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Climate Hustle

The runaway greenhouse effect on Venus

What the science says...

Venus very likely underwent a runaway or ‘moist’ greenhouse phase earlier in its history, and today is kept hot by a dense CO2 atmosphere.

Climate Myth...

Venus doesn't have a runaway greenhouse effect
Venus is not hot because of a runaway greenhouse.

In keeping with my recent theme of discussing planetary climate, I am revisiting a claim last year made by Steven Goddard at WUWT (here and here, and echoed by him again recently) that “the [runaway greenhouse] theory is beyond absurd,” and that it is pressure, not the greenhouse effect that keeps Venus hot.  My focus in this post is not on his alternative theory (discussed here), but to discuss Venus and the runaway greenhouse in general, as a matter of interest and as an educational opportunity.  In keeping my skepticism fair, I’d also like to address claims (sometimes thrown out by Jim Hansen in passing by) that burning all the coal, tars, and oil could conceivably initiate a runaway on Earth.

It is worth noting that the term runaway greenhouse refers to a specific process when discussed by planetary scientists, and simply having a very hot, high-CO2 atmosphere is not it.  It is best thought of as a process that may have happened in Venus’ past (or a large number of exo-planets being discovered close enough to their host star) rather than a circumstance it is currently in.

A Tutorial of Present-Day Venus

Venus’ orbit is approximately 70% closer to the sun, which means it receives about 1/0.72 ~ 2 times more solar insolation at the top of the atmosphere than Earth.  Venus also has a very high albedo which ends up over-compensating for the distance to the sun, so the absorbed solar energy by Venus is less than that for Earth.  The high albedo can be attributed to a host of gaseous sulfur species, along with what water there is, which provide fodder for several globally encircling sulfuric acid (H2SO4) cloud decks.  SO2 and H2O are the gaseous precursor of the clouds particles; the lower clouds are formed by condensation of H2SO4 vapor, with SO2 created by photochemistry in the upper clouds. Venus’ atmosphere also has a pressure of ~92 bars, nearly equivalent to what you’d feel swimming under a kilometer of ocean.  The dense atmosphere could keep the albedo well above Earth’s even without clouds due to the high Rayleigh scattering (the effect of clouds on Venus and how they could change in time is discussed in Bullock and Grinspoon, 2001). Less than 10% of the incident solar radiation reaches the surface.

Observations of the vapor content in the Venusian atmosphere show an extremely high heavy to light isotopic ratio (D/H) and is best interpreted as a preferential light hydrogen escape to space, while deuterium escapes less rapidly.  A lower limit of at least 100 times its current water content in the past can be inferred (e.g. Selsis et al. 2007 and references therein).

The greenhouse effect on Venus is primarily caused by CO2, although water vapor and SO2 are extremely important as well.  This makes Venus very opaque throughout the spectrum (figure 1a), and since most of the radiation that makes its way out to space comes from only the very topmost parts of the atmosphere, it can look as cold as Mars from IR imagery. In reality, Venus is even hotter than the dayside of Mercury, at an uncomfortable 735 K (or ~860 F). Like Earth, Venusian clouds also generate a greenhouse effect, although they are not as good infrared absorbers/emitters as water clouds.  However, the concentrated sulfuric acid droplets can scatter infrared back to the surface, generating an alternative form of the greenhouse effect that way.  In the dense Venusian CO2 atmosphere, pressure broadening from collisions and the presence of a large number of absorption features unimportant on modern Earth can come into play (figure 1b), which means quick and dirty attempts by Goddard to extrapolate the logarithmic dependence between CO2 and radiative forcing make little sense.  The typical Myhre et al (1998) equation which suggests every doubling of CO2 reduces the outgoing flux at the tropopause by ~4 W/m2, although even for CO2 concentration typical of post-snowball Earth states this can be substantially enhanced.  Figure 1b also shows that CO2 is not saturated, as some skeptics have claimed.

 

 Figure 1: a) Radiant spectra for the terrestrial planets.  Courtesy of David Grisp (Jet Propulsion Laboratory/CIT), from lecture "Understanding the Remote-Sensing Signatures of Life in Disk-averaged Planetary Spectra: 2" b) Absorption properties for CO2. The horizontal lines represent the absorption coefficient above which the atmosphere is strongly absorbing.  The green (orange) rectangle shows that portion of the spectrum where the atmosphere is optically thick for 300 (1200) ppm.  From Pierrehumbert (2011)

 How to get a Runaway?

To get a true runaway greenhouse, you need a conspiracy of solar radiation and the availability of some greenhouse gas in equilibrium with a surface reservoir (whose concentration increases with temperature by the Clausius-Clapeyron relation).  For Earth, or Venus in a runaway greenhouse phase, the condensable substance of interest is water— although one can generalize to other atmospheric agents as well.

