Spectroscopy and its Application Chemical and Biological detection Professor: Nam Sun Wang Haimo Liu 12/04/2007.

Slides:



Advertisements
Similar presentations
Astronomical Spectroscopy. The Electromagnetic Spectrum.
Advertisements

Light and Spectroscopy
Spectral Lines Celestial Fingerprinting. Goals From light we learn about –Composition –Motion.
Methods: Fluorescence Biochemistry 4000 Dr. Ute Kothe.
5 Spectral Lines Celestial Fingerprinting. 5 Goals From light we learn about –Composition –Motion.
Spectroscopy. Atoms and Light  Atomic electron energy levels are a source of discrete photon energies.  Change from a high to low energy state produces.
Light. What is Light? The third form of energy The only thing astronomers study Electromagnetic radiation The thing that our eyes detect How radio works.
Celestial Fingerprinting
L2 Spectral Lines Celestial Fingerprinting. L2 Continuum Spectra A Continuum Spectrum: Light emitted across a continuous range of wavelengths. A blackbody.
2B Spectral Lines Celestial Fingerprinting. 2B Continuum Spectra A Continuum Spectrum: Light emitted across a continuous range of wavelengths. A blackbody.
Advanced Higher Chemistry Unit 1 Spectroscopy. Spectroscopy  Spectroscopy is used to give information regarding the structure of atoms or molecules.
Lecture 13: Searching for planets orbiting other stars I: Properties of Light 1.How could we study distant habitats remotely ? 2.The nature of light -
4-1 Chap. 7 (Optical Instruments), Chap. 8 (Optical Atomic Spectroscopy) General design of optical instruments Sources of radiation Selection of wavelength.
Page 158. Emitting to the Truth Start a new thread/topic Learning Target: What does color tell us about the underlying structure of matter? Update TOC.
Origin of an Atomic Absorption Peak E2E2 E1E1  E = h Frequency Intensity Energy Transition Absorption Spectrum 1.
December in Antarctica: The Sun never sets. The images are 1 hour apart.
Chapter 4 Spectroscopy.
Atomic Spectra. Much of what we know about atomic structure comes from analysis of light either being emitted or absorbed by substances. Elements can.
Light and the Electromagnetic Spectrum. Light Phenomenon Isaac Newton ( ) believed light consisted of particles By 1900 most scientists believed.
Introduction to Excited Elements Lab
Atomic Emission Spectrum Make-Up Lab
Stars and Galaxies 28.1 A Closer Look at Light Chapter 28.
Light and the Electromagnetic Spectrum. Light Phenomenon Isaac Newton ( ) believed light consisted of particles By 1900 most scientists believed.
How do colors in a spectrum help us understand stars? Image from
Light and Energy How the structure of electrons relates to the function of emitting energy as light.
Light and Spectroscopy. Light  Charges interact via electric and magnetic forces  Light is a repetitive disturbance in these forces! Electromagnetic.
Chapter 5 Light: The Cosmic Messenger. 5.2 Learning from Light Our goals for learning What types of light spectra can we observe? How does light tell.
Fluorometric Analysis
How Do Materials Emit Light? Incandescence Atomic Emission Molecular Fluorescence Phosphorescence Photoluminescence.
Spectra What determines the “color” of a beam of light? The answer is its frequency, or equivalently, its wavelength. We see different colors because.
The Creation of Light. How is light created? All light starts as a vibration of charged particles, electrons that move between different energy levels.
Kepler 1: planet with two suns. Homework #3 Due Wednesday, 11:00 p.m. Answers to all homework questions will be posted on the class website First exam:
Spectroscopy The study of the interaction between matter and light.
© 2010 Pearson Education, Inc. Range of Visible Light Our eyes can see from 400 (blue/purple) to 700 (red) nm. Nm = nanometers = meters Our eyes.
Spectroscopy. Spectroscopy and Star Fingerprints LT: To understand how spectral lines can identify elements in a star. Terms: Spectroscopy – branch of.
Atomic Fluorescence Spectroscopy. Background l First significant research by Wineforder and Vickers in 1964 as an analytical technique l Used for element.
Emission Spectra.
Light and the Electromagnetic Spectrum. Light Phenomenon Isaac Newton ( ) believed light consisted of particles By 1900 most scientists believed.
Chemistry XXI Unit 2 How do we determine structure? The central goal of this unit is to help you develop ways of thinking that can be used to predict the.
Different Types of Spectrums. Types of Spectrums Continuous Spectrum Emission Spectrum Absorption Spectrum All colors of the spectrum Are shown (some.
Atomic Spectra and Electron Orbitals. The Classical Atom Electrons orbited the nucleus. Electrons orbited the nucleus. Problem!! Problem!! Accelerating.
Spectroscopy and Atoms
Starlight What is it? What does it tell us? Write down all notes in RED.
Spectroscopy Objectives –Understand the relationship between light, color, energy, frequency and wavelength of light –Understand how light interacts with.
Introduction to Infrared Spectroscopy
4. Complex Knowledge: demonstrations of learning that go aboveand above and beyond what was explicitly taught. 3. Knowledge: meeting the learning goals.
Friday Oct 17 Objective: Observe the emission spectrum of different elements and compare it with white light. Checkpoint: What ion does aluminum form after.
CHAPTER 5 The Structure of the Atom 5.4 Light and Spectroscopy.
Electron Arrangement Senior Chemistry R. Slider. Electromagnetic (EM) Spectrum Wavelength The actual length of one full wave. Notice: IR > vis > UV Wavelength.
Spectroscopy and its Application
Spectroscopy Lecture.
The Bohr Model of the Atom
Ground State vs. Excited State Electrons
BOHR’S ATOM AND ATOMIC SPECTRA
 Spectroscopy continued 
Physics and the Quantum Mechanical Model
Early Quantum Theory and Models of the Atom
CHAPTER 5 The Structure of the Atom 5.4 Light and Spectroscopy.
How do scientists know what stars and planets are made of?
Light and the Electromagnetic Spectrum
Nature of light and atomic spectrum
Energy and Electrons energy
Electromagnetic Spectrum and Space
Light, Photon Energies, and Atomic Spectra
5.4 Learning from Light Our goals for learning
Atomic emission spectrum
5.4 Learning from Light Our goals for learning
Understand the electromagnetic spectrum and how it is organized.
Aim: How to identify elements based on their atomic spectra
Matter and Particles of Light: Quantum Theory
Presentation transcript:

