The 13th and 14th Workshops on Antarctic Meteorology and Climate     

Matthew A.LAZZARA  Sophie A.ORENDORF  Taylor P.NORTON  Jordan G.POWERS  David H.BROMWICH  Scott CARPENTIER  John J.CASSANO  Steven R.COLWELL  Arthur M.CAYETTE  Kirstin WERNER 《大气科学进展》2020,37(5):423-430

1.Overview In July 2018,the Antarctic community came together to meet at the 13th Workshop on Antarctic Meteorology and Climate(WAMC)in Madison,Wisconsin,USA(Fig.1);and in the following year in June 2019,the 14th WAMC was held in Charleston,South Carolina,USA(Fig.2).With a growing history,the WAMC addresses the topics of Antarctic meteorology and climate(Kameda et al.,2008;Colwell et al.,2016;Lazzara et al.,2018)as well as weather-related issues of scientific and operational support.The workshops bring together researchers,operational forecasters,numerical modelers,observational specialists,and students.The themes of both workshops included Antarctic meteorological observations,Antarctic atmospheric numerical modeling,Antarctic meteorological and climate research,and Antarctic weather forecasting and operational services.The 2018 and 2019 WAMC were both followed by a one-day focus on the Year of Polar Prediction-Southern Hemisphere(YOPP-SH),when preparations and follow-up discussions were made with regard to the YOPP Special Observing Period from 16 November 2018 to 15 February 2019.  相似文献   

Global distribution of the intensity and frequency of hourly precipitation and their responses to ENSO     

Li  Xiao-Feng  Blenkinsop  Stephen  Barbero  Renaud  Yu  Jingjing  Lewis  Elizabeth  Lenderink  Geert  Guerreiro  Selma  Chan  Steven  Li  Yafei  Ali  Haider  Villalobos Herrera  Roberto  Kendon  Elizabeth  Fowler  Hayley J. 《Climate Dynamics》2020,54(11):4823-4839

Climate Dynamics - We investigate the global distribution of hourly precipitation and its connections with the El Niño–Southern Oscillation (ENSO) using both satellite precipitation...  相似文献   

Mid-level clouds over the Sahara in a convection-permitting regional model     

Mantsis  Damianos F.  Sherwood  Steven  Dixit  Vishal  Morrison  Hugh  Thompson  Greg 《Climate Dynamics》2020,54(7):3425-3439

Climate Dynamics - The simulation of Saharan mid tropospheric clouds is investigated with the weather research and forecasting (WRF) regional atmospheric model at convection permitting...  相似文献   

A diagnostic study of the southern hemisphere summer circulation of the CCC general circulation model     

Charles A. Lin  Lin Su  Steven J. Lambert 《大气与海洋》2013,51(3):297-319

Abstract

The medium‐scale wave regime, consisting largely of zonal wavenumbers 5–7, frequently dominates the summer Southern Hemisphere tropospheric circulation. We perform a diagnostic study of this circulation as simulated by the Canadian Climate Centre (CCC) general circulation model (GCM). The analysis of Hövmöller diagrams, space‐time and zonal wavenumber spectra shows that the CCC GCM is able to simulate the observed medium‐scale wave regime.

The zonally averaged meridional eddy heat and momentum transports and the associated baroclinic and barotropic energy conversions are also examined. The distributions of the transports on the vertical plane agree well with the observations. After comparison with the observed December‐January‐February 1979 distributions, some quantitative differences remain: the heat transport is too weak aloft and too large near the surface, whereas the momentum transport tends to be too weak. The baroclinic and barotropic conversions show a maximum in the medium‐scale waves. The time evolution of the Richardson number of the mean flow suggests that the medium‐scale wave is due to a baroclinic instability.  相似文献   

Sensitivity of multi-gas climate policy to emission metrics     

Steven J. Smith  Joseph Karas  Jae Edmonds  Jiyong Eom  Andrew Mizrahi 《Climatic change》2013,117(4):663-675