The familiar water vapor feedback can be illustrated in Figure 2, whereby an increase in surface temperature increases the water vapor content, which in turn results in increased atmospheric opacity and greenhouse effect.  In a plot of outgoing radiation vs. temperature, this would result in less sensitive change in outgoing flux for a given temperature change (i.e., the outgoing radiation is more linear than one would expect from the σT4 blackbody-relation). 

 

Figure 2: Graph of the OLR vs. T for different values of the CO2 content and relative humidity.  For a fixed RH, the specific humidity increases with temperature. The horizontal lines are the absorbed shortwave radiation, which can be increased from 260-300 W m-2.  The water vapor feedback manifests itself as the temperature difference between b’-b and a’-a, since water vapor feedback linearizes the OLR curve.  Eventually the OLR asymptotes at the Komabayashi-Ingersoll limit.  Adopted from Pierrehumbert (2002)

 

One can imagine an extreme case in which the water vapor feedback becomes sufficiently effective, so that eventually the outgoing radiation is decoupled from surface temperature, and asymptotes into a horizontal line (sometimes called the “Komabayashi-Ingersoll” limit following the work of the authors in the 1960’s, although Nakajima et al (1992) expanded upon this limiting OLR in terms of tropospheric and stratospheric limitations).  In order to sustain the runaway, one requires a sufficient supply of absorbed solar radiation, as this prevents the system from reaching radiative equilibrium.  Once the absorbed radiation exceeds the limiting outgoing radiation, then a runaway greenhouse ensues and the radiation to space does not increase until the oceans are depleted, or perhaps the planet begins to get hot enough to radiate in near visible wavelengths.

 

Figure 3: Qualitative schematic of how the ocean reservoir is depleted in a runaway.  From Ch. 4 of R.T. Pierrehumbert’s Principles of Planetary Climate

 

On present-day Earth, a “cold trap” limits significant amounts of water vapor from reaching the high atmosphere, so its fate is ultimately to condense and precipitate out.  In a runaway scenario, this “cold trap” is broken and the atmosphere is moist even into the stratosphere.  This allows energetic UV radiation to break up H2O and allow for significant hydrogen loss to space, which explains the loss of water over time on Venus.  An intermediate case is the “moist greenhouse” (Kasting 1988) in which liquid water can remain on the surface, but the stratosphere is still wet so one can lose large quantities of water that way (note Venus may never actually encountered a true runaway, there is still debate over this).  Kasting (1988) explored the nature of the runaway /moist greenhouse, and later in 1993 applied this to understanding habitable zones around main-sequence stars.  He found that a planet with a vapor atmosphere can lose no more than ~310 W/m2, which corresponds to 140% of the modern solar constant (note the albedo of a dense H2O atmosphere is higher than the modern), or about 110% of the modern value for the moist greenhouse.

 

Earth and the Runaway: Past and Future

 

Because Earth is well under the absorbed solar radiation threshold for a runaway, water is in a regime where it condenses rather than accumulating indefinitely in the atmosphere.  The opposite is true for CO2, which builds up indefinitely unless checked by silicate weathering or ocean/biosphere removal processes.  In fact, a generalization to the runaway threshold thinking is when the solar radiation is so low, so that CO2 condenses out rather than building up in the atmosphere, as would be the case for very cold Mars-like planets.  Note the traditional runaway greenhouse threshold is largely independent of CO2 (figure 2 & 4; also see Kasting 1988), since the IR opacity is swamped by the water vapor effect.  This makes it very difficult to justify concerns over an anthropogenic-induced runaway.

 


Figure 4: The H2O–CO2 greenhouse. The plot shows the surface temperature as a function of radiated heat for different amounts of atmospheric CO2 (after Abe 1993). The albedo is the fraction of sunlight that is not absorbed (the appropriate albedo to use is the Bond albedo, which refers to all sunlight visible and invisible). Modern Earth has an albedo of 30%. Net insolations for Earth and Venus ca. 4.5 Ga (after the Sun reached the main sequence) are shown at 30% and 40% albedo. Earth entered the runaway greenhouse state only ephemerally after big impacts that generated big pulses of geothermal heat. For example, after the Moon-forming impact the atmosphere would have been in a runaway greenhouse state for ∼2 million years, during which the heat flow would have made up the difference between net insolation and the runaway greenhouse limit. A plausible trajectory takes Earth from ∼100 bars of CO2 and 40% albedo down to 0.1–1 bar and 30% albedo, at which point the oceans ice over and albedo jumps. Note that CO2 does not by itself cause a runaway. Also note that Venus would enter the runaway state when its albedo dropped below 35%.  Se e Zahnle et al 2007

 

This immunity to a runaway will not be the case in the long-term.  In about a billion years, the sun will brighten enough to push us into a state where hydrogen is lost much more rapidly, and a true runaway greenhouse occurs in several billion years from now, with the large caveat that clouds could increase the albedo and delay this process.