Spectroscopy and its Application Chemical and Biological detection Professor: Nam Sun Wang Haimo Liu 12/04/2007

Spectrum and Spectroscopy  Spectrum: (a). Different colors observed when the white light was dispersed through the prism (b). The changing of light intensity as a function of frequency  Spectroscopy: Study of spectrum, to identify substances

Spectroscopy  Types of spectroscopy: (a) Continuous spectroscopy (b) Absorption spectroscopy (c) Emission spectroscopy

Emission Process Electrons ground level High energy level Absorb energy Energy emission

Equipment  Left: Equipment diagram  Right: Schematic diagram

Applications  Absorption spectrum: used in deducing the presence of elements in stars and other gaseous objects which cannot be measured directly.  Emission spectrum: provide a definition of the spectrum of each atom, used to be compared with absorption spectrum

Spectrum of planets  Compare the absorption spectrum with the element’s emission spectrum, people can build the spectrum of planets.

Fluorescence Spectroscopy  Light source, self-emission which means the electrons transferred to the lowest level spontaneously  Different fluorescence: (a) different meta-stable states (b) different various vibrational states of the ground state

Time-resolved fluorescence spectroscopy  It provides fluorescence intensity decay in terms of lifetimes  Advantages: enhance the discrimination among fluorophores (overlapping emission spectra ) sensitive to various parameters of the biological microenvironment

Time-resolved fluorescence spectroscopy  Time-resolved laser-induced fluorescence spectroscopy (tr-LIFS)

Mathematical method

If is an impulse, then the impulse response will be

Mathematical method  Based on the definition of convolution:

Mathematical method  For the tr-LIFS system, the impulse response function is what would be recorded as the observed fluorescence decay Estimation of the intrinsic fluorescence decay was carried out via deconvolution of the observed fluorescence

Spectral Imaging system  Imaging provides intensity at every pixel of the image I (x, y)  spectrometer provides the intensity of a single spectrum, I(λ)  spectral image provides a spectrum at each pixel, I (x, y, λ)

Observation of multiple activities  Trying to use 5 different kinds of fluorescent molecules to label each of the 24 chromosomes in human body  2 to 5 minus 1=31

Observation of multiple colors

Living cell spectral imaging  Compromise: only two kinds of cellular organ were labeled

¿Questions?