Superconducting Confined Electron Devices for Possible Application as Submillimeter Wave Detectors . ... At a normal-superconductor interface electrons undergo a charge conversion process called Andreev reflection that transforms single electrons in the normal phase into Cooper pairs in the superconducting phase 1 . ... These so-called Andreev bound states (ABS) can be regarded as standing waves formed by the reflection of electrons between the two superconducting barriers. ... A. F. Andreev, Zh. ...

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• Enhanced dust heating in the bulges of early-type spiral galaxies
• Determining dust temperatures and masses in the Herschel era: The importance of

In two previous papers we investigated in detail the formation of Hydrogen lines in high pressure dMe stellar chromospheres, constraining the possible structures over a two orders of magnitude pressure range. ... We found that when decreasing the transitoin region presure (i.e. the chromospheric temperature gradient), the Balmer lines change rapidly from emission to strong absorption, then the profiles weaken and become narrower until they disappear totally (zero H$_{\alpha}$ stars). ...

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• Armagh Observatory
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• Possible Perseid Meteor Outburst on the morning of 12 August | International

This page provides explanatory text for the dials shown on the Rice Current Solar Wind Conditions and Current Solar Wind Conditions (Dials Only) webpage. These dials use the last good received set of measurements from the Real Time Solar Wind package on the Advanced Composition Explorer (ACE) spacecraft. ... Measured) This quantity is the number of solar wind protons per unit volume as measured by the ACE Solar Wind Electron Proton Alpha Monitor (SWEPAM) . ... It is measured by ACE/SWEPAM. ...

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• Plasmasphere and plasmapause [Oulu]
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... Low-temperature kinetics of conduction electrons in metals and semiconductors. ... Basic research directions in the 6. ... 26(9), Sept. t9g3 tron-electron scattering can be singled out and measured even in nontransition metals, and so that electrons can be heated to a temperature higher than that of the Iattice not only in semiconductors but also in metals. ... In metals, nonlinearities result from the effect of the magnetic field of currents on electron trajectories and thus on the conductivity. ...

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• LPCBC: Abstract, 2_28
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• Theoretical department of ISSP RAS

ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Information & tools for observers . ... Australia Telescope Online Archive (ATOA) . ... ATCA | ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... The Australia Telescope National Facility Colloquium . ...

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• HI absorption against pulsars
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• MM Workshop Mail Exploder: other possible speakers

... X-rays are made up of photons that are emitted from stars, or quasars, or supernovae, the sun, or simply: anything that is undergoing a change either in size or temperature or giving out heat. ... in an X-ray binary star system, in which one normal star's orbit is crossed by a neutron star, when the neutron star by means of gravitational pull takes matter from the normal star X-rays form. ... Artists conception of a normal star (HDE 226868) and a black hole taking matter from the normal star. ...

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• Possible Pitfalls
• Raymond Model
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The primary purpose of KM-7 is to measure the temperature of cold electrons Te in Plasmasphere. ... The spacecraft potential can be evaluated from these measurements. ... MLT . ... Fig.1 . KM-7 measurements in MRK mode during the whole orbit 124 , 27.IX.96. ... Preliminary results . In period considered SC passed the plasmasphere at low and middle latitudes near L < 4 at heights = 8000-10000 km. At L > 4-5 and heights > 8000-10000 km SC was in auroral zone. ...

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• Plasma Physics -- History
• The Exploration of the Earth's Magnetosphere"
• Events on January 10-11, 1997 - INTERBALL observations

... NASA Lunar Orbiter . ... The Lunar Prospector is designed for a low-polar orbit investigation of the Moon, including mapping of surface composition and possible polar ice deposits, measurements of magnetic and gravity fields, and study of lunar outgassing events. Data from the 1- to 3-year mission will allow construction of a detailed map of the surface composition of the Moon, and will improve our understanding of the origin, evolution, current state, and resources of the Moon. ...

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. Latest HI Rez Visible Satellite Image . IR Enhanced Image of the PNW . (not always available - sorry) . 500 MB surface and the water vapor distribution: . Surface Pressures: . Extreme precipitation in 1995 and 1996 . Temperatures: Jan-Feb , Mar-Apr , May-Jun , July-August , Sept-Oct, Nov-Dec . Precipitation: Jan-Feb , Mar-Apr , May-Jun, July-Aug , Sept-Oct, Nov-Dec . Annual Precipitation Trends . The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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• Solar Collection and Energy Transport.

... Methane Rain Possible on Titan . ... 2.08.2006 . ... Credit Copyright: Mark Garlick (Space-art.co.uk) Explanation: Might it rain cold methane on Saturn's Titan? Recent analyses of measurements taken by the Huygen's probe that landed on Titan in 2005 January indicate that the atmosphere is actually saturated with methane at a height of about 8 kilometers. ... 2005 2006 . ... Publications with keywords: methane - Titan - Saturn . Publications with words: methane - Titan - Saturn . ...

