The gravitational and
microwave measurements in particular could soon reveal just how far the Spot extends into Jupiter — whether it floats like an iceberg near the top of the atmosphere, or instead bores deep into the planet's innards.
By the time NASA restarted its passive -
microwave measurements in 1978, the hole had vanished.
Not exact matches
It is important to understand that using your
microwave oven will expose you to an energy density of milliwatts per square centimeter (the standard energy unit
measurement in the U.S.).
Microwave safe, hypo allergenic and dishwasher friendly, this translucent silicone sleeve allows you to see
measurements and liquid
in the bottle.
In 2000, the observation moved beyond a reasonable doubt, thanks to
measurements of
microwave radiation that rippled out from the original Big Bang.
NASA began taking passive -
microwave measurements of sea ice
in 1972, using an instrument aboard its Nimbus - 5 satellite.
FIFTY years ago, on 20 May 1964, Arno Penzias and Robert Wilson of the Bell Telephone Laboratories
in Holmdel, New Jersey, recorded their first astronomical
measurements of
microwave radiation from the supernova remnant Cassiopeia A.
«
In many parts of the world
microwave measurements systems can become a complement to CT scans and other imaging systems, which are often missing or have long waiting lists.»
«Precise
measurements of cosmic
microwave radiation reveal minute differences
in temperature.
Results from a clinical study demonstrates that
microwave measurements can be used for a rapid detection of intracranial bleeding
in traumatic brain injuries.
«The result indicates that the
microwave measurements can be useful
in ambulances and
in other care settings.»
There were even some hints of such «anisotropy»
in the early 2000s, when
measurements from NASA's Wilkinson
Microwave Anisotropy Probe (WMAP) spacecraft suggested that some subtle undulations
in the motley CMB appeared to line up along a so - called «axis of evil» — which most researchers discount as a statistical fluke.
Based on
measurements of the expansion using Type Ia supernovae,
measurements of temperature fluctuations
in the cosmic
microwave background, and
measurements of the correlation function of galaxies, the universe has a calculated age of 13.7 ± 0.2 billion years.
In contrast, the Scripps team opted to directly correlate albedo
measurements made by NASA's CERES instrument data with observations of sea ice extent made by the Special Sensor
Microwave Imager (SSM / I) radiometers aboard Defense Meteorological Satellite Program satellites.
In 2007 researchers saw hints of that pattern in preliminary measurements from NASA's Wilkinson Microwave Anisotropy Probe (WMAP
In 2007 researchers saw hints of that pattern
in preliminary measurements from NASA's Wilkinson Microwave Anisotropy Probe (WMAP
in preliminary
measurements from NASA's Wilkinson
Microwave Anisotropy Probe (WMAP).
And Yoon and Ham applied an electric field at a
microwave frequency, which allows for the direct
measurement of the electrons» collective acceleration
in the form of a phase delay
in the current.
Since 2003, WMAP researchers have made more precise energy
measurements of the
microwaves that allow them to look farther back
in time.
Measurements of Jovian gravity suggest that Jupiter's core is large and diffuse, and
microwave views show that ammonia wells up to the cloud tops from deep
in the atmosphere (SN: 6/24/17, p. 14).
Measurements based on the cosmic microwave background, the earliest light in the universe, suggest one rate of expansion, while measurements of nearby supernovas suggest a
Measurements based on the cosmic
microwave background, the earliest light
in the universe, suggest one rate of expansion, while
measurements of nearby supernovas suggest a
measurements of nearby supernovas suggest a faster one.
With the help of EDMR, electrically detected magnetic resonance, an ultrasensitive method of
measurement, they were able to determine the local defects» structure by detecting their magnetic fingerprint
in the photo current of the solar cell under a magnetic field and
microwave radiation.
* Correction, 26 August, 12:25 p.m.: The story has been updated to reflect that
in the photo of Weiss at the lab bench, he is working on equipment for
measurements of the cosmic
microwave background.
All of these
measurements were conducted with spectrometers built exclusively
in the Ziurys group, which includes three mm / sub - mm / THz direct absorption spectrometers and one Fourier transform
microwave / mm instrument.
Previously, the most precise test of cosmological models came from
measurements with the European Space Agency's Planck satellite of what is known as the cosmic
microwave background (CMB)-- a faint glow
in the sky emitted 380,000 years after the Big Bang.
«Along with the
microwave radiometer
measurements, which have also shown surprises
in the deep atmosphere, these results demonstrate that if we want to understand giant planets, we will need to study all of Jupiter,» Levin says.
