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http://www.cplire.ru/html/lab234/Tarasov/reprints/PhysicaC2002p444.pdf.

1. Space Weather Dials Interpretation Guide
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. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/ISTP/dialinterp.html -- 8.1 Кб -- 21.12.2007
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2. http://www.naic.edu/~phil/calcb/meascalMay03/meascalMay03.html
16may03 The hcorcal measured values: . ... The power levels during the measurements. ... The ratio of the other cals to the hcorcal: New diodes were installed on the cband system on 22apr03. On 25apr03 the cals were measured using absorber and tracking blank sky. ... After this the "other cals" were measured relative to the hcorcal while tracking blank sky. ... The ratio of the "other" cals was then computed relative to the hcorcal (see measuring cals on the telescope using sky and absorber ). ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/calcb/meascalMay03/meascalMay03.html -- 9.1 Кб -- 01.03.2006
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3. Optical constant database - Level: measurement/paper
... Optical constants of Fe 2 O 3 in the infrared spectral region. ... Optical constants: . amorphous Fe 2 O 3 . ... The Reflectance of polarized radiation at the incidence angle 12 deg was measured in the range from 1400 to 200 cm -1 for monocrystalline hematite (alpha-Fe 2 O 3 ) and amorphous Fe 2 O 3 samples. Special technique applied allowed to reduce the relative errors downto 1% for the reflectance values of 0.005-0.8. The optical constants were obtained by the Kramers-Kronig method. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/JPDOC/PAPERS/4-pop73.html -- 2.8 Кб -- 19.11.2010
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4. Atmospheric opacity and system temperature
Next: Antenna gain considerations and Up: Some Theory Previous: Polarisation . To provide correct flux density units for the visibilities, , from an interferometer, the measured correlation coefficient at the correlator ( ) needs to be scaled by a system temperature and a telescope sensitivity factor ( ). ... For a zenith opacity , observing at an elevation of , and if the atmosphere is approximated as having a uniform temperature , then the atmospheric contribution to system temperature is . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/userguide/node79.html -- 7.8 Кб -- 10.04.2016
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5. http://www.cplire.ru/html/lab234/pubs/2014_05.pdf
... 2*1018 /1/2, , 0.1 , 1.6 , 1 350 , 100 , 5*10 20 - 3. 10-100 10-100 , . ... Integrated structures comprising cold electron bolometers and twin-slot antennas have been studied in the temperature range 0.06-3 K. Dynamic resistance ratio and optical response was measured for 2-15 K black body radiation temperature. ... 12000 290 10000 RR Te 280 Electron temperature, mK 270 Resistance ratio, Rd/Rn 8000 260 250 6000 240 4000 230 220 210 0 50 100 150 200 250 300 2000 Phonon temperature, mK 3. ... 0.1 . ...
[ Текст ]  Ссылки http://www.cplire.ru/html/lab234/pubs/2014_05.pdf -- 1059.3 Кб -- 21.03.2016
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6. http://selena.sai.msu.ru/Symposium/ir_luna_e.pdf
THE THERMAL RADIATION OF THE LUNAR SURFACE IN THE IR RANGE OF THE SPECTRUM (10-12 µm). ... 0.80 0.60 0.40 0.20 0.00 -0.20 -0.40 -0.60 -0.80 -0.80 -0.60 -0.40 -0.20 0.00 0.20 0.40 0.60 0.80 Fig.1 0.80 0.60 0.40 0.20 0.00 -0.20 -0.40 -0.60 -0.80 -0.80 -0.60 -0.40 -0.20 0.00 0.20 0.40 0.60 0.80 Fig.2 0.60 0.40 0.20 -0.00 -0.20 -0.40 -0.60 -0.60 -0.40 -0.20 -0.00 0.20 0.40 0.60 0.80 Fig.3 Indicatrix of the thermal radiation of the Moon (10.5-12.5 µ). ...
[ Текст ]  Ссылки http://selena.sai.msu.ru/Symposium/ir_luna_e.pdf -- 308.5 Кб -- 06.10.2008
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7. STIS CCD Detector - Living with Radiation Damage
... STIS . ... In a space environment, CCD detectors accumulate radiation damage, which over time leads to increasing dark current, more hot pixels, and reduced charge transfer efficiency. After twelve years on orbit, the effects of such radiation damage on the STIS CCD have become substantial. ... Since in a CCD, charge must be transferred many times before reaching the readout register, even a small decrease in CTE can have a large effect on the measured count rate near the center of the detector. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/stis/documents/newsletters/full_stories/0909_CCD_radiation_dam.html -- 23.2 Кб -- 12.04.2016
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8. S.P.Korolev RSC Energia - ECOLOGICAL MONITORING
... RADIATION AND ECOLOGICAL MONITORING . ... OF MEASURING CHANNELS . Parameters of ecological fields measured by ARES . Parameter measured, . ... Volumetric activity of gases radionuclides in the air, Bq/m 3 : . ... of inert gases . ... Volumetric activity of a- and b-active aerosols, Bq/m 3 : . ... Concentration of nitric oxide NO, mg/m 3 . ... Meteorological parameters measured by ARES . ... 0.5 + 0.05 V), where V - measured wind velocity . ... Official WEB-site of S.P.Korolev RSC Energia . ...
