Factors Controlling Free Air and Ocean Temperature of the Last 30 Years and Extrapolation to the Past

1987 ◽  
pp. 67-87 ◽  
Author(s):  
Reginald E. Newell ◽  
Jane Hsiung
Keyword(s):  
The Past ◽  
2020 ◽  
Author(s):  
Jeemijn Scheen ◽  
Thomas F. Stocker

Abstract. Paleoreconstructions and modern observations provide us with anomalies of surface temperature over the past millennium. The history of deep ocean temperatures is much less well-known and was simulated in a recent study for the past 2000 years under forced surface temperature anomalies. In this study, we simulate the past 800 years with an illustrative forcing scenario in the Bern3D ocean model, which enables us to assess the role of changes in ocean circulation on deep ocean temperature. We quantify the effect of changing ocean circulation by comparing transient simulations (where the ocean dynamically adjusts to anomalies in surface temperature – hence density) to simulations with fixed ocean circulation. We decompose temperature, ocean heat content and meridional heat transport into the contributions from changing ocean circulation and changing sea surface temperature (SST). In the deep ocean, the contribution from changing ocean circulation is found to be as important as the changing SST signal itself. Firstly, the small changes in ocean circulation amplify the Little Ice Age signal around 3 km depth by at least a factor of two, depending on the basin. Secondly, they fasten the arrival of this atmospheric signal in the Pacific and Southern Ocean at all depths, whereas they delay the arrival in the Atlantic between about 2.5 and 3.5 km by two centuries. This delay is explained by an initial competition between the Little Ice Age cooling and a warming due to an increase in relatively warmer North Atlantic Deep Water at the cost of Antarctic Bottom Water. Under the consecutive AMOC slowdown, this shift in water masses is inverted and aging of the water causes a late additional cooling. Our results suggest that small changes in ocean circulation can have a large impact on the amplitude and timing of ocean temperature anomalies below 2 km depth.


2020 ◽  
Vol 87 (5) ◽  
Author(s):  
Anthoni Giam ◽  
William Toh ◽  
Vincent Beng Chye Tan

Abstract The analysis of complex blast scenarios typically requires advanced computational methods such as multi-material Eulerian and coupled Eulerian–Lagrangian (CEL) analysis where Jones–Wilkins–Lee (JWL) equation of state is used to model the explosive material. While multiple sets of empirical JWL parameters for trinitrotoluene (TNT) explosives have been published over the past few decades, there is also a lack of guidelines and comparative studies on their applications for the blast analysis. A standardized description of the explosive material behavior allows for a better interpretation of results from research studies involving different blast scenarios and JWL parameters. In this paper, the authors utilize numerical finite element (FE) simulations to investigate the influence of different TNT JWL parameter sets on the blast wave characteristics of a free-air blast across different scaled distances. Utilizing multi-material Eulerian analysis, a series of spherical free-air blasts involving a 100-kg TNT charge modeled with different TNT JWL parameters are conducted. The blast wave characteristics including the incident overpressure, impulse, and time of arrival (TOA) are benchmarked against the empirical-based Kingery–Bulmash air blast formulations through the conventional weapon effect calculator conwep. It was found that the incident overpressure and impulse are highly sensitive to the JWL parameters, with differences as high as 40% at smaller scaled distances, while the influence on TOA is much less significant. This paper hopes to provide a guide for future users on the appropriate JWL parameter sets to model the air blast events involving TNT explosives.


2005 ◽  
Vol 13 ◽  
pp. 951-952
Author(s):  
J.W.V. Storey ◽  
M.C.B. Ashley ◽  
M.G. Burton ◽  
J.S. Lawrence

AbstractA well-focused research program over the past decade has shown that the South Pole has many remarkable characteristics that are particularly favorable for astronomy. These include the very cold, dry atmosphere and the vanishingly small free-air turbulence. Dome C, site of the new French/Italian station Concordia, has all of these attributes plus the added advantage of very low ground-level wind speeds. Higher on the plateau, locations such as the 4200 m high Dome A may well represent the ultimate ground based astronomical observing sites.


