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901.
Zhmur V. V. Novoselova E. V. Belonenko T. V. 《Izvestiya Atmospheric and Oceanic Physics》2021,57(6):632-641
Izvestiya, Atmospheric and Oceanic Physics - The potential vorticity (PV) in the ocean is considered, including the history of the term. Various aspects and basic formulas used to calculate the PV... 相似文献
902.
903.
904.
A. A. Zhamaletdinov A. N. Shevtsov E. P. Velikhov A. A. Skorokhodov V. E. Kolesnikov T. G. Korotkova P. A. Ryazantsev B. V. Efimov V. V. Kolobov M. B. Barannik P. I. Prokopchuk V. N. Selivanov Yu. A. Kopytenko E. A. Kopytenko V. S. Ismagilov M. S. Petrishchev P. A. Sergushin P. E. Tereshchenko B. V. Samsonov M. A. Birulya M. Yu. Smirnov T. Korja Yu. M. Yampolski A. V. Koloskov N. A. Baru S. V. Poljakov A. V. Shchennikov G. I. Druzhin W. Jozwiak J. Reda Yu. G. Shchors 《Izvestiya Atmospheric and Oceanic Physics》2015,51(8):826-857
905.
906.
Akkur V. Raman Rayaroth Damodaran Lisa A. Levin Thiruchitrambalam Ganesh Yannamani K. V. Rao Sateesh Nanduri Rakhesh Madhusoodhanan 《Marine Ecology》2015,36(3):679-700
The Bay of Bengal remains one of the least studied of the world's oxygen minimum zones (OMZs). Here we offer a detailed investigation of the macrobenthos relative to oxygen minimum zone [OMZ – DO (dissolved oxygen), concentration <0.5 ml·1?1] at 110 stations off the North East Indian margin (160 and 200 N) featuring coastal, shelf and slope settings (10–1004 m). Macrobenthos (>0.5 mm) composition, abundance and diversity were studied in relation to variations in depth, dissolved oxygen, sediment texture and organic carbon. Using multivariate procedures powered by SIMPROF analysis we identified distinct OMZ core sites (depth 150–280 m; DO 0.37 ml·1?1) that exhibited dense populations of surface‐feeding polychaetes (mean 2188 ind. m?2) represented by spionids and cossurids (96%). Molluscs and crustaceans were poorly represented except for ampeliscid amphipods. The lower OMZ sites (DO > 0.55 ml·l?1) supported a different assemblage of polychaetes (cirratulids, amphinomids, eunicids, orbinids, paraonids), crustaceans and molluscs, albeit with low population densities (mean 343 ind. m?2). Species richness [E(S100)], diversity (Margalef d; H’) and evenness (J’) were lower and dominance was higher within the OMZ core region. Multiple regression analysis showed that a combination of sand, clay, organic carbon, and dissolved oxygen explained 62–78% of the observed variance in macrobenthos species richness and diversity: E(S100) and H’. For polychaetes, clay and oxygen proved important. At low oxygen sites (DO <1 ml·l?1), depth accounted for most variance. Residual analysis (after removing depth effects) revealed that dissolved oxygen and sediment organic matter influenced 50–62% of residual variation in E(S100), H’ and d for total macrofauna. Of this, oxygen alone influenced up to ~50–62%. When only polychaetes were evaluated, oxygen and organic matter explained up to 58–63%. For low oxygen sites, organic matter alone had the explanatory power when dominance among polychaetes was considered. Overall, macrobenthic patterns in the Bay of Bengal were consistent with those reported for other upwelling margins. However, the compression of faunal gradients at shallower depths was most similar to the Chile/Peru margin, and different from the Arabian Sea, where the depth range of the OMZ is two times greater. The Bay of Bengal patterns may take on added significance as OMZs shoal globally. 相似文献
907.
R.R. Rao M.S. Girish Kumar M. Ravichandran A.R. Rao V.V. Gopalakrishna P. Thadathil 《Deep Sea Research Part I: Oceanographic Research Papers》2010,57(1):1-13
The observed variability of the Kelvin waves and their propagation in the equatorial wave guide of the Indian Ocean and in the coastal wave guides of the Bay of Bengal (BoB) and the southeastern Arabian Sea (AS) on seasonal to interannual time scales during years 1993–2006 is examined utilizing all the available satellite and in-situ measurements. The Kelvin wave regime inferred from the satellite-derived sea surface height anomalies (SSHA) shows a distinct annual cycle composed of two pairs of alternate upwelling (first one occurring during January–March and the second one occurring during August–September) and downwelling (first one occurring during April–June and the second one occurring during October–December) Kelvin waves that propagate eastward along the equator and hit the Sumatra coast and bifurcate. The northern branches propagate counterclockwise over varied distances along the coastal wave guide of the BoB. The potential mechanisms that contribute to the mid-way termination of the first upwelling and the first downwelling Kelvin waves in the wave guide of the BoB are hypothesized. The second downwelling Kelvin wave alone reaches the southeastern AS, and it shows large interannual variability caused primarily by similar variability in the equatorial westerly winds during boreal fall. The westward propagating downwelling Rossby waves triggered by the second downwelling Kelvin wave off the eastern rim of the BoB also shows large interannual variability in the near surface thermal structure derived from SODA analysis. The strength of the equatorial westerlies driven by the east–west gradient of the heat sources in the troposphere appears to be a critical factor in determining the observed interannual variability of the second downwelling Kelvin wave in the wave guides of the equatorial Indian Ocean, the coastal BoB, and the southeastern AS. 相似文献
908.
