Fad! - Center for Molecular Protein Science, CMPS
... is considerably slower than predicted by the Debye-Stokes-Einstein equation. Charged residues, particularly carboxylate, are more extensively hydrated than other residues, accounting for the variation in the extent of hydration between different proteins. ...
... is considerably slower than predicted by the Debye-Stokes-Einstein equation. Charged residues, particularly carboxylate, are more extensively hydrated than other residues, accounting for the variation in the extent of hydration between different proteins. ...
Transparencies
... If dipole converged β2mrs = 0.4±0.1 Small discrepancy between LG and CMB dipoles are due to ZoA, 2nd and 3rd assumptions mentioned in the earlier slide and structure beyond. But no big deal! ...
... If dipole converged β2mrs = 0.4±0.1 Small discrepancy between LG and CMB dipoles are due to ZoA, 2nd and 3rd assumptions mentioned in the earlier slide and structure beyond. But no big deal! ...
Mössbauer Spectroscopy
... a stone from a boat. The majority of the energy is submitted to the stone, but a small amount goes into the kinetic energy of the recoiling boat. During the summer time, the boat will simply pick up this recoil energy. If, however, the person throws the stone during winter time, with the boat frozen ...
... a stone from a boat. The majority of the energy is submitted to the stone, but a small amount goes into the kinetic energy of the recoiling boat. During the summer time, the boat will simply pick up this recoil energy. If, however, the person throws the stone during winter time, with the boat frozen ...
Theory off chaotic light
... • Chaotic source: gas discharge lamp, where the different atoms are excited by an electrical discharge and emit their radiation independently of one another. emission line determined by statistical spread in atomic velocities and random occurrence of collisions. ...
... • Chaotic source: gas discharge lamp, where the different atoms are excited by an electrical discharge and emit their radiation independently of one another. emission line determined by statistical spread in atomic velocities and random occurrence of collisions. ...
Effects of ionospheric damping on MHD wave mode structure D.-H. Lee
... as f = 16–23, 30, 40 mHz (not shown). In both power spectrum and spatial structure, transverse modes are strongly affected by the damping rate, while the compressional modes are not. The results shown here are also indicative of the effects of other ionospheric damping coefficients, such as d = 0.8, ...
... as f = 16–23, 30, 40 mHz (not shown). In both power spectrum and spatial structure, transverse modes are strongly affected by the damping rate, while the compressional modes are not. The results shown here are also indicative of the effects of other ionospheric damping coefficients, such as d = 0.8, ...
Lecture 33: Near and Far Fields of the Resistance.
... is called radiation. Antennas for communication, radio, RADAR, microwave ovens, etc. are all based on this concept of electromagnetic radiation. One topic of further exploration that you may wish to investigate is when the plot radius r max is made very small, for example when rmax = 0.1 λ0. In such ...
... is called radiation. Antennas for communication, radio, RADAR, microwave ovens, etc. are all based on this concept of electromagnetic radiation. One topic of further exploration that you may wish to investigate is when the plot radius r max is made very small, for example when rmax = 0.1 λ0. In such ...
Lecture 1: Introduction to EM 1
... 3. [xx] next to the formula indicates units. 4. Matlab logo: ...
... 3. [xx] next to the formula indicates units. 4. Matlab logo: ...
Electromagnetically Induced Transparency
... include a transparency window at a normally highly absorbing resonance, but in addition to this, the dispersion properties of the medium are greatly enhanced. The observed effect is shown in Fig. 1. EIT allows for many new phenomenon, including efficient non-linear mixing, slow light, and lasing wit ...
... include a transparency window at a normally highly absorbing resonance, but in addition to this, the dispersion properties of the medium are greatly enhanced. The observed effect is shown in Fig. 1. EIT allows for many new phenomenon, including efficient non-linear mixing, slow light, and lasing wit ...
Nucleic Acids Research
... Qgrid web server which identifies charge and hydrophobic clusters in proteins (http://www.netasa.org/qgrid/ index.html). The Qgrid program calculates the distribution of charge and hydrophobic regions throughout the protein and applies a hierarchical clustering algorithm for clustering the atoms base ...
... Qgrid web server which identifies charge and hydrophobic clusters in proteins (http://www.netasa.org/qgrid/ index.html). The Qgrid program calculates the distribution of charge and hydrophobic regions throughout the protein and applies a hierarchical clustering algorithm for clustering the atoms base ...
Lecture-8-Optics
... a period of T = 2/. This is the case of “right-circularly polarized light”. It is often expressed as an R – state. This is a script R. ...
... a period of T = 2/. This is the case of “right-circularly polarized light”. It is often expressed as an R – state. This is a script R. ...
ppt
... – Aperture effects in physical parameters e.g. spectral type, line equivalent width. – Spectrophotometry at present (DR5) it is 10% accurate. – Spectra were not corrected against foreground extinction (e.g. using SFD map) from the pipeline (DR5). – Stellar absorptions: needed to be corrected if use ...
... – Aperture effects in physical parameters e.g. spectral type, line equivalent width. – Spectrophotometry at present (DR5) it is 10% accurate. – Spectra were not corrected against foreground extinction (e.g. using SFD map) from the pipeline (DR5). – Stellar absorptions: needed to be corrected if use ...
What makes the color pink?
... • Light comes in little particles of energy, called photons • Each wavelength has own size energy particle: ...
... • Light comes in little particles of energy, called photons • Each wavelength has own size energy particle: ...
Hubble`s Law and the Expansion Rate of the Universe
... c. Find the angular size of the galaxy using its image. The images used in this lab are negatives, so that bright objects, such as stars and galaxies, appear dark. There may be more than one galaxy in the image; the galaxy of interest is always the one closest to the center. To measure the siz ...
... c. Find the angular size of the galaxy using its image. The images used in this lab are negatives, so that bright objects, such as stars and galaxies, appear dark. There may be more than one galaxy in the image; the galaxy of interest is always the one closest to the center. To measure the siz ...
Circular dichroism
Circular dichroism (CD) is dichroism involving circularly polarized light, i.e., the differential absorption of left- and right-handed light. Left-hand circular (LHC) and right-hand circular (RHC) polarized light represent two possible spin angular momentum states for a photon, and so circular dichroism is also referred to as dichroism for spin angular momentum. This phenomenon was discovered by Jean-Baptiste Biot, Augustin Fresnel, and Aimé Cotton in the first half of the 19th century. It is exhibited in the absorption bands of optically active chiral molecules. CD spectroscopy has a wide range of applications in many different fields. Most notably, UV CD is used to investigate the secondary structure of proteins. UV/Vis CD is used to investigate charge-transfer transitions. Near-infrared CD is used to investigate geometric and electronic structure by probing metal d→d transitions. Vibrational circular dichroism, which uses light from the infrared energy region, is used for structural studies of small organic molecules, and most recently proteins and DNA.