While there remain disparities among different tropospheric temperature trends estimated from satellite
Microwave Sounding Unit (MSU and advanced MSU)
measurements since 1979, and all likely still contain residual errors, estimates have been substantially improved (and data set differences reduced) through adjustments for issues of changing satellites, orbit decay and drift
in local crossing time (i.e., diurnal cycle effects).
Group 1: Materials, Resonators, & Resonator Circuits A. Fundamental Properties of Materials B. Micro - and Macro-Fabrication Technology for Resonators and Filters C. Theory, Design, and Performance of Resonators and Filters, including BAW, FBAR, MEMS, NEMS, SAW, and others D. Reconfigurable Frequency Control Circuits, e.g., Arrays, Channelizers Group 2: Oscillators, Synthesizers, Noise, & Circuit Techniques A. Oscillators — BAW, MEMS, and SAW B. Oscillators -
Microwave to Optical C. Heterogeneously Integrated Miniature Oscillators, e.g., Single - Chip D. Synthesizers, Multi-Resonator Oscillators, and Other Circuitry E. Noise Phenomena and Aging F.
Measurements and Specifications G. Timing Error
in Digital Systems and Applications Group 3:
Microwave Frequency Standards A.
Microwave Atomic Frequency Standards B. Atomic Clocks for Space Applications C. Miniature and Chip Scale Atomic Clocks and other instrumentation D. Fundamental Physics, Fundamental Constants, & Other Applications Group 4: Sensors & Transducers A. Resonant Chemical Sensors B. Resonant Physical Sensors C. Vibratory and Atomic Gyroscopes & Magnetometers D. BAW, SAW, FBAR, and MEMS Sensors E. Transducers F. Sensor Instrumentation Group 5: Timekeeping, Time and Frequency Transfer, GNSS Applications A. TAI and Time Scales, Time and Frequency Transfer, and Algorithms B. Satellite Navigation (Galileo, GPS,...) C.Telecommunications Network Synchronization, RF Fiber Frequency Distribution D. All - optical fiber frequency transfer E. Optical free - space frequency transfer F. Frequency and Time Distribution and Calibration Services Group 6: Optical Frequency Standards and Applications A. Optical Ion and Neutral Atom Clocks B. Optical Frequency Combs and Frequency
Measurements C. Ultrastable Laser Sources and Optical Frequency Distribution D. Ultrastable Optical to
Microwave Conversion E. Fundamental Physics, Fundamental Constants, and Other Applications
Painstaking
measurements of the cosmic
microwave background — the omnipresent radiation that is the afterglow of the Big Bang — tells us that a sixth of all matter
in our galaxy is ordinary, while the rest is dark matter.
In this lecture, George Efstathiou will describe how recent
measurements of the cosmic
microwave background radiation made with the Planck Satellite can be used to answer these questions and to elucidate what happened within 10 - 35 seconds of the creation of our Universe.
In addition to the
microwave measurement, this device enables transforming quantum information from one frequency to another while simultaneously amplifying it.
``... The MSUs are cross-track scanners with
measurements of
microwave radiance
in four channels ranging from 50.3 to 57.95 GHz on the lower shoulder of the Oxygen absorption band.
(1)
In addition to the data of the near - surface temperatures, which are composed of measurements from weather stations and sea surface temperatures, there is also the microwave data from satellites, which can be used to estimate air temperatures in the troposphere in a few kilometers altitud
In addition to the data of the near - surface temperatures, which are composed of
measurements from weather stations and sea surface temperatures, there is also the
microwave data from satellites, which can be used to estimate air temperatures
in the troposphere in a few kilometers altitud
in the troposphere
in a few kilometers altitud
in a few kilometers altitude.
While there remain disparities among different tropospheric temperature trends estimated from satellite
Microwave Sounding Unit (MSU and advanced MSU)
measurements since 1979, and all likely still contain residual errors, estimates have been substantially improved (and data set differences reduced) through adjustments for issues of changing satellites, orbit decay and drift
in local crossing time (i.e., diurnal cycle effects).
All these sensors make
measurements at critical frequencies at and above 85 gigahertz (GHz); sensors measure
microwave emissions at 183 GHz, the signature frequency band emitted by water vapor, making it feasible to detect frozen hydrometeors (snow, ice, and the like)
in the atmosphere.