Interesting, some (e.g.. Zahnle et al 2007) have argued that Earth may have been in a transient runaway greenhouse phase within the first few million years, with geothermal heat and the heat flow from the moon-forming impact making up for the difference between the net solar insolation and the runaway greenhouse threshold, although this would last for only a brief period of time.  Because the runaway threshold also represents a maximum heat loss term, it means the planet would take many millions of years to cool off following such magma ocean & steam atmosphere events of the early Hadean, much slower than a no-atmosphere case (figure 5).

 

Figure 5: Radiative cooling rates from a steam atmosphere over a magma ocean. The radiated heat is equal to the sum of absorbed sunlight (net insolation) and geothermal heat flow. The plot shows the surface temperature as a function of radiated heat for different amounts of atmospheric H2O (adapted from Abe et al. 2000). The radiated heat is the sum of absorbed sunlight (net insolation) and geothermal heat flow. The different curves are labeled by the amount of H2O in the atmosphere (in bars). The runaway greenhouse threshold is indicated. This is the maximum rate that a steam atmosphere can radiate if condensed water is present. If at least 30 bars of water are present (a tenth of an ocean), the runaway greenhouse threshold applies even over a magma ocean. Note that the radiative cooling rate is always much smaller than the σT4 of a planet without an atmosphere

Conclusions

Venus likely underwent a runaway or “moist greenhouse” phase associated with rapid water loss and very high temperatures.  Once water is gone, silicate weathering reactions that draw down CO2 from the atmosphere are insignificant, and CO2 can then build up to very high values.  Today, a dense CO2 atmosphere keeps Venus extremely hot.

Last updated on 11 April 2011 by Chris Colose.

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Comments 201 to 214 out of 214:

  1. Mike

    15% outside 6-30 isn't trivial in my book.

  2. Mike, your comment about Mauna Kea which is just over 4000 meters high.

    Stop and consider what one would see if you were to look down from that altitude. Here are a series of emission spectra, calculated using Modtran with different lookdown altitudes starting at zero - the surface. All graphs are using US Standard Atmosphere, surface temperature of 288.2 K, clear sky, 400 ppm CO2, 1.7 ppm CH4, 40 ppb Tropospheric O3, standard values for atmospheric water and Stratospheric O3.

    As you go up in level you are seeing the impact of the levels below. When one part of the graph doesn't change between one level and the next, then the atmosphere has become transparent at that wavenumber. Also note the total upwards radiatave flux and how it declines with altitude.

    This is the surface. Flux is 360.472 W/m2. It follows the Planck Curve for 288.2K




    Next 1 km up, looking down. Flux has dropped to 351.994 Some small declines across the water bands, slightly larger effect from the CO2 band. Atmospheric window unchanged.

    Next 2 km. Flux is now 337.55. More activity from water and CO2.

    Next is 4km. Flux now 312.242 W/m2. The CO2 notch becoming more pronounced, Also the water regions are becoming more jagged. I will dscuss this later.

    We have only just reched the altitude of Mauna Kea and activity from below has alreaady reduced the flux compared to the surface by around 48 W/m2. This much has happened before we even consider looking up.

    Next, 8km. Now in the upper troposphere. Flux is now 279.146. CO2 notch very prominent. Around 32 W/m2 decline in flux over the second 4 km contrasted with 48 W/M2 in the first 4 km. Reduced change from the water vapour regions nearere the CO2 regions, but still change below 450 and above 1350 cm-1.

    Next 16 km up. Now we are into the lower Stratosphere. Flux is now 261.782 W/M2. Only around 17.5 W/M2 change over the last 8 km vs around 71 W/M2 in the first 8 km. Essentially no change in any of the water bands above 450 cm-1. Water is only contributing more below 450 cm-1. where it is a stronger absorber. The atmosphere is now quite dry. CO2 is still contributing significantly and the Ozone notch due to statospheric Ozone has kicked in.

     

    Next, 32 km looking down. Now in the upper Stratosphere where air temperatures are starting to rise. Flux is now 258.924. Only a small contribution now, mainly from Ozone. Notice the small spike visible at the bottom of the CO2 notch, and that the bottom of the notch is no longer below the 220 K Plamck curve but actuall is sitting on it. The CO2 band is actually radiating slightly more. This is originating from the warmer upper stratosphere.

     

    Next, 70 km looking down. Flux is now 259.961. Flux has actually increased slightly. Ozone hasn't contributed any more but the CO2 notch is now sitting a little above the 220K planck line and the central spike is higher. CO2 is adding slightly to emissions above the 32 km level.