V.V. Gopalakrishna F. Durand K. Nisha M. Lengaigne T.P. Boyer J. Costa R.R. Rao M. Ravichandran S. Amrithash L. John K. Girish C. Ravichandran V. Suneel 《Deep Sea Research Part I: Oceanographic Research Papers》2010,57(6):739-754
The southeastern Arabian Sea (SEAS), located in the Indian Ocean warm pool, is a key-region of the regional climate system. It is suspected to play an important role in the dynamics of the Asian summer monsoon system. The present study reports the salient features derived from a newly harvested observational dataset consisting of repeated fortnightly XBT transects in the SEAS over the period 2002–2008. The fortnightly resolution of such a multi-year record duration is unprecedented in this part of the world ocean and provides a unique opportunity to examine the observed variability of the near-surface thermal structure over a wide spectrum, from intra-seasonal to interannual timescales. We find that most of the variability is trapped in the thermocline, taking the form of upwelling and downwelling motions of the thermal stratification. The seasonal variations are consistent with past studies and confirm the role of the monsoonal wind forcing through linear baroclinic waves (coastally-trapped Kelvin and planetary Rossby waves). Sub-seasonal variability takes the form of anomalous events lasting a few weeks to a few months and occurs at two preferred timescales: in the 30–110 day band, within the frequency domain of the Madden–Julian oscillation and in the 120–180 day band. While this sub-seasonal variability appears fairly barotropic in the offshore region, the sign of the anomaly in the upper thermocline is opposite to that in its lower part on many occasions along the coast. Our dataset also reveals relatively large interannual temperature variations of about 1 °C from 50 to 200 m depth that reflect a considerable year-to-year variability of the magnitude of both upwelling and downwelling events. This study clearly demonstrates the necessity for sustained long-term temperature measurements in the SEAS. 相似文献
909.
S. A. Sviridov N. A. Palshin V. A. Solovyev A. V. Zaretskiy A. A. Metal’nikov 《Oceanology》2010,50(1):139-147
A coastal observatory for long-term continuous measurements of oceanological parameters and real-time data transfer via the
Internet to remote users is described. The observatory was designed at the Shirshov Institute of Oceanology (SIO) and tested
at its southern branch (SB) in the Black Sea. The architecture, components, and design principles of the observatory are discussed
along with its application for solving problems of water dynamics in the coastal zone. Results of field tests are given. 相似文献
910.
This paper studies the causes and mechanisms of the formation of extreme anomalies in the tropospheric temperature associated
with the North Atlantic Oscillation (NAO). Our approach is based on understanding that, in the annual cycle, continental-scale
tropospheric temperature anomalies (planetary waves with longitudinal wave numbers of 1–3) can both intensify under the direct
action of heat inflow as an energy source for these anomalies (radiation cooling/heating) and weaken as a result of the destructive
action of heat inflow under temperature advections with the opposite (to the heat inflow) sign [4, 5]. According to the monthly
mean data of the NCEP/NCAR reanalysis over the 40-year period, seasonal air temperature anomalies have been studied at the
level 850 hPa (T
850) in different regions of Eurasia. It has been confirmed that the negative NAO phase in winter is favorable for preserving
negative T
850 anomalies in the east of the continent at this time of year, whereas the positive NAO phase is favorable for negative T
850 anomalies in the west. However, it has been revealed that this dependence was critically violated during the winter seasons
approximately two years before an extreme event. This was explained by the fact that, in those years, the NAO influence on
winter T
850 anomalies was limited. This paper formally considers a certain mechanism of anomalous heat inflow as an energy source for
these anomalies with functions of the formation (intensification) of negative T
850 anomalies in winter and positive T
850 anomalies in summer, as well as with a function of the limitation of the influence of the predominant dynamic mode on some
regions of the continent. It is shown that, in the 1960s, T
850 anomalies with negative NAO indices in the east of the continent were governed by a hypothetic mechanism of heat inflow as
an energy source for anomalies; in 1980s, at prolonged positive NAO indices, T
850 anomalies in the west of the continent could also be governed by this mechanism. This paper, within the accepted degree of
detail, demonstrates the process of limitation of the NAO influence in some years (1966, 1967, 1987, and 1988), which leads
to an unbalance of the anomalies and a possible extreme phenomenon. It is demonstrated that, in some seasons, the anomalies
were not governed by the hypothetic mechanism of the heat inflow under the action of large NAO changes and a complete upset
of the annual cycle of anomalies. Determining the first indicators of the unbalance, which can lead to extreme anomalies,
is shown to be difficult if it is based only on an analysis of winter seasons (as is the case with most of the works) without
invoking the annual trends of the tropospheric temperature and the NAO index. 相似文献