Motivated primarily by Mitchum's conclusion, Keihm et al., 2000 (Abstract; Google Scholar access) actively tried to come up with something that could cause a «drift»
in the satellites, and eventually decided that a temporary problem
in the «TOPEX
Microwave Radiometer path delay
measurements», which stopped
in December 1996 could do that.
This new product, however, exploits direct broadcast (DB) capability from several satellites
in low Earth orbit that make
microwave measurements over the continental United States and Alaska.
• the factors that contribute to uncertainties
in the trends inferred from three categories of instrumental
measurements —
Microwave Sounding Units (MSU) carried aboard National Oceanic and Atmospheric Administration (NOAA) satellites, radiosondes, and surface observations;
Microwave radiometers are a passive
measurement technique; that is, they monitor Earth's own heat energy emissions
in the 1 - to 200 - gigahertz frequency range.
Temperatures aloft can be measured
in a number of ways, two of which are useful for climate monitoring: by radiosondes (balloon - borne instrument packages, including thermometers, released daily or twice daily at a network of observing stations throughout the world), and by satellite
measurements of
microwave radiation emitted by oxygen gas in the lower to mid-troposphere, taken with an instrument known as the Microwave Sounding Unit (MSU).5 The balloon measurements are taken at the same Greenwich mean times each day, whereas the times of day of the satellite measurements for a given location drift slowly with changes in the satellit
microwave radiation emitted by oxygen gas
in the lower to mid-troposphere, taken with an instrument known as the
Microwave Sounding Unit (MSU).5 The balloon measurements are taken at the same Greenwich mean times each day, whereas the times of day of the satellite measurements for a given location drift slowly with changes in the satellit
Microwave Sounding Unit (MSU).5 The balloon
measurements are taken at the same Greenwich mean times each day, whereas the times of day of the satellite
measurements for a given location drift slowly with changes
in the satellite orbits.
Plus, they are inherently a much less direct
measurement of temperature: they actually measure
microwave brightness, which must be mathematically processed to arrive at temperatures at various altitudes
in the atmosphere.
Except when satellites are inferring temperature from
microwave sounding units,
in which case the fixed locations on the surface taking direct
measurements with thermometers have had their real data manipulated to achieve a desired result.
For practical purposes, SSTsubskin can be well approximated to the
measurement of surface temperature by a
microwave radiometer operating
in the 6 - 11 GHz frequency range, but the relationship is neither direct nor invariant to changing physical conditions or to the specific geometry of the
microwave measurements.
In the original configuration of NPOESS, the ocean surface vector wind data record established by QuikSCAT was to be replaced by passive
microwave measurements of wind speed and direction by the polarimetric CMIS radiometer.
Lin, B., B. Wielicki, P. Minnis, and W. Rossow, 1998: Estimation of water cloud properties from satellite
microwave, infrared and visible
measurements in oceanic environments: 1.
From the beginning, there were serious concerns within the scientific community (both research and operational) about the viability of passive
microwave measurements of ocean surface vector winds, especially
in storms and
in other areas of rain and large amounts of cloud liquid water.
QuikSCAT
measurements are also limited to a spatial resolution of 12.5 km and are not routinely made closer than about 30 km from land.26 Many
in the
microwave breakout group argued that high priority should be given to a sustained, more capable, next - generation scatterometer program that can meet these requirements while at the same time continuing the ocean surface vector winds CDR established by QuikSCAT.
Some participants expressed concern that a capability for passive
microwave precipitation
measurements may not emerge
in the revised MIS sensor, and they suggested that NPOESS place emphasis on the water cycle (water vapor, liquid water, ice water, and precipitation) when considering MIS requirements, possibly including giant magneto - impedance (GMI) bands.
Prigent, C., F. Aires, W.B. Rossow, and A. Robock, 2005: Sensitivity of satellite
microwave and infrared observations to soil moisture at a global scale: Relationship of satellite observations to
in situ soil moisture
measurements.
This study uses satellite radiation budget
measurements along with satellite
microwave sea ice data to document the Arctic - wide decrease
in planetary albedo and its amplifying effect on the warming.
With respect to ongoing research, I wonder if a series of high - resolution
measurements in the 53 - 57 GHz band from an airborne
microwave spectrometer (vertical looking up, vertical looking down and horizontal) under measured conditions of temperature, pressure and humidity might allow improved deconvolution of the satellite data.
«Satellites are not a thermometer
in space, they're not making direct
measurements of atmospheric temperature, they're measuring the
microwave emissions from oxygen molecules,» Santer said.