    Finally, the same 70 km lookdown height, but with a cumulus cloud model added. Flux is now down to 222.909, 37 W/M2 lower! And we can see visibly reduced emissions across the water and atmospheric window regions from 450 to 1350 cm-1.




  3. Summary.

    Total decline in radiative flux between the surface and 70 km -  (360.472 - 259.961) = 100.511 W/M2

    Around 48% of this occurs within the first 4 km, below the height of Mauna Kea!

    Another 32% occurs from 4 to 8 km, only partly due to water vapour.

    The remaining 30% occurs from 8 km up.

    Then adding clouds adds a further 37 W/M2 of reduction.

    And a note about how jagged the curve becomes as we ascend. We are seeing the declining impact of line broadening. At lower altitudes the individual absorption lines are smeared out over each other producing more even absorption/emission. At higher altitudes we start to see the individal spectral lines standing out more distinctly.

  4. Mike

    Finally, contrast this run, again with the Cumulus cloud model looking down from 4 km with the clear sky 4 km lookdown graph above. The presence of the clouds wipes out all structure from below, absorbs everything including in the Atmospheric Window (N-band) and forces emissions across the spectrum to a lower value. The model sets the cloudtops at 2.7 km.

    A lot of stuff happens below the height of Mauna Kea. And since the average altitude of all land is around 850 meters, biasing your thinking around what happens above 4000 metres is missing a hell of a lot of detail.

  5. Mike Hillis @200.

    Your chart is a very bad choice and your interpretaion of it is exceedingly poor. Indeed, you are giving a very good impression of somebody well out of his depth.

    The contention you make @195 is "Upwelling radiation below 6 and above 30, for the purposes of a discussion about the Earth's greenhouse effect and the absorbtion of IR by its atmosphere, is trivial."

    The AGW discussion about the Earth's greenhouse effect is greatly concerned with an effect that will hopefully remain well below 1% of global energy flows. I appreciate that you comments here @SkS strongly suggest you have problems with the concerns others have with AGW but this is SkS and the goal of SkS is to explain what peer reviewed science has to say about AGW. Thus I would suggest that if you want to talk of some part of the planet's energy balance being "trivial," you bear in mind where you are and frame your argument accordingly.

    The chart you present @200 does not well characterise your contended position. Why the two limits 30 microns & 6 microns? They are even strongly asymetric on the chart you chose to present. I feel you are but struggling to defend your statement @181 "Earth doesn't even emit 4 microns" and @190/91 "As for the gish gallop of whether Earth radiates 4 microns:- it doesn't." This was ever a hiding-to-nothing for you. Even the graphic you present @191 to defend your indefensible position graphs the "upwelling" emissions down to 2.5 microns. You were wrong. Get over it.

    You latest chart is a very strange choice. Its origins are as Figure 1 on this webpage. Note that the discussion there for which that Fig 1 is presented is all about solar radiation. It is not about the earth's surface radiation, the "upwelling" stuff withinin your contention and so it is entirely wrong to start waving its Fig 1 as being an authority on that "upwelling" radiation. Mind, that image has spread across the interweb and been used for various purposes, not all of which are well advised. The "upwelling" radiation profile in that graphic is no more than schematic. And obviously so. Note how the peak radation level is at 10 microns. You present this graphic as your authoritative evidence but you grossly misrepresent it. Indeed, I am puzzled as to why you feel the need to source your own graphical representation of the "upwelling" radiation when this comment thread is stacked high with such graphics.

  6. Mike Hillis @200, for what it is worth, 5.77 to 56.58 microns represents a band containing 95% of IR emissions at 288 K, with approximately symetrical quantities of excluded emissions in each tail, so it is probably closer to what you are looking for.  The right tail (in your graph at 200) cuts of at a much lower point in the y-axis than does the left tail, but that is due to the truncated shape of the left tail curve requiring a lower instantanious radiative flux at the cut of to represent the same total radiative flux in the tail.

    Regardless, for the purely technical point as to whether "the atmosphere is almost 100% transparent or largely transparent to a majority of upwelling wavelengths of IR", we only require a precise characterization as to what counts as an upwelling wavelength, and 6 to 30 microns is precise.  It also represents a bandwidth of 24 microns compared to the 5 microns from 8-13 microns, that being the only band of IR radiation with >50% transmittance from surface to space within the 6-30 (or 5.77 to 56.58) micron band.  Ergo for either definition, it is not true that "the atmosphere is almost 100% transparent or largely transparent to a majority of upwelling wavelengths of IR".