1956 ◽  
Vol 37 (6) ◽  
pp. 251-262 ◽  
Author(s):  
J. R. Gerhardt ◽  
C. M. Crain ◽  
H. Chapman

The study of tropospheric refractive index distributions which began in 1951 using an airborne microwave refractometer has been continued during the past year with emphasis being placed on obtaining data on the microstructure of the atmosphere. Refractometers sufficiently sensitive to observe refractive index or equivalent moisture content variations having frequencies up to 100 cycles per second and amplitudes as small as 0.01 N-unit have been used in aircraft over New England, Florida, Ohio and Colorado areas to measure refractive index fluctuations from near the surface to up to 20,000 feet. Special efforts have been made to obtain data on free air and air to cloud index changes and a summary of certain of these data is presented. Preliminary analyses are made of data showing flights through clouds, convective thermals and frontal systems.


2010 ◽  
Vol 3 (9) ◽  
pp. 622-626 ◽  
Author(s):  
Matt S. McGlone ◽  
Chris S. M. Turney ◽  
Janet M. Wilmshurst ◽  
James Renwick ◽  
Katharina Pahnke

2018 ◽  
Author(s):  
Małgorzata Merchel ◽  
Waldemar Walczowski

Abstract. This study investigated the temporal variability of the basic physical properties of deep and intermediate waters in the Nordic Seas from 1997 to 2016. Special attention paid to quantifying changes in their temperature and salinity and determining potential drivers of these changes. Hydrographic data were obtained during annual cruises of the R/V Oceania in the Nordic Seas region from 1997 to 2016. The results show that, in the past 20 years, deep and intermediate waters in the studied region have warmed at least 10 times more than the mean global ocean temperature change; salinity has also changed. This means that changes in these waters' properties have a much greater impact on recent climate change intensification than previously thought. For example, ocean circulation, dissolved oxygen, carbon dioxide content, and sea level rise, may also change much faster.


2020 ◽  
Vol 11 (4) ◽  
pp. 925-951
Author(s):  
Jeemijn Scheen ◽  
Thomas F. Stocker

Abstract. Paleoreconstructions and modern observations provide us with anomalies of surface temperature over the past millennium. The history of deep ocean temperatures is much less well-known and was simulated in a recent study for the past 2000 years under forced surface temperature anomalies and fixed ocean circulation. In this study, we simulate the past 800 years with an illustrative forcing scenario in the Bern3D ocean model, which enables us to assess the impact of changes in ocean circulation on deep ocean temperature. We quantify the effect of changing ocean circulation by comparing transient simulations (where the ocean dynamically adjusts to anomalies in surface temperature – hence density) to simulations with fixed ocean circulation. We decompose temperature, ocean heat content and meridional heat transport into the contributions from changing ocean circulation and changing sea surface temperature (SST). In the deep ocean, the contribution from changing ocean circulation is found to be as important as the changing SST signal itself. Firstly, the small changes in ocean circulation amplify the Little Ice Age signal at around 3 km depth by at least a factor of 2, depending on the basin. Secondly, they fasten the arrival of this atmospheric signal in the Pacific and Southern Ocean at all depths, whereas they delay the arrival in the Atlantic between about 2.5 and 3.5 km by two centuries. This delay is explained by an initial competition between the Little Ice Age cooling and a warming due to an increase in relatively warmer North Atlantic Deep Water at the cost of Antarctic Bottom Water. Under the consecutive Atlantic meridional overturning circulation (AMOC) slowdown, this shift in water masses is inverted and ageing of the water causes a late additional cooling. Our results suggest that small changes in ocean circulation can have a large impact on the amplitude and timing of ocean temperature anomalies below 2 km depth.


1967 ◽  
Vol 31 ◽  
pp. 405
Author(s):  
F. J. Kerr

A continuum survey of the galactic-centre region has been carried out at Parkes at 20 cm wavelength over the areal11= 355° to 5°,b11= -3° to +3° (Kerr and Sinclair 1966, 1967). This is a larger region than has been covered in such surveys in the past. The observations were done as declination scans.


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