... The models provided are: . abs - absorption of x-rays by neutral gas with solar abundances. parameter 1 = . ... parameter 2 = . ... normalization - logarithmic value of the flux density at 1 keV in units of keV cm -2 s -1 keV -1 . ... normalization - logarithmic value of the normalization of the gaussian in units of keV cm -2 s -1 . ... absorption ( params )* model ( params ) . ... A single value for the normalization (i.e., fixed normalization) will force the program to use that value. ...

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• The AstroStat Slog Blog Archive my first AAS. VI. Normalization

... Other Characteristics of the Sun: Variability of Rotation, Magnetism, Chemical Structure, Planetary System. ... Methods of Solar Magnetic Fields Measuring: Visual, Photografic, Photoelectric. ... Empiric Datas of Magnetic Fields in Photosphere, Chromosphere and Corona. ... Characteristics of Magnetic Field in Balanced Force Tubes by Potential and Forceless Field. ... Phenomenons in Active Region (Magnetic Field, Spots, Torches, Solar Prominences, Flares, Discharges. ... Magnetic Fields in Flares. ...

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• Internal Structure of Stars

... Future seminars . P a s t seminars . Seminar council . Collective processes and structures in spiral galaxies " . ... A new approach to studying global structures in thin stellar disks, which allows to describe universally both bar and spiral modes, is presented. ... Study of line-of sight velocity maps of gaseous disk in spiral galaxies allows, under some conditions, to reconstruct 3 components of gas velocity in the galactic plane. ...

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... MIPT Solid State Physics Department . ... Interacting Electrons in Normal Metals . ... The course is an introduction to interacting Fermi-particle physics and intended for future experimentalists. ... Hartree-Fock approximation. ... Linear reaction function. Calculation of density-density reaction function. Relation of density-density reaction function to compressibility of Fermi liquid and thermodynamic state density. ... Density-density reaction function of free Fermi gas in long-wave limit. ...

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• Laboratory of Real Structure of Crystals ISSP RAS
• LPCBC: Abstract 2_11
• Laboratory for Spectroscopy of Molecular Structures

... 2005 August 8 . Mars to Appear Normal This August . ... Regardless of numerous urban legends circulating, Mars will appear relatively normal in August. October is the best month to see Mars this year. ... As Earth catches up to Mars in their respective orbits around the Sun, Mars will keep rising earlier in the night. On 2005 October 30, Earth will have caught up to Mars and the planets will be the nearest to each other in their orbits -- this time around. ... About APOD | ...

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• APOD: 2001 May 1 - Antarctica Hears Little Normal Matter in the Big Bang
• APOD: December 12, 1995 - Shapley 1: An Annular Planetary Nebula
• APOD: 2001 July 24 - The Red Spider Planetary Nebula

. (a) . (b) . Figure 3. a) SEM picture of an NHEB power detector structure. The structure is fabricated by e-beam lithography and shadow metal evaporation from different angles. The absorber strip is made of normal metal (copper) and has dimensions 5x0.25x0.07 mm 3 . At right: Schematic diagram of the NHEB. b) Electrical NEP of the sensor as function of frequency measured at three substrate temperatures.

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• Simulation of a Distant Cluster of Normal Galaxies
• CSPICE Routines: NVP2PL_C
• CSPICE Routines: NVC2PL_C

Next: The Scenario Machine: Operational Up: Evolution of Magnetic Rotators Previous: Ejector-propeller hysteresis . ... The length of this segment is determined by the eccentricity. ... In this case no hysteresis occurs and transitions E -- P and the reverse take place in symmetrical points of the orbit. ... Here EP means a mixed state of the rotator at which it is in the ejector state during one part of the orbit, and in the propeller state during the rest of the orbital cycle. ...

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• Normal star evolution
• Why do Radiopulsars not Usually Form Pairs with Normal Stars?
• Contents

... Theoretical investigation was carried out of electron transport phenomena in superconducting heterostructures S-MB-N and S-MB-S with magnetic barriers (MB) determined by monolayer of ferromagnet (F) or spin-valve structures FNF or FIF (N is a normal metal, I is insulating layer). ... The I-V characteristics of cuprate bicrystal Josephson junctions have been experimentally investigated at different temperatures, barrier transparency factors and the phase difference of superconducting electrodes. ...

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• Atmospheric influence on the different radioengineering systems functioning.
• Project 6 - RFBR - Multilayer epitaxial heterostructures of high-temperature
• Project 7 - INTAS - Dynamics and non-equilibrium transport in advanced

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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• Substorm fine structure [Oulu]
• Space Physics Group of Oulu
• Solar Energetic Particles

... We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. ... Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. ... The derived temperature maps are quite similar to the ones obtained earlier with a different methods, the main differences occurring in the spot latitudes and relative strength of the spot structures....