    More substantially, nothing in this discussion has called into question Costa and Shine's estimate that the mean clear sky radiation from the surface to space is 66Wm^-2 and that the global mean all sky radiation from the surface to space is 20Wm^-2 (+/-20%), as discussed by MA Rodger @184.  That is, only 28% of clear sky radiation to space directly from the surface, while only 8.5% averaged globally comes directly from the surface.  The percentages are significantly smaller as a fraction of total surface emission.    

  7. Glenn @202


    From your charts there is still plenty of water vapor above Mauna Kea, which doesn't surprise me because of the tropical latitude. The

    Tokunaga charts

    don't resemble the polar charts much in the water vapor Q-band (15-23 um), but they also don't resemble sea level tropical transmittiance charts. From Mauna Kea the Q band transmittance stays around 50% up to 28 um.

  8. As for Venus, let me put this as simply as possible. Venus has an albedo of .65 which means 35% of the sun's radiation is absorbed. We know that only 10% reaches the surface, which means that 25% is absorbed by the atmosphere on the way in. But the atmosphere is not as hot as the surface, which is the hottest place on Venus, even though it only receives 10%. Why? It's obviously because of the lapse rate heat pump I described above. Heat is absorbed by the atmosphere and pumped downward.

    How can you call this scenario a greenhouse effect?

    Response:

    [JH] Please specifiy who you are addressing a question to.

  9. Mike Hillis @208.
    You embark on yet another episode of poorly described nonsense. You now tell us that the surface temperature of Venus results "obviously because of the lapse rate heat pump I described above." I assume you refer to the comment thread at some point "above" your comment @171 when you initiated a long and rather silly argument about the relative size of absorption wavelengths in Earth's atmosphere.
    To recap, at that point, you had just declared that you were "on the same page now" as Glenn Tamblyn @168, a page which Glenn helpfully put in context @170. So this 'above description' cannot be there.
    I appreciate you find such tasks difficult, but you refer to a comment that is a very long way up the comment thread. Thus it is properly beholden on you to indicate you 'above description' with a little more exactitude.

  10. My post was addressed to any reader who argues for a runaway greenhouse effect on Venus, and yes, the lapse rate heat engine I described was affirmed by Glenn Tamblyn @168, though he recanted later.

    Now for some more evidence. Venus spectrum and CO2 bands

    Venus is much hotter than Earth, and radiates a Planck curve with much shorter wavelengths. It appears to peak around 3 or 4 microns with the bulk between 2 and 10 microns. The 15 micron band is barely on the chart. The CO2 absorption bands within this Planck curve are very thin, so I ask again, how can you (we, or anybody) call this scenario a greenhouse effect, especially since most of the sun's radiation which Venus absorbs is absorbed by it's atmosphere on the way in?

  11. Mike Hillis.

    First I need to correct a basic mistake you have made wrt albedo. The figure you have cited of 0.65 is the simple albedo for Venus. The simple average of albedo's across a range of wavelengths. However if we were to use this to calculate how much energy is reflected we would get it wrong because energy isn't constant across all wavelengths obviously, it follows the Planck curve. So if for example albedo was higher at wavelengths that have high energy, near the peak of the Planck curve, this would reflect more energy. So we need to take an average that is weighted by energy density. This is called the Bond Albedo.

    For Venus the Bond Albedo is 0.9.

    Next, the graph you link to isn't what you think it is.

    This is data for the Earth, not Venus!The site you have taken it from is here. As you will note, they don't dispute the role of the GH effect on Venus. However, they credit another site as the source, but do not give all the detail. The original source is here. And this is their discussion of that graph.

    "There are two ways that Venus’ atmosphere could be responsible for keeping the surface hot, either individually or in combination. First, Venus’ atmosphere is very dense, and there is a physical relationship known as the ideal gas law that indicates that gases under pressure tend to be hotter. Second, robotic probes have measured Venus’ atmosphere to be about 97% CO2, and we can see from the image above (click for a larger version) that the absorption spectrum for CO2 (AT EARTH TEMPERATURE AND PRESSURE – VENUSIAN TEMPERATURE AND PRESSURE INCREASES THE WIDTH OF THE ABSORPTION BANDS, MAKING CO2 A STRONGER ABSORBER IN VENUS' ATMOSPHERE THAN IN EARTH'S) strongly overlaps the peak emission spectrum of Venus’ surface. The overlap in the spectra suggests that the greenhouse effect of so much CO2 is the cause" (my emphasis)

    The graph you show is what CO2 does in Earth's atmosphere, not Venus!

    What you are missing in this is referred to in the comment above about temperature and pressure increasing the width of the absorption bands. This factor is profoundly important.

    The actual absorption properties of CO2 (and other GH gases) are that they have a large number (10's of 1000's) if distinct spectral absorption lines, spread over what we call bands. In principle each absorption line would be infinitely narrow, they would by exact wavelengths. However quantum mechanics imposes a minimum width restriction, based on Heisenberg's Uncertainty Principle. But this minimum width for each line is still extremely, extremely narrow.