The Global Warming Potential (GWP) index is currently used to create CO₂-equivalent emission totals for multi-gas greenhouse targets. While many alternatives have been proposed, it is not possible to uniquely define a metric that captures the different impacts of emissions of substances with widely disparate atmospheric lifetimes, which leads to a wide range of possible index values. We examine the sensitivity of emissions and climate outcomes to the value of the index used to aggregate methane emissions using a technologically detailed integrated assessment model. The methane index is varied between 4 and 70, with a central value of 21, which is the 100-year GWP value currently used in policy contexts. We find that the sensitivity to index value is, at most, 10–18 % in terms of methane emissions but only 2–3 % in terms of the maximum total radiative forcing change, with larger regional emissions differences in some cases. The choice of index also affects estimates of the cost of meeting a given end of century forcing target, with total two-gas mitigation cost increasing by 7–9 % if the index is increased, and increasing in most scenarios from 4 to 23 % if the index is lowered, with a slight (1 %) decrease in total cost in one case. We find that much of the methane abatement occurs as the induced effect of CO₂ abatement rather than explicit abatement, which is one reason why climate outcomes are relatively insensitive to the index value. We also find that the near-term climate benefit of increasing the methane index is small.  相似文献   

Hard X-ray Microflares down to 3 keV     

Krucker  Säm  Christe  Steven  Lin  R.P.  Hurford  Gordon J.  Schwartz  Richard A. 《Solar physics》2002,210(1-2):445-456

The excellent sensitivity, spectral and spatial resolution, and energy coverage down to 3 keV provided by the Reuven Ramaty High-Energy Solar Spectroscopic Imager mission (RHESSI) allows for the first time the detailed study of the locations and the spectra of solar microflares down to 3 keV. During a one-hour quiet interval (GOES soft X-ray level around B6) on 2 May, 1:40–2:40 UT, at least 7 microflares occurred with the largest peaking at A6 GOES level. The microflares are found to come from 4 different active regions including one behind the west limb. At 7′′ resolution, some events show elongated sources, while others are unresolved point sources. In the impulsive phase of the microflares, the spectra can generally be fitted better with a thermal model plus power law above ∼ 6–7 keV than with a thermal only. The decay phase sometimes can be fitted with a thermal only, but in some events, power-law emission is detected late in the event indicating particle acceleration after the thermal peak of the event. The behind-the-limb microflare shows thermal emissions only, suggesting that the non-thermal power law emission originates lower, in footpoints that are occulted. The power-law fits extend to below 7 keV with exponents between −5 and −8, and imply a total non-thermal electron energy content between 10²⁶–10²⁷ erg. Except for the fact that the power-law indices are steeper than what is generally found in regular flares, the investigated microflares show characteristics similar to large flares. Since the total energy in non-thermal electrons is very sensitive to the value of the power law and the energy cutoff, these observations will give us better estimates of the total energy input into the corona. (Note that color versions of figures are on the accompanying CD-ROM.) Supplementary material to this paper is available in electronic form at http://dx.doi.org/10.1023/A:1022404512780  相似文献   

Fossils explained 44: Post-Palaeozoic nautiloids     

Stephen K. Donovan  & Steven Baker† 《Geology Today》2003,19(5):181-185

  相似文献   

Slip rates on the Helike Fault, Gulf of Corinth, Greece: new evidence from geoarchaeology     

Ioannis K. Koukouvelas  Dora Katsonopoulou  Steven Soter  Paraskevas Xypolias 《地学学报》2005,17(2):158-164

Palaeoseismological and archaeological analysis of a trench enabled us to estimate the Holocene slip rates on the East Helike Fault, flanking the south-western Gulf of Corinth. We recognized two major fault strands within the trench: the ‘north fault’ controls a succession of three colluvial wedges and the deposition of a 2.7 m thick sedimentary sequence. The ‘south fault’ controls the deposition of a 2.9-m thick brownish-red colluvium. Based on colluvial stratigraphy, radiocarbon dating of the sediments suggests that the slip rate was c. 0.3 mm yr⁻¹ from 10 250 to c. 1400 bp , when it increased dramatically to c. 2.0 mm yr⁻¹ after a strong earthquake event near 1400 bp . The faster slip rate evidently increased the sedimentation rate.  相似文献   

A kinematical approach to dark energy studies     

David Rapetti  Steven W. Allen  Mustafa A. Amin  Roger D. Blandford 《Monthly notices of the Royal Astronomical Society》2007,375(4):1510-1520

  相似文献   

MICROBIOCLIMATE: ONE TOOL FOR ENVIRONMENTAL ASSESSMENT     

Steven A. Carlson  Evan Denney 《The Professional geographer》1978,30(1):42-47

  相似文献