LCVR Temperature : 26.98 Celsius : 24/ Apr / 2014 17:59:05.134 LCVR #1 ( Channel 3) : 2.0210 : LCVR #2 ( Channel 4) : 2.0500 : [ stored ] : 24/ Apr / 2014 17:59:05.141 LCVR #1 ( Channel 3) : 2.0210 : LCVR #2 ( Channel 4) : 2.0500 : [ stored ] : 24/ Apr / 2014 17:59:05.294 LCVR #1 ( Channel 3) : 2.0210 : LCVR #2 ( ...

Next: Limiting Energy Channels Input Up: *fit* - Fit Data Previous: Raymond Model . The model is a two-temperature Raymond thermal spectrum, low temperature range is 0.55 to 0.65 keV, high temperature range is 1 to 2 keV, element abundance table is cosmic, abundance of heavy elements (atomic number >2 ) is 50% of the value in the table. Note that 0.7 = log(5.0), specifies that the second component normalization will be 5 times the normalization of the first component. ...

... Next, consider a more elaborate UBVRI photometer with two channels (a ``red'' and a ``blue'' tube). We suppose it has separate filter wheels in the two beams; the first filter wheel contains the UBV filters, and the second has the R and I filters. ... If the filter wheels had been in series instead of in separate beams, the unused wheel would have to be set to a clear position, instead of the ``any'' entered in the first five lines of Table . ...

The .out files contain the data displayed in plots of the wide spectral scans of High-CAL and the respective bets-fits obtained. Each of the 14 pipelines has a separate file. What to expect inside this file ? ... These files are made available for interested people to download. ... Note: Since the measurements for the beam0-pol_1, beam 5 (both pol.s) were missed from the set on tJD:53228 (due to the pre-amp and WAPP problems respectively), the corresponding fits & .out files missing. ...

Instrument Science Report WFC3 2002-05 Internal background and dark current of the IR channel of WFC3 in ambient conditions _______________________ Massimo Stiavelli June 4, 2002 ____________________________________________________________________________ Abstract During the ground testing of WFC3 it may be desirable to operate the IR channel enclosure at ambient temperature. ... Detector dark current Table 2 : dark current as a function of temperature according to three different models. ...

Number of spectral channels . ... Spectral channels MSU-SK #1 (#2): . ... 0,54-0,60 (0,54-0,59) µm . ... Ground Resoultion I-IV/V channels . ... Scanning Rate I-IV/V channels . ... Radiation Temperature Measurement Range in Channel V . ... Instrument Error for Radiation Temperatute Measurement in Channel V . ... Ground resolution corresponds to normal flihgt altitude 650 km. For more information send a mail to: info@sputnik.infospace.ru . ...

RATAN-600 Radiometer = 6.3 cm . ... 4.8 GHz . ... Physical temperature . ... System noise temperature . ... 2.2 mK . ... Noise Added Radiometer . Operating mode . Single - beam mode . ... left circular . and right circular . ... Noise generator . ...

INFRARED FOURIER-SPECTROMETER SICH-F . ... Instrument work regimes: 1) Inside. 2) Calibration at inside standard sources 2 - 4 times per a rotation. 3) Calibration at "free space" 2 - 4 times per a rotation. 4) Infrared radiation measuring 10 - 40 min. per a rotation. ... Spectrometer consists of the photodetector block and the block of signal processing and control. ... Diagnostic information and attach data will transfer by state telemetric channels. ... Detector temperature. ...

... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...

Sun Dance . ... Credit Copyright: A. Title ( Stanford Lockheed Institute ), TRACE , NASA Explanation: Hot gas dances across the surface of the Sun in this picture from the orbiting TRACE satellite . The temperature of the gas is color coded so that blue represents hundreds of thousands of Kelvin , while red represents extreme temperatures in the millions of Kelvin. Hot gas is channeled into lanes ordered by the Sun's chaotic magnetic field . ... NASA Official: Jay Norris. ...