    A single molecule, at rest, not colliding with anything else would exhibit such idealised narrow absorption lines.

    But two other factors produce what is known as 'line broadening'. This smears each line out, potentially till they overlap and possibly overlap over wider ranges of wavelengths.

    Temperature Broadening is due to Doppler shift. Molecules aren't at rest, and their velocity distribution means that a proportion of molecules absorb at somewhat differing wavelengths from the primary wavelength of each line since the molecule is moving realtive to the photon it absorbs.

    Pressure Broadening is due to the fact that absorption events for a single molecule may occur while that molecule is colliding or in close proximity to another molecule, again shifting the wavelength that the absorption occurs at.

    At sea levle pressures hear on Earth Pressure broadening is already significant, as well as Temperature broadening.

    When we move to Venus, with much higher temperatures,  and pressures vastly higher than Earth, with also hugely higher CO2 proportions, broadening essentially smears absorption across the entire spectrum.

    Mike, I think the mistake you are making is projecting what you know about IR absorption from an Earth context and assuming it is similar on Venus.

    Response:

    [JH] I inadvertently deleted a second response by Glenn Tamblyn. Here is the complete text of it.

    Next Mike, I didn't 'recant' about the Lapse Rate Engine. It is central to understanding what is going on.

    It sems here you haven't fully understood previous comments. You seem to think that the Lapse Rate is a process to be considered instead of the GH Effect.

    As I have said before, the Lapse Rate is a part of the GH effect.

    Let me reiterate.
    The GH effect arises as a result of 3 mechanisms.

    1. Radiative Balance requires that the effective emission altitude (EEA), the altitude at which radiation to space, on average, originates from must tend towards the temperature required for the planet to be in radiative balance.
    2. GH Gases determine the radiative properties of the atmosphere. They determine whatthe effective emission altitude will be.

      These two process tend to drive the EEA to the required emission temperature. On Earth this tends to drive the 5 km level towards a temperature of -18 C. And for Venus this tends to drive the 50+ km level to a temperature between -80 and -90 C.
    3. The Lapse Rate Engine then drives other layers above and below the EEA to matching temperatures.

    So for example, on Earth Radiative Balance and GH Gases drive the 5 km layer towards -18C. The Lapse Rate engine then drives the surface towards + 15 C and the 10km level towards -41C.

    On Venus Radiative Balance and GH Gases drive the 50+ km layer towards -80 - -90 C, and the Lapse Rate drives the surface towards 500 C warmer than this.

    The Lapse Rate is a part of the GH Effect!

    And your comment about incoming solar radiation being absorbed by the atmosphere. So what.

    1/3rd of solar energy absorbed on Earth is absorbed in the atmosphere. It doesn't matter whether absorption happens at the surface or in the atmosphere. The air circulation behind the Lapse Rate redistributes energy within the atmosphere, irrespective of whether it was originally absorbed at the surface or in the atmosphere, to produce a temperature gradient, and allow the EEA to tend towards the needed balance temperature.

  12. Mike Hills @210.

    You still fail to describe the workings of your proposed Lapse Rate Heat Engine. We can see from Glenn Tamblyn's comments @211/212 were he stands on the matter and that it is incompatable with your comments @208/210. Yet #208/210 does not give "any reader who argues for a runaway greenhouse effect on Venus" the slightest inkling of what you propose. In truth, anyone familiar with your input into this comment thread would still struggle, unable to glean whether you still incorporate any or all of the various fallacies you presented variously down this thread. The Unified Theory of Climate from denialists Nikolov & Zeller whose work you cited @121? A katabatic-type mechanism as you proposed @132, which is strangely a mechanism that does the exact opposite of what you appear to propose? The vertical-means-down fallacy you use at, for instance, @158? Or your fallacy that the surface of Venus would require more direct solar heating than it does so as to be hotter than the insulating atmosphere above it, as described say @208? How many of these fallacies do you still use to support your proposed Lapse Rate Heat Engine?

    Simply, nobody else truly knows what it is your trying to say. Can you give it your best shot?

  13. Mike Hillis.

    In your posts @143 and @147 you seem to agree with me that adiabatic processes can’t increase the average temperature of an atmosphere, but merely redistribute it.
    If the average temperature is determined by absorbed insolation only, one would expect the Venusian atmosphere with its very high albedo to be colder than the Earth’s, right?
    So, how do you explain this temperature/pressure profile?