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• Астронет > Methane Rain Possible on Titan
• GL 105C: The Coolest Star?
• Journal "Peremennye Zvezdy"

... 2006 August 2 . Methane Rain Possible on Titan . ... Explanation: Might it rain cold methane on Saturn's Titan? ... Combined with observations of a damp surface and lakes near the poles, some astrobiologists conclude that at least a methane drizzle is common on parts of Titan. ... The later scenario is depicted in the above drawing of Titan. ... About APOD | ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ... A service of: EUD at NASA / GSFC . ...

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• Medium
• APOD: 2005 August 28 Muon Wobble Possible Door to Supersymmetric Universe
• APOD: 2002 August 6 - Muon Wobble Possible Door to Supersymmetric Universe

... We present the results of recent pulsar observations at frequencies between 27.9 GHz and 34.8 GHz, i.e. in a wavelength range of 10.75 mm to 8.61 mm, made with the Effelsberg radiotelescope. The measured flux densities of two out of nine detected pulsars suggest that the spectrum flattens at high frequencies or even shows a turn-over. ... In this work we will only focus on pulsar spectra. ... Figure 4: Derived spectra of the second strongest pulsar observed at mm-wavelengths. ...

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• OptInt PmWiki : MROIFastTipTilt / Tech Meet 11

... We computed the permanently shadowed areas and temperatures inside the craters for the variation of the position of the lunar pole of rotation with respect to the ecliptic pole with a period of 18.6 years. ... According to our results, the total permanently shadowed area in the polar craters of the Moon is equal to 50428.7 km2, or 0.13% of the total area of the lunar surface [3]. ... The area of permanently shaded part of a crater makes 59 % from all area of a crater [3]. ...

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Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...

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• East Siberian Center for the Earth's Ionosphere Research. Capabilities and

... For every level we have plotted the dependence between width and Lande factor and obtained the linear regression parameters: the inclination, the zero Lande factor line width and the correlation. ... Fig. 1. presents a model components, the intensity of which decreases (b) line with 10 and increases (c) to the center of spectral line (the field is 12 k6s). ... Our results show strong dependencies of line width on the level of width measurements. ...

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• http://mavr.sao.ru/hq/lizm/conferences/pdf/1991/1992_2_p12-p16.pdf
• http://mavr.sao.ru/hq/lizm/conferences/pdf/1987/1987_p6-p9.pdf
• http://mavr.sao.ru/hq/katya/CosmosPh/en/Abstract_Pustilnik_3.txt

The HTSC group has an access to a set of technological equipment for thin film preparation and laboratory measurement system for low temperature electrical measurements. The technological complex of the " Thin Film Oxide Electronics " Laboratory includes two clean rooms of the "1000" class, with a complete set of equipment for photolithography (spinner, oven, hot plate, mask aligner, chemical bench, de-ionized water source) in each clean room. ...

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• Lab234 - Design, fabrication and experimental studies of a novel device: Cold
• Project 1 - SfP - Ovsyannikov, Supersensitive high-Tc superconducting
• Project 4 - RFBR - Stepantsov, Determination of the space anisotropy of order

The low aspect ratio, or spherical tokamak Globus-M [1] has recently been built in a support of international spherical tokamak plasma investigation program. ... The survey to determine the work scope in diagnostic design for Globus-M is given in the paper. ... The next one is an advanced diagnostic set intended to supply the data on basic plasma parameters: electron temperature and density profiles, ion temperature, plasma composition, radiation profile, Zeffective. ... Magnetic Diagnostics. ...

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EXPLANATION OF DANA'S FIBER TESTS ON THE 12M TELESCOPE.. ... But we know full well that this is not directly possible- the delay in the optical fiber carrying this signal will change both with temperature and to some degree with fiber bending as the telescope tracks objects or moves from one object to another. ... So we would like to identify at least one pair of single mode fibers in our bundle, whose delay changes due to antenna tracking etc are pretty well matched. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/JensentagR2257tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/JensentagR2257tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/NicollstagT2211tp.pdf

National Space Agency of Ukraine and . ... The Second International Meeting on WARNING Mission . ... Space Research Institute of Ukrainian National Academy of Sciences - National Space Agency, . ... The Head of Scientific committee of the Project “Warning” is DR V.G.Bar`yahtar, Academitian of Ukrainian National Academy of Sciences. ... Lviv Center Space Research Institute of Ukrainian National Academy of Sciences, . ... National Space Agency of Ukraine, Bozhenka St. 11, 252022 Kyiv-22, Ukraine. ...

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• SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM
• WARNING MISSION: Background
• ENERGOSPECTROMETER OF IONOSPHERIC PLASMA P3-3

... In the first page of this chapter, Eddington computes an effective temperature of 3.18 K, but this has nothing to do with the 2.725 K blackbody spectrum of the Cosmic Microwave Background (CMB) . Here is a quote of what Eddington actually said: . ... We shall first calculate the energy density of this radiation. ... It is clear that Eddington's model fits the optical data, but that Eddington did not anticipate either the CMB (red curve) or the interstellar dust (ISD, green curve). ...

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• Possible Graphical Verifications
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