Polarization and brightness temperature observations of Venus with the GMRT [PDF]
Venus was observed at frequencies of 1297.67 MHz (23 cm), 607.67 MHz (49 cm) and 233.67 MHz (1.28 m) with the Giant Metrewave Radio Telescope (GMRT) during the period of 25th July and 6th September 2015 when it was close to its inferior conjunction. Values of the brightness temperature (Tb) of Venus from these observations were derived as 622{\pm}43 K,
Nithin Mohan +3 more
openaire +2 more sources
brightness temperature data of Balmer-Kapteyn Region
The zip file includes the raw Brightness temperature (TB) data, and the processed TB, normalized TB (nTB), TB difference (dTB) of Balmer-Kapteyn ...
Tang,Tianqi
core +1 more source
Analysis of SMOS brightness temperature and vegetation optical depth data with coupled land surface and radiative transfer models in Southern Germany [PDF]
Soil Moisture and Ocean Salinity (SMOS) L1c brightness temperature and L2 optical depth data are analysed with a coupled land surface (PROMET) and radiative transfer model (L-MEB).
F. Schlenz +3 more
doaj +1 more source
METHOD OF THE ATMOSPHERE BRIGHTNESS TEMPERATURE MEASURING AT FREQUENCIES AROUND 100 GHZ [PDF]
Subject and Purpose. The improvement of the atmosphere brightness temperature measuring method at frequencies of about 100 GHz is considered. The possibilities of the atmospheric carbon monoxide (CO) remote sensing instrument, developed at Institute of ...
A. M. Korolev +4 more
doaj +1 more source
Multifrequency spectra of solar brightness temperature derived from eclipse observations [PDF]
. Changes in solar radio-brightness temperature were derived at 2.8,19.3 and 22.2 GHz from the observations of radio flux during the total eclipse of 1980 February 16.
G. Raju +9 more
core +1 more source
Snow stratigraphic heterogeneity within ground-based passive microwave radiometer footprints: implications for emission modeling [PDF]
Two-dimensional measurements of snowpack properties (stratigraphic layering, density, grain size and temperature) were used as inputs to the multi-layer Helsinki University of Technology (HUT) microwave emission model at a centimeter-scale horizontal ...
Sandells, Melody +7 more
core +1 more source
SPECIAL FIELDS OF THE GALAXY RADIO EMISSION
The brightness temperatures of radio emission were measured with the UTR-2 low-frequency radio telescope at frequencies 12.6, 14.7, 16.7, 20 and 25 MHz for the following Galaxy regions: the North Pole, the area of minimum radio brightness and the ...
N. M. Vasilenko, M. A. Sidorchuk
doaj +1 more source
Homogeneous vs Biased IGM: Impact on Reionization
This paper considers the impact of large scale biasing of the IGM on reionization. The two simplest but extreme scenarios for IGM biasing are: an unbiased IGM which has a constant density and an IGM with density equal to the collapsed matter density.
Dinesh Raut
doaj +1 more source
Colour of baked products during baking
The parameters of the colour of the surface of bakery products - brightness L*, a* for red and b* for yellow colour - were measured at different temperature regimes. The parameters were found to change during the time of baking.
P. Novotná, A. Landfeld
doaj +1 more source
Microwave Observations of Venus with CLASS
We report on the disk-averaged absolute brightness temperatures of Venus measured at four microwave frequency bands with the Cosmology Large Angular Scale Surveyor.
Sumit Dahal +23 more
doaj +1 more source