Recent Changes - Search : . ... Basic Editing . ... edit SideBar . ... Go to new wiki . History . ... LBAMay2012 / . SRCP into channels 1-4, SCLP is channels 5-8 . ... dbbcifa=3,agc,2 . dbbcifb=2,agc,2 . ... Systemp temperature measurements are kludged in - SRCP is logged as tsysS and SLCP is logged as tsysX . ... Edit - History - Print - Recent Changes - Search . ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... First three columns show base-difference images of the evolution of the wave in 3 EUV channels (211 , 193 , 171 ) of AIA in which the wave is clearly visible. ... From our study we have quantitatively confirmed previous results that during wave passage the plasma visible in the Atmospheric Imaging Assembly (AIA) 171 channel is getting heated to higher temperatures corresponding to AIA 193 and 211 channels. ...

All stars derive their energy through the thermonuclear fusion of light elements in to heavy elements. High temperatures are required so that the mutual electrostatic repulsion of the protons in each fusing atomic nucleus is overcome. ... Elements with more protons in their nuclei require higher temperatures. ... This sequence is now shown in the animation below. ... First Step of the Proton-Proton Chain Narration . Second Step of the Proton-Proton Chain Narration . ...

. Next: Diameters Up: Stellar parameters from calibrations Previous: Gravities Contents . Temperatures of stars are derived from their spectral type and luminosity class. Calibrations are stored in files spec_par.V, spec_par.IV, spec_par.III, spec_par.II, spec_par.I in oyster/starbase . teff_stars Compute effective temperature for all stars in startable. teff_star ( spectrum _char ) Function. Return effective temperature for star with specified spectrum. Christian Hummel 2015-04-28

... 2013 July 31 . 130 Years of Earth Surface Temperatures . Image Credit: GISS , NASA . Explanation: How has the surface temperature of Earth been changing? ... On average, the display demonstrates that the temperature on Earth has increased by nearly one degree Celsius over the past 130 years, and many of the warmest years on record have occurred only recently. ... About APOD | ... NASA Official: Phillip Newman Specific rights apply . NASA Web Privacy Policy and Important Notices . ...

... Gallery . Simulation Images . Simulations of convection in stars . Side-view of the temperatures in a simulationтАж . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . ... Title: Side-view of the temperatures in a simulation of a white dwarf . ... NOTE: All images are copyright and must not be reproduced or mirrored in any form without written permission. ... Side-view of the temperatures in a simulation of a white dwarf €йRegner Trampedach . ...

STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Remote Sensors . ... TS34C-M Wireless long range remote temperature sensor . ... Wireless long range remote temperature sensor #TS34C-M. Reads outdoor temperature in degrees Fahrenheit as well as humidity and transmits up to 328 feet (100 meters). ...

... A. M. Neminsky, P. N. Nikolaev, and D. V. Shovkun . ... The temperature dependence of the magnetic field penetration depth lambda ( T ) is determined down to 0.2 T c by the ac-susceptibility measurements on the Rb 3 C 60 fine powder with small, about 1 K, variation in the grains' superconducting transition temperatures. The lambda ( T ) temperature dependence is exponential at low temperatures, which allows us to determine the energy gap Delta 0 =1.7 k B T c . ...

... the PI of the experiment SPECTRO - multi-detector low energy particle measurements (energy, angle and ion mass spectra); . Yuri I. Galperin , Space Research Institute (IKI) of Russian Academy of Sciences, Moscow, Russia, . ... Vladimir A. Gladyshev , Space Research Institute (IKI) , Moscow, Russia, . ... Rostislav A. Kovrazhkin , Space Research Institute (IKI) , Moscow, Russia, . ... Alexander K. Kuzmin , Space Research Institute (IKI) , Moscow, Russia, . ... Back to the Arcad-3 Home Page ...

Operating of the superconducting integrated receiver channel of the TELIS atmospheric sounder. ... The noise temperature of the SIR was measured to be as low as 120 K, with an intermediate frequency band of 4 ­ 8 GHz in double sideband operation; the spectral resolution is well below 1 MHz. The SIR was implemented in the three-channel balloon-borne instrument TELIS (TErahertz and submillimeter LImb Sounder) that detects spectral emission lines of stratospheric trace gases (like ClO and BrO). ...