[ Сохраненная копия ]  Ссылки http://www.energia.ru/eng/conversion/ecology/radiation-02.html -- 13.8 Кб -- 02.10.2012
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9. http://www.mrao.cam.ac.uk/~graca/talks/PhiSky_Rocha.pdf
Constraints on the variation of the fine structure constant from recent CMB measurements Graca Rocha Cavendish Astrophysics, University of Cambridge October 22, 2003 Recent CMB experiments such as Boomerang, MAXIMA, DASI, CBI, VSA among others and most recently WMAP seem to validate, apar t some intriguing discrepancies, the so-called concordance model of cosmology. ... DASI and WMAP detected the polarization of the CMB via the temperature polarization (scalar E-mode) cross power-spectrum (TE). ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~graca/talks/PhiSky_Rocha.pdf -- 1078.8 Кб -- 27.09.2004
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10. The AstroStat Slog Blog Archive Differential Emission Measure [Eqn]
... Archives . ... Magnitude [Eqn] . ... Differential Emission Measures (DEMs) are a summary of the temperature structure of the outer atmospheres (aka coronae) of stars, and are usually derived from a select subset of line fluxes. ... is called the Differential Emission Measure and is a very useful summary of the temperature structure of stellar coronae. ... Tags: DEM , Differential Emission Measure , EotW , Equation , Equation of the Week , stellar coronae . ... Comment ( RSS ) | ... Chandra Blog . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2008/eotw-dem/index.html -- 24.3 Кб -- 01.03.2014
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11. Phys. Rev. Lett. 72, 3092 (1994): Neminsky et al. - Temperature dependence of
... 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 . ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lek/shovkun/abs10.html -- 2.7 Кб -- 22.05.2004
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12. ENERGOSPECTROMETER OF IONOSPHERIC PLASMA P3-3
ENERGOSPECTROMETER OF IONOSPHERIC PLASMA P3-3 . ... The major objective of the P3-3 experiment is complex investigation the main parameters of ionospheric plasma with high time and spatial resolution. ... Measured parameters: . ... The experiment produce regular data - measured with fixed time interval and «packet» data - measured once per specific time interval and producing blocks of TM-information. ... If all parameters will be measured once per second, the experiment will produce 10 MB per orbit. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/projects/warning/p3-3.html -- 6.2 Кб -- 15.02.2000
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13. http://www.mso.anu.edu.au/~brian/A3002/probset1.pdf
... Problem 5. ... See figure 1 for the light curve of these narrow Nitrogen lines. ... Figure out the behaviour of each parcel of gas, and then add them all up to find the light curve. 5.4 (3pts) Using expression from problem 5.2, derive the expression for the time after SN explosion date, when the first light from the ionised ring reaches Earth. Using the expression from problem 5.2, derive the expression for the time after SN explosion date when the maximum brightness of the ring occurs. ...
[ Текст ]  Ссылки http://www.mso.anu.edu.au/~brian/A3002/probset1.pdf -- 262.1 Кб -- 02.09.2009
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14. KM-7 Results Page
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. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/auroral/km7.htm -- 3.9 Кб -- 26.11.1996
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/auroral/km7.htm -- 3.9 Кб -- 26.11.1996
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15. Radiation Damage
. Previous slide . Next slide . Back to first slide . View graphic version .
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/Appendix/Agenda/tsld002.htm -- 2.1 Кб -- 12.12.2000
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16. Eddington's Temperature of Space
... 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). ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/~satr/cosmo/Eddington-T0.html -- 7.3 Кб -- 16.10.2000
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17. Archeops Main Page
The Archeops experiment aimed at measuring the cosmic background emitted just after the Big Bang. The study of this radiation is essential to obtain precise information on the evolution of the Universe: density, Hubble constant, age of the Universe.. To achieve this goal, measurements have been done with devices cooled down at 100mK temperature placed at the focus of a warm telescope. ... 28960 visitors . ...
[ Сохраненная копия ]  Ссылки http://www.archeops.org/ -- 6.8 Кб -- 09.04.2016
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18. Seminars
The seminar is supported by the grant of Federal Programm "Integration" . ... Measuring the Hubble Constant from Reverberating Accretion Discs in AGNs . We show how wavelength-dependent time delays between continuum flux variations of active galactic nuclei (AGNs) can be used to test the standard black hole--accretion disc paradigm, by measuring the temperature structure T(R) of the gaseous material surrounding the purported black hole. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/sciwork/archive/49/eannot1.html -- 3.3 Кб -- 30.08.1999
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19. Figure 7
Figure 8a. The cooling of the right, bottom secondary support rod is shown for a night in May of 1996. An accurate time of the enclosure opening is not known, but is thought to have been within 15 minutes of the first data point shown in this graph. The squares show the temperature of the ambient air at the time of the rod measurements. ... M3 is the time constant of the exponential fit in units of inverse seconds. Converting to hours gives a time constant of 1.03 hours . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/users/morgan/APO/SH_measurements/altitude.sweeps/aug.14-15.00/graphics/Fig8.html -- 3.6 Кб -- 29.03.2003
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20. Таблица основных физических величин
... RECOMMENDED VALUES OF PHYSICAL CONSTANTS AND CONVERSION FACTORS. ... This reference must be included when these constants are used in a context where their full accuracy is important. ... elementary charge (of proton) . ... gravitational constant . ... unified atomic mass constant . ... of electron . ... of proton . ... Planck constant . ... Rydberg constant, m 0 2 m e e 4 c 3 /8h 3 . ... fine structure constant, m 0 e 2 c/2h . ... Bohr radius, h 2 ( pm 0 c 2 m e e 2 ) . ... Bohr magneton, e h /2m e...
[ Сохраненная копия ]  Ссылки http://www.scientific.ru/refdat/cohen.html -- 10.8 Кб -- 10.03.2011
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