allowed energies of atom can be presented in energy-level diagram Spectroscopic notation for these states is ππππ π€π€ 2ππ+1πΏπΏπΏπΏ+ππ 1s1 2p 1ππ1 Lowest energy state of the atom is stable and it is called ground state Other higher energy stationary states are called excited states Atomic physics Electron can jump from a stationary state to another by emitting or absorbing energy These electronic transitions are called excitations and deexcitations If absorbed energy is high enough, electron can be removed from nucleus potential Atomic physics In ECRIS plasma heating is based on energy transfer from microwaves to electrons via electron cyclotron resonance Electron energies range from cold electrons with 1 eV energies up to hot electrons with energies in the order of 100 keV Collisions between electrons and atoms Electron impact ionization β’ Electron impact ionization if energy of electron is higher than ionization potential β’ Ionization rate π π ππ β ππππ , ππππ,ππ , πππ£π£ππ From ECRIS electron energy distribution function Excitations In addition to ionization, electron can also jump to higher energy stationary state These reactions are called excitations Electron impact excitation β’ Electron impact excitation β’ Excitation rate π π ππ β ππππ , ππππ,ππ , πππ£π£ππ From ECRIS electron energy distribution function Downward transition Excited electronic states can decay via radiative transition to lower energy states Electromagnetic radiation is emitted in transition Optically allowed transitions follow the selection rules: β βπΏπΏ = 0,1 β βπ½π½ = 0,1, but π½π½ = 0 to π½π½ = 0 is forbidden β βππ = 0 Electronic states which cannot decay via radiative transitions are called metastable states Spontaneous emission 7437 nm 53.7 nm 728 nm 501 nm 2058 nm 58.4 nm β’ Due to spontaneous emission electron in excited state undergoes a transition to a lower energy state β’ Photon with wavelength of ππ = βππ β(πΈπΈππ βπΈπΈππ ) will be emitted β’ Intensity of emission is πΌπΌππ = ππ ππ π΄π΄ππππ Metastable state Spontaneous emission β’ Emission lines donβt ever have sharp delta function profile (βππ > 0) β’ Profile depends on the broadening mechanism: β’ Natural broadening β’ Doppler broadening β’ Stark/Zeeman broadening β’ Instrumental broadening β’ In our plasma first three are small compared to instrumental broadening Spontaneous emission In this hands-on-training we will focus only to transitions in visible part of the whole electromagnetic spectrum Spontaneous emission Emitted photons can be measured and plotted to wavelength spectrum Optical emission plasma spectroscopy The wavelength spectrum of light is like a fingerprint of an element Light intensity depends on ion density and electron energy distribution function & Plasma spectroscopy can be used to identify particle species in the plasma Plasma spectroscopy can give insight on how different methods and different ECR parameters affects on electrons and high charge states. Analysis Analysis of emission spectrum Emission lines of different elements are listed in NIST spectral database https://www.nist.gov/pml/atomic-spectradatabase Analysis Analysis Analysis