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Next: Radio pulse characteristics Up: An overview Previous: The structure of neutron . Typically Gauss for normal pulsars . Consistent with flux conservation during stellar collapse . ... Gravity dominates stellar structure . B field dominates exterior . Stellar surface is so small that observed emission is dominated by the magnetic field. ... Only field lines inside light cylinder are closed . Particles are constrained move along field lines . ...

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• correlator:mpiscript [ATNF VLBI Wiki]
• casacore: casa::Normal Class Reference
• Basic Structure

Next: Data Structures Up: Monitor and Command Previous: Adapting MIDAS to . Three different user-levels are maintained within the MIDAS system. NOVICE (beginning MIDAS user) . ... EXPERT (expert MIDAS user) . These user-levels are set via the command SET/MIDAS_SYS user=level , . ... Help text for NOVICE- and USER- level MIDAS users is limited to the screen size of the terminal, i.e. you have to hit . ... For NOVICE- and USER- level MIDAS users the full error text is displayed. ...

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• Normalization and Fitting
• Structure of Tables
• Pre-processing the spectra

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. January 6, 1998 . The Red Spider Planetary Nebula . ... WFPC2 , HST , NASA . Explanation: Oh what a tangled web a planetary nebula can weave. The Red Spider Planetary Nebula shows the complex structure that can result when a normal star ejects its outer gases and becomes a white dwarf star . ... About APOD > . ... NASA Technical Rep.: ...

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• Sakigake
• Mechanics and Cryogenics
• suexec - Switch user before executing external programs - Apache HTTP Server

Magnetic stars, 2004, 210-211 ° Searching for the depression at 5200 A in some HgMn stars Chountonov G.A. Special Astrophysical Observatory of the Russian AS, Nizhnij Arkhyz 369167, Russia Abstract. Tens of sp ectrograms of HgMn, normal and Si stars have taned at the 1 m telescop e with a resolution of ab out 3 ° in the A ° Maitzen depressions were calculated by integration in the g 5200 A. y bands. ... It is very likely that the depression is caused by Si or rare earth elements. ...

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• http://mavr.sao.ru/hq/katya/CosmosPh/en/Abstract_Pustilnik_3.txt
• Main Researches Activities
• Laboratory of Astrospectroscopy

My research interests are focussed on the theory and modelling of accretion processes as well as star and planet formation mechanisms. I am particularly interested in the stability properties of accretion discs, the generation of MHD turbulence and associated angular momentum transport, disk - planet interactions and the origin and characteristics of jets and winds from accreting systems . ... These results have been published in Salmeron & Wardle, 2005, M.N.R.A.S., 361: 45-69. ...

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• CHIAKI's Research

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Quasi-stationary electron distributions for the different values of the particle escape time. ... The electron-cyclotron maser instability is widespread in the Universe, producing, e.g., radio emission of the magnetized planets and cool substellar objects. ... The model used takes into account the radiation escape from the source region and the particle flow through this region. ...

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• THE EVOLUTIONARY STATUS OF RCBS
• Taurid Complex
• The Evolutionary Status of RCBs

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

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• Summary of Friction
• Current Weather Conditions
• Energy From the Oceans

Next: Feature enhancement: local Up: No Title Previous: Feature enhancement: filtering . ... As a result, a common magnitude scale (contour lines on the maps above, or color scale on Fig.1) will poorly display the short-duration events in a signal. Normalizing each line of the map (fixed duration) so it has unit variance (in effect dividing the energy map by the mean energy spectrum) at each duration restores more details of small-scale activity (Fig. ...

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• Long description of how floats overlap with boxes in normal flow
• Turbulent flows
• Long description for normal flow example

... Spiral Galaxy NGC 300 . 21.08.2002 . NGC 300 is so interesting because it is so normal. ... The site is one of the premier observing locations on Earth. Earths North Magnetic Pole . ... A magnetic compass does not point toward the true North Pole of the Earth. Rather, it more closely points toward the North Magnetic Pole of the Earth. ... Asteroid 2002 NY40 will fly by planet Earth early in the morning August 18 Universal Time (late in the evening August 17 Eastern Daylight Time). ...

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... Should be broken out by telescope within a facility.) ... Should be broken out by telescope within a facility.) - # programs allocated time ­ number of programs with non- staff PI's ­ number of programs with observatory staff as PI's ­ number of thesis programs ­ number with U.S. PI's ­ number with foreign PI's ­ information on geographic distribution - # states, # institutions, characterization of institution (R1, PUI, etc), if information ...

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• http://www.naic.edu/~tghosh/now/dynspec_20_50.desc
• pdev_birdies_25jun07
• high resolution decimation test