We get
very high flux at the center for getting to 600 — 800 C.
The authors report
very high fluxes associated with a small set of wells in southwest Pennsylvania, while finding «little or no emission» from other wells in a larger area.
Not exact matches
In a
very massive star, photon radiation — the outward
flux of photons that is generated due to the star's
very high interior temperatures — pushes gas from the star outward in opposition to the gravitational force that pulls the gas back in.
So, really, it's a moment of
flux in which the stakes are
very high but it's one in which fundamentally, people didn't know how to disagree.
However, ice is a poor conductor so, unless ice is
very thin or the geothermal heat
flux very high, tends not to influence melt at the ice surface.
Beta decay is often
very slow, and, if the
flux of neutrons is
high, the nucleus might capture another neutron before there is time for it to undergo decay.
Schaefer et al. state that there are four active volcanoes within the Southern Patagonian Icefield, which may be accounting for some additional basal melt, but that changes to mass balance from a
high geothermal heat
flux can only account for a
very small additional mass loss.
What also comes with it are
very high neutron
flux levels, which open up a variety of applications for stockpile stewardship,
high energy density physics and nuclear physics.
A good fit to the data is found by two distinct dust populations: (1)
very small, hence unbound, hot dust grains confined in a narrow region at the sublimation rim of carbonaceous material; (2) bound grains at 2 AU that are protected from sublimation and have a
higher mass despite their fainter
flux level.
The shortwave extreme ultraviolet
flux is much
higher in the distant past, which could pose problems for early Mars to develop a
very dense CO2 atmosphere early on for example, since C and O could escape from Mars early in its history (driven by these energetic wavelengths).
Reviewing the instruments in the pdf was
very interesting, the
high sensitivity / resolution for the CCD and a lack of shielding in the wake of possible ICME solar
flux in the next few years may be worrisome.
«The solar wind, because it is an extended ionized gas of
very high electrical conductivity, drags some magnetic
flux out of the Sun, thereby filling the heliosphere with the weak interplanetary magnetic field.
Chart: Solar X-Ray
Flux is described as follows: Level
Flux (watts / sq meter) Description A less than 10 ^ -LRB--8)
Very Low Background A between 10 ^ -LRB--8) and 10 - 7 Low Background B between 10 ^ -LRB--7) and 10 - 6 Moderate Background C between 10 ^ -LRB--6) and 10 - 5
High Background / Low Flare M between 10 ^ -LRB--5) and 10 - 4 Moderate Flare X between 10 ^ -LRB--4) and 10 - 3
High Flare Y greater than10 ^ -LRB--3) Extreme Flare http://www.ips.gov.au/Educational/2/1/3
Then try 1365/4 for the
flux and emissivity of 0.88 (which is closer to that of rock and soil) and you get 287.6 K which is
very close to the assumed mean surface temperature and thus obviates any need for that «33 degree of warming» In fact the 0.88 should be even lower and that gives
higher temperatures above 290K.
See lower figure 5.7 total heat
flux is essentially zero
higher than 80 north and
very little down to 70 north outside winter sea ice extent.
'' a
flux response function with a
very long tail (
high ECS,
high equilibration time) may give a result similar to the Schwartz exponential response function with a low ECS and low equilibration time.»
«c) the information content in the temperature and OHC series is not sufficient to allow accurate estimation of ECS and equilibration time; a
flux response function with a
very long tail (
high ECS,
high equilibration time) may give a result similar to the Schwartz exponential response function with a low ECS and low equilibration time.»
This persistence of
very high latent heat
flux is opposite to the seasonal trends of transpiration and evaporation in savannas, even with similar total rainfall (Saleska et al., 2003; da Rocha et al., 2009).
Tropical cyclones seem to me to be a
very good potential source of forcing «by daily and six - hourly winds and heat
fluxes», according to Enhanced vertical mixing within mesoscale eddies due to
high frequency winds in the South China Sea [3]:
Ben Wouters, At the link you provided you state, «magma erupting continuously at plate boundaries, a small but reasonably steady
flux» Considering that there is something like 45,000 miles of spreading centers, erupting over a width of a few miles, and that the temperature of the magma is
very high, I'm curious how you came to the conclusion that it was a «small»
flux.