A high performance solar radio observation system in terrible RFI environments for existing telescope

Author(s):  
Liang Dong ◽  
LeSheng He ◽  
Min Wang ◽  
Guannao Gao
2019 ◽  
Vol 49 (8) ◽  
pp. 901-909 ◽  
Author(s):  
Yao CHEN ◽  
ShiWei FENG ◽  
FaBao YAN ◽  
ChangShuo CHEN ◽  
YanRui SU ◽  
...  

2018 ◽  
Vol 11 (11) ◽  
pp. 6059-6074 ◽  
Author(s):  
Alexander Gvakharia ◽  
Eric A. Kort ◽  
Mackenzie L. Smith ◽  
Stephen Conley

Abstract. We present the development and assessment of a new flight system that uses a commercially available continuous-wave, tunable infrared laser direct absorption spectrometer to measure N2O, CO2, CO, and H2O. When the commercial system is operated in an off-the-shelf manner, we find a clear cabin pressure–altitude dependency for N2O, CO2, and CO. The characteristics of this artifact make it difficult to reconcile with conventional calibration methods. We present a novel procedure that extends upon traditional calibration approaches in a high-flow system with high-frequency, short-duration sampling of a known calibration gas of near-ambient concentration. This approach corrects for cabin pressure dependency as well as other sources of drift in the analyzer while maintaining a ∼90 % duty cycle for 1 Hz sampling. Assessment and validation of the flight system with both extensive in-flight calibrations and comparisons with other flight-proven sensors demonstrate the validity of this method. In-flight 1σ precision is estimated at 0.05 ppb, 0.10 ppm, 1.00 ppb, and 10 ppm for N2O, CO2, CO, and H2O respectively, and traceability to World Meteorological Organization (WMO) standards (1σ) is 0.28 ppb, 0.33 ppm, and 1.92 ppb for N2O, CO2, and CO. We show the system is capable of precise, accurate 1 Hz airborne observations of N2O, CO2, CO, and H2O and highlight flight data, illustrating the value of this analyzer for studying N2O emissions on ∼100 km spatial scales.


2018 ◽  
Author(s):  
Alexander Gvakharia ◽  
Eric A. Kort ◽  
Mackenzie L. Smith ◽  
Stephen Conley

Abstract. We present the development and assessment of a new flight system that uses a commercially available continuous-wave, tunable infrared laser direct absorption spectrometer to measure N2O, CO2, CO, and H2O. When the commercial system is operated in an off-the-shelf manner, we find a clear cabin pressure/altitude dependency for N2O, CO2, and CO. The characteristics of this artifact make it difficult to reconcile with conventional calibration methods, so we present a novel procedure employing a high-flow system with high-frequency, short-duration sampling of a known calibration gas. This approach corrects for cabin pressure dependency as well as other sources of drift in the analyzer while maintaining a ~ 90 % duty cycle for 1 Hz sampling. Assessment and validation of the flight system with both extensive in-flight calibrations and comparisons with other flight-proven sensors demonstrate the validity of this method. In-flight 1σ precision is estimated at 0.05 ppb, 0.10 ppm, 1.00 ppb, and 10 ppm for N2O, CO2, CO, and H2O respectively, and traceability to WMO standards is found to be 0.14 ppb, 0.34 ppm, and 2.33 ppb for N2O, CO2, and CO. We show the system is capable of precise, accurate 1 Hz airborne observations of N2O, CO2, CO, and H2O and highlight flight data illustrating the value of this analyzer for studying N2O emissions on ~ 100 km spatial scales.


Author(s):  
Kushagra Upadhyay ◽  
Bhuwan Joshi ◽  
Prabir K. Mitra ◽  
R. Bhattacharyya ◽  
Divya Oberoi ◽  
...  

Solar Physics ◽  
2012 ◽  
Vol 277 (2) ◽  
pp. 447-457 ◽  
Author(s):  
K. Iwai ◽  
F. Tsuchiya ◽  
A. Morioka ◽  
H. Misawa

2020 ◽  
Vol 51 (4) ◽  
pp. 413-423
Author(s):  
Ke XU ◽  
ZiQian SHANG ◽  
FaBao YAN ◽  
Yang LIU ◽  
Zhao WU ◽  
...  

2018 ◽  
Vol 11 (7) ◽  
pp. 2941-2953 ◽  
Author(s):  
Sebastian D. Eastham ◽  
Michael S. Long ◽  
Christoph A. Keller ◽  
Elizabeth Lundgren ◽  
Robert M. Yantosca ◽  
...  

Abstract. Global modeling of atmospheric chemistry is a grand computational challenge because of the need to simulate large coupled systems of ∼100–1000 chemical species interacting with transport on all scales. Offline chemical transport models (CTMs), where the chemical continuity equations are solved using meteorological data as input, have usability advantages and are important vehicles for developing atmospheric chemistry knowledge that can then be transferred to Earth system models. However, they have generally not been designed to take advantage of massively parallel computing architectures. Here, we develop such a high-performance capability for GEOS-Chem (GCHP), a CTM driven by meteorological data from the NASA Goddard Earth Observation System (GEOS) and used by hundreds of research groups worldwide. GCHP is a grid-independent implementation of GEOS-Chem using the Earth System Modeling Framework (ESMF) that permits the same standard model to operate in a distributed-memory framework for massive parallelization. GCHP also allows GEOS-Chem to take advantage of the native GEOS cubed-sphere grid for greater accuracy and computational efficiency in simulating transport. GCHP enables GEOS-Chem simulations to be conducted with high computational scalability up to at least 500 cores, so that global simulations of stratosphere–troposphere oxidant–aerosol chemistry at C180 spatial resolution (∼0.5∘×0.625∘) or finer become routinely feasible.


2018 ◽  
Author(s):  
Sebastian D. Eastham ◽  
Michael S. Long ◽  
Christoph A. Keller ◽  
Elizabeth Lundgren ◽  
Robert M. Yantosca ◽  
...  

Abstract. Global modeling of atmospheric composition is a grand computational challenge because of the need to simulate large coupled systems of chemical species interacting with transport on all scales. Off-line chemical transport models (CTMs), where the chemical continuity equations are solved using meteorological data as input, have the advantages of simplicity and reproducibility, and are important vehicles for developing knowledge that can then be transferred to Earth system models. However, they have generally not been designed to take advantage of massively parallel computing architectures. Here we develop such a high-performance capability (GCHP) for GEOS-Chem, a CTM driven by GEOS meteorological data from the NASA Goddard Earth Observation System (GEOS) and used by hundreds of research groups worldwide. GCHP is a grid-independent implementation of GEOS-Chem using the Earth System Modeling Framework (ESMF) that permits the same standard model to be run in a distributed-memory framework, scalable from six cores on a single node up to hundreds of cores distributed across a network. GCHP also allows GEOS-Chem to take advantage of the native GEOS cubed-sphere grid for greater accuracy and computational efficiency in simulating transport. GCHP enables GEOS-Chem simulations to be conducted with high computational scalability up to at least 500 cores, so that global simulations of stratosphere-troposphere oxidant-aerosol chemistry at C180 spatial resolution (~0.5° × 0.625°) or finer become routinely feasible.


1967 ◽  
Vol 1 (2) ◽  
pp. 61-62
Author(s):  
T. L. Landecker

The study of the sources of the slowly varying component at decimetre and centimetre wavelengths has been a major preoccupation of solar radio astronomers. Grating interferometers and other high-resolution aerial systems have enabled the separation of the S-component from the Sun’s total emission, and the study of individual sources. Nevertheless much of value remains to be derived from whole-sun intensity measurements—the most basic solar radio observation.


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