    Height (km)Temp (C)Pressure (atm.)
    046292.10
    1038547.39
    2030622.52
    302229.851
    401433.501
    50751.066
    60-100.2357
    70-430.0369
    80-760.00476
    90-1040.000374
    100-1120.0000266

    Source: Wikipedia

    As you see, about 50% of Venus’ atmosphere (by mass) is hotter than 385oC, nearly 90% is hotter than 222oC and nearly 99.9% is warmer than the average of the terrestrial atmosphere (about -20oC).
    If you calculate a "mass-weighted" average temperature based on this table the result is about 350oC. This is obviously much, much hotter than can be explained by any redistribution of heat. Something else must be going on!
    The graph below gives a clear indication of what this "something" is.

    IR radiation from Venus

    Only a very tiny fraction (~1 %) of the nearly 16,000 watts/m2 of IR radiation from the surface escapes to space. The lower and middle atmosphere is almost completely opaque to IR, so virtually all the heat loss to space happens from the very thin and cold upper layers that are more or less transparent. This raising of the effective emission altitude to colder, less emitting layers of the atmosphere is the very core of the atmospheric greenhouse effect. The lapse rate engine is not an alternative to this, but a crucial part of it, as Glenn Tamblyn has explained.
    An isothermal atmosphere (same temperature at all altitudes) full of greenhouse gases couldn’t raise the surface temperature because the effective emission altitude wouldn’t matter for the heat loss to space. And an atmosphere with normal lapse rate but no greenhouse gases would be transparent to IR and thus let the surface radiate directly to space as if the atmosphere wasn’t there at all.

  14. Mike Hillis

    You might also be interested in this chapter by Crisp & Titov about the development of the understanding of thermal balance and radiative trannsfer in the Venusian atmosphere. The book was published in 1997 so more has happened since.

    There are a number of extra factors that need to be consered.

    • Obviously pressure and temperature broadening of the existing absorption lines/bands.
    • Also Collision Induced Absorption. This is where molecules that may not otherwise be absorbers, or wavelengths where absorption may not normally occur at all become able to absorb during the transient time when a collision is occurring. For example, Nitrogen (N2) is the major GH gas on Titan due to CIA and Nitrogen/Hydrogen (N2/H2) collisions may have been a contributor to the GH Effect in the Early Earth atmosphere.
    • Scattering, which is negligible in the IR in Earth's atmosphere needs to be included when dealing with the much denser Venusian atmosphere.
    • Continuum Absorption is another mode of absorption that can occurr where a molecule absorbs over a continuus spectrum. H2O continuum absorption needs to be included when considering H2O vapour on Earth. CO2 also exhibits continuum absorption on Venus. At the time of writing of this book, the understanding of continuum absorption was still developing. It is better understood today.
    • Spectral data from the HiTran spectroscopic database doesn't apply for Venus, what is used is the HiTemp database of data for higher temperatures.

    Consider Mike. Gases absorb in lines/bands but solids and liquids absorb/emit with continuous spectra. Venus has an atmospheric density nearly 100 times that of Earth. That means it has a density nearly 10% of liquid water. Is the lower Venusian atmosphere a thick gas or a thin liquid? At what density does the transition from discrete band/line absorption to continuous whole-of-spectra absorption occur?

  15. Elsewhere, EE writes:

    "Regarding question by mj at 43, I think skeptics are correct in that mentioning Venus is not very useful in advancing GW argument. By using the same albedo/black body radiation that was used for Mars..... Venus is 67M miles vs 93M miles so it absorbs twice the solar radiation. If Venus had the same albedo and same greenhouse as earth, it would still be unbearably hot. About 185 degrees Fahrenheit....too hot for me. Greenhouse or not, I'd be dead on that planet. "

    I am not sure what is meant by "the same greenhouse effect", but it is interesting to explore the difference between the actual Venus, and Venus with an Earthlike and with zero albedo, all with no greenhouse effect.

    First, the mean incoming solar radiation for Venus an albedo of 0, 0.306 (ie, Earthlike) and 0.77 (its current value) are 650.4, 451.4 and 149.6 W/m^2 respectively.  As it happens, for a body with liquid water, the water vapour feedback imposes a cap on OLR on the assumption that there is such a thing as the greenhouse effect.  That cap arises because, as temperatures rise, the water vapour feedback becomes stronger until a point is reached were the increase in the water vapour feedback compensates for any increase in outgoing radiation from the surface, so that while the temperature may rise, the OLR does not.  That cap, for Earth is approximately 385 W/m^2 (Nakajima et al, 1992), and would be similar for Venus.  Indeed, prior to the formation of Venus very thick atmosphere, it would have been slightly lower. 

    Crucially, for Venus with 0 or an Earthlike albedo, that cap is less than the globally averaged incoming insolation.  That means that for Venus with Earthlike albedo, there is an excess of about 70 W/m^2 between the energy Venus would recieve from the Sun, and the amount it would radiate to space.  That extra 70 W/m^2 must go into heating the surface, first by boiling away any liquid water on the surface, and then by raising the temperatures well above anything like the temperatrures we are used to.

