RESUMO
Space weather phenomena can threaten space technologies. A hazard among these is the population of relativistic electrons in the Van Allen radiation belts. To reduce the threat, artificial processes can be introduced by transmitting very-low-frequency (VLF) waves into the belts. The resulting wave-particle interactions may deplete these harmful electrons. However, when transmitting VLF waves in space plasma, the antenna, plasma, and waves interact in a manner that is not well-understood. We conducted a series of VLF transmission experiments in the radiation belts and measured the power and radiation impedance under various frequencies and conditions. The results demonstrate the critical role played by the plasma-antenna-wave interaction around high-voltage space antennae and open the possibility to transmit high power in space. The physical insight obtained in this study can provide guidance to future high-power space-borne VLF transmitter developments, laboratory whistler-mode wave injection experiments, and the interpretation of various astrophysical and optical phenomena.
RESUMO
A large number (~1000) of coincident auroral far ultraviolet (FUV) and ground-based ionosonde observations are compared. This is the largest study to date of coincident satellite-based FUV and ground-based observations of the auroral E region. FUV radiance values from the NASA Thermosphere, Ionosphere, Mesosphere Energetics and Dynamics (TIMED) Global Ultraviolet Imager (GUVI) and the Defense Meteorological Satellite Program (DMSP) F16 and F18 Special Sensor Ultraviolet Spectrographic Imager (SSUSI) are included in the study. A method is described for deriving auroral ionospheric E region maximum electron density (NmE) and height of maximum electron density (hmE) from N2 Lyman-Birge-Hopfield (LBH) radiances given in two channels using lookup tables generated with the Boltzmann 3-Constituent (B3C) auroral particle transport and optical emission model. Our rules for scaling (i.e., extracting ionospheric parameters from) ionograms to obtain auroral NmE and hmE are also described. Statistical and visual comparison methods establish statistical consistency and agreement between the two methods for observing auroral NmE, but not auroral hmE. It is expected that auroral non-uniformity will cause the two NmE methods to give inconsistent results, but we have not attempted to quantify this effect in terms of more basic principles, and our results show that the two types of NmE observations are well correlated and statistically symmetrical, meaning that there is no overall bias and no scale-dependent bias.
RESUMO
The analysis of conformationally stable (conformational conservative) tetrapeptides selected from protein structures deposited in PDBSelect data bank has been fulfilled. The subset contained 943 tetrapeptide amino acid sequences and there were merely five 3D protein segment representatives for each sequence. As a result, the conclusion has been drawn on the basis of DSSP annotation analysis that in the majority of cases (900 of 943) alpha-helical conformation is obvious. Different than alpha-helix, in particular, the left-handed polyproline II helical conformation was observed in 43 sequences. The physical and chemical properties of conformationally stable peptides taken from the appropriate sample were estimated by the average hydrophobicity/hydrophilicity of tetrapeptides. The results of calculations show that the "neutrality" towards hydrophobicity/hydrophilicity is representative of conformationally stable oligopeptides. It should be noted, that dispersion of hydrophobicity/hydrophilicity distribution is sufficiently lower than for the test subsets. Thus, the conformationally stable oligopeptides present a distinct group of local protein structures which are very close with respect to conformational and physicochemical properties. In accordance with our developed theory of specific long range interactions these peptides are the objects being quite useful for effective mutual molecular recognition.