«A recent underwater expedition to the Red Sea offshore from Sudan and Eritrea [18]
found surface water temperatures 28 °C in winter and up to 34 °C in the summer, but despite that extreme heat the coral was healthy with much fish life with very little sign of coral bleaching»
Not exact matches
«We
found that there was a
surface temperature impact due to changes in
water vapor in a fairly narrow region of the stratosphere,» explains research meteorologist Karen Rosenlof of the National Oceanic and Atmospheric Administration's (NOAA) Aeronomy Laboratory, one of the authors of the study.
The
temperature of the latter was
found to have increased by up to 4 °C above the
temperature of the
water while it twisted and turned at the
surface for about ten hours at a time.
In the search for other Earths, the main goal is to
find a planet the same size as ours that sits in the habitable zone — the region around a given star where planetary
surface temperature would be similar to ours, allowing liquid
water to exist.
Surface temperatures probably soar to almost 600 °C, so there's no hope of
finding liquid
water there, let alone life.
There, many kilometers deep, the carbonate rocks will be exposed to very high pressures and
temperatures, converting the carbonate rocks back to the silicates and expelling CO2 and
water — these gases will then
find their ways to the
surface through explosive volcanoes near the plate subduction boundaries.
Using these steady - states, we
find that if volatile cycling is either solely dependent on
temperature or seafloor pressure, exoplanets require a high abundance (more than 0.3 % of the total mass) of
water to have fully inundated
surfaces.
The research published in Nature Communications
found that in the past, when ocean
temperatures around Antarctica became more layered - with a warm layer of
water below a cold
surface layer - ice sheets and glaciers melted much faster than when the cool and warm layers mixed more easily.
The first step in
finding possible abodes for life is to
find planets in the Habitable Zones of their stars, whose
surface temperatures would allow liquid
water.
Hansen et al. recently explored the effect of stratification of meltwater
water on storminess, sea
surface temperature and sea level rise and
found that, among other things, their model predicted strong feedbacks in ice sheet exposure to destabilizing influences.
Using an ocean circulation model for the shelf, the authors
find that
surface temperatures may increase by 0.5 to 2.0 °C, seasonal
surface salinity may drop by up to 2 PSS in some areas, and that Haida Eddies will strengthen, as will the Vancouver Island Coastal Current and freshwater discharges into coastal
waters.
It seemsthe observed increase in trade winds lead to the
surfacing of cooler
waters in the Eastern Pacific ocean and this phenomenon is
found by models to cause global average
temperatures to cool.
''... worked with two sediment cores they extracted from the seabed of the eastern Norwegian Sea, developing a 1000 - year proxy
temperature record «based on measurements of δ18O in Neogloboquadrina pachyderma, a planktonic foraminifer that calcifies at relatively shallow depths within the Atlantic
waters of the eastern Norwegian Sea during late summer,» which they compared with the temporal histories of various proxies of concomitant solar activity... This work revealed, as the seven scientists describe it, that «the lowest isotope values (highest
temperatures) of the last millennium are seen ~ 1100 - 1300 A.D., during the Medieval Climate Anomaly, and again after ~ 1950 A.D.» In between these two warm intervals, of course, were the colder
temperatures of the Little Ice Age, when oscillatory thermal minima occurred at the times of the Dalton, Maunder, Sporer and Wolf solar minima, such that the δ18O proxy record of near -
surface water temperature was
found to be «robustly and near - synchronously correlated with various proxies of solar variability spanning the last millennium,» with decade - to century - scale
temperature variability of 1 to 2 °C magnitude.»
He
found that larger rocky planets are more likely than smaller ones to have
surface temperatures where liquid
water could exist, given the same amount of light from the star.
They
found that an atmospheric exchange of
surface heat drives the greatest
temperature fluctuations in reefs located in shallow, low - tide
waters.
When that air
finds a
surface, such as a cold duct boot, at a
temperature below the dew point, the
water vapor just can't help itself.
Motivated by
findings that major components of so - called cloud «feedbacks» are best understood as rapid responses to CO2 forcing (Gregory and Webb in J Clim 21:58 — 71, 2008), the top of atmosphere (TOA) radiative effects from forcing, and the subsequent responses to global
surface temperature changes from all «atmospheric feedbacks» (
water vapour, lapse rate,
surface albedo, «
surface temperature» and cloud) are examined in detail in a General Circulation Model.
Corrections: Del Genio et al. (1991); Raval and Ramanathan (1989)
found that satellite infrared measurements gave «compelling evidence for the positive feedback between
surface temperature,
water vapour and the greenhouse effect; the magnitude of the feedback is consistent with that predicted by climate models;» similarly, Rind et al. (1991), p. 500; Sun and Held (1996); and the final nail in the coffin, Soden et.
«We
find that the observed
surface temperature and lapse rate structure of the lower atmosphere can be reproduced quite closely with a greenhouse model that contains the
water vapor abundance reported by the Venera spectrophotometer experiment.
Try to
find some experimental evidence of what happens to bulk
water temperature when overhead illumination by ~ 10um radiation is raised and the
surface is free to evaporate in response.
Zhang et al. (2006)
found that the
surface LW flux was very sensitive to assumptions about tropospheric
water vapor and
temperatures but did not analyze the dependence on clouds.