    That, in essence, is the runaway greenhouse effect.  It cannot exist without a greenhouse effect, but a Venus with Earthlike albedo and zero initial greenhouse effect cannot avoid it.

    In some respects, even more interesting is the current very high upward surface radiation coupled with the very low OLR found on Venus, or in simpler terms, the fact that Venus with less recieved radiation than Earth, has a surface hot enough to melt lead.  Given that Venus is less dense than Earth, and consequently does not have as much radioactive material, that cannot be due to high geothermal heat flux.  Consequently it is inexplicable without a greenhouse effect.

    These two crucial facts about Venus show that the greenhouse effect is real, and that it is potent.  There exist no other viable explanations; and certainly none proposed by AGW "skeptics" (whose explanations tend to start by ignoring the conservation of energy).  In science, a theory is only as good as its ability to explain things better than its competitors.  In this case the greenhouse effect is an efficient explanation of both the current state of Venus, and how it got into that state.  It has no viable competition in that role.  This, rather than our relative comfort on Venus with no greenhouse effect (or a much reduced greenhouse effect) and Earthlike albedo is what makes mention of Venus a good argument in favour of the theory of the greenhouse effect.

    Granted it will not persuade all AGW "skeptics", but that is because most AGW "skeptics" have decided to make their beliefs on AGW immune to evidence.  Nothing is a good argument for those with minds so closed.

  16. John and Others: I apologize - this may already be answered in the 5 pages of posts, but that is rough sledding.

    I have read a number of papers on the runaway greenhouse effect (Hastings, 1988 and others) and can see how water vapor plays a role in spinning up the temps – a fascinating process. However, once the water is expensed, is the system left in a state of equilibrium? I asked because I tried to apply a simple one-layer equilibrium energy balance model to Venus. The TOA is fine, but I am not even in the ballpark on the surface temperature. A full radiative transfer model will likely get to a better answer, but I am wonder if you have any idea what assumptions or basic physics is missing from those models that they don’t hold on Venus?

    Many thanks,

    M

  17. MVW @216:

    1)  The runaway greenhouse effect is premised on two essential facts.  First, increasing water vapour in the atmosphere, as with any GHG, decreases the total amount of Outgoing Longwave Radiation (OLR) for a given Global Mean Surface Temperature (GMST).  Second, if OLR is less than the Net Incoming Solar Radiation (NISR), surface temperatures will increase.  The way the runaway greenhouse effect works is that, for a given atmospheric pressure, and GMST, as surface temperature increases the amount of evaporated H2O increases at a sufficient rate that the OLR stays constant.  Because it stays constant, the gap between OLR and NISR cannot be closed while this situation occurs, and the temperatures must keep on increasing.

    Eventually, of course, if this situation arises, the oceans will boil dry.  At that point, the gap between OLR and will still exist, but can begin to close.  That is, the system is not in a state of equilibrium at that point, but can finally achieve it over the course of time.  (Technically it does not achieve equilibrium, but quasi equilibrium, ie, equilibrium approximated over a short time period of at least a year, given that solar insolation is not constant throughout the year.)

    2)  Energy transfers within the atmosphere are not restricted to just radiation.  Therefore a model of atmospheric temperature that relies solely on radiative energy transfers will not accurately estimate surface temperatures.  This was first shown by Manabe and Strickler (1964), from whom this figure comes:

     

    As you can see, using a simple, one dimensional model they showed that if radiative transfers within the atmosphere were the sole source of energy transfers, that would result in a much warmer surface temperature (approx 30oC warmer).  For Earth, energy transfers by convection and latent heat need to be accounted for in addition to those by radiation.  On Venus, because of the absence of water vapour, only energy transfers by convection and radiation need to be accounted for.  In a full Global Circulation Model, lateral energy tranfers also need to be accounted for.

    The temperature profile of Venus atmosphere has been modeled.  As one example, here is a one dimensional model equivalent to that from Manabe and Strickler from Tomasko et al (1980):

    For what it is worth, here is a 2017 paper on a full Venus GCM (pay wall for full paper), and a 2017 update on another full Venus GCM.

  18. Thanks Tom.  This is helpful.  A couple additional thoughts.  As you note, the purely radiative model will produce a surface temperature that is 30 degrees warmer than a more complete model.  Just applying a simple energy balance model to Venus gives a surface temperature that is cooler.  I just now found a paper  by Titov and others "Radiation in the Atmosphere" and they noted (as does original article here) that very little of the NISR reaches the surface of Venus.  It struct me that Venus is heated from the top rather than the bottom, so it is more like the ocean than the atmospheric situation on Earth.  But that is just a thought.

    Mike

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