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This article is or was the subject of a Wiki Education Foundation-supported course assignment. Further details are availableon the course page. Student editor(s):Dtolson1. Peer reviewers:Jmead2,65Eq.
Above undated message substituted fromTemplate:Dashboard.wikiedu.org assignment byPrimeBOT (talk)03:24, 17 January 2022 (UTC)[reply]
CiaoMente et malleo, good job, as usual!
May I suggest to give some lines of introduction, and link the article toMarine isotope stage? The average reader would better understand what is this article about.
Anyways, I'm happy you are doins such a good job, keep on going!
--Kaapitone08:00, 20 May 2007 (UTC)[reply]
(copied from main MIS article talk) When somebody next edits this, please take a look athttp://www.whoi.edu/pclift/Ruddiman.pdf, orhttp://hol.sagepub.com/content/21/5/865.full.pdf+html by Ruddiman, Kutzbach, Vavrus inThe Holocene Aug 2011. I think they make a pretty good case (or at least, raise some good red flags) about Stage 11 being considered the best analog of Stage 1., but rather being an outlier in multiple ways.JohnMashey (talk)22:45, 13 January 2014 (UTC)[reply]
I chose to expand on the article for Marine Isotope Stage 11 (MIS 11) to include sections for potential causes and why it is currently considered an analog for Holocene climate. The current article for MIS 11 mentions in the lede that there there may be some correlation between climatic elements of MIS 11 and the Holocene, but there is no exploration of why that is. Additionally, the article focuses on what we know of climate characteristics from proxy records, but does not discuss the lead in processes or what might have caused MIS 11 to last longer than most other interglacial periods in the climate record. I might begin by discussing those climate elements (ice volume, ocean temperature, etc) that are known to be similar and what proxies tell us that. Next I would add a discussion of why MIS 11 is theorized to be an analog for the future Holocene/Anthropocene climatic trend and how our observation of this period in the past can help us model predictions for the future. Finally, I would consider changing or elaborating on this lede, particularly to address the comparison of MIS 5 to MIS 11 which I have not been able to find any evidence for yet. This will require more research but it may be erroneous or outdated information.
Potential Sources (to be expanded):
Dtolson1 (talk)18:18, 8 May 2017 (UTC)[reply]
When I read the introduction I felt the same way, the author mentions a relation to present day climate but does not really elaborate. Perhaps you can also add a better graph of temperature variability (Vostok) centered in MIS11, and perhaps if available other proxies that show Carbon and Sea level variability during MIS11. You might also consider the "Red flags" the previous reviewer left here, and adding a couple lines in the main "Marine Isotope Stages" topic. Cheers!65Eq (talk)65Eq—Precedingundated comment added16:14, 15 May 2017 (UTC)[reply]
I have completely revised this article from its previous form. I welcome any suggestions or revisions on the new content.Dtolson1 (talk)23:17, 12 June 2017 (UTC)[reply]
At the end of the section Astronomical features a citation is needed. I believe you are looking for Berger and Loutre 2002 "An Exceptionally Long Interglacial Ahead?"— Precedingunsigned comment added by98.193.221.114 (talk)05:31, 30 August 2018 (UTC)[reply]
Glad to see the Wikipedia community is so actively gatekeeping! You know, a professor reviewed my edits to this article and did not have the same reaction y’all did. But we aren’t bigshot Wiki editors so what do we know. I put time and effort into those edits, but if they are TRULY valueless then y’all should point this out to the general Wiki community and work to end the practice of assigning poorly-maintained Wiki articles for students to edit and fill out.Dtolson1 (talk)16:31, 3 January 2019 (UTC)[reply]
Please bear with me, I will 1st give a theoretical reason why CO2 is irrelevant, then 2nd I will give an empirical proof:
1.) The CO2 contribution to atmospheric gases @ .04% is minimal, compared with the main constituents N2 @ 78%, O2 @ 21% and Ar @1%. While it is true that IR band radiation absorbed by atmospheric CO2 will be passed on by Brownian motion to N2, O2 and Ar, the amount is very small due to CO2 presence at a low .04%.
2.) During the recent solar eclipse Aug 21, 2017 we could observe the chill of the air almost immediately, within minutes. My own location was particularly suitable although >250 miles from the 70 mile strip of totality, we still had 87% coverage of the Sun's disk by the Moon. There was brilliant sunshine and calm air before and after the eclipse. At about 12:00 CST, my electronic backyard thermometer (radio) showed the temperature dropping from 92 F to 86 F almost instantaneously, within a few minutes. Thereafter, temperature climbed to 94 F by 2:30 CST. The air was dry and no clouds present with low relative humidity, water vapor was scarce. The drop in temperature meant that vast amounts of thermal energy had been lost to space by IR band radiation (the only means available in the absence of heat conduction or convection). Ergo: The tiny amount of CO2 was of no avail when it came to stopping IR loss to space.
In conclusion, it is time to face the reality that CO2 is irrelevant. Recent studies show anthropogenic climate change has far more to do with aerosols, cloudiness and albedo. Climate experts have pointed this out for over a decade, esp. in Japan. Humans, who are largely carbon, should not have to worry about being subject to carbon sequestration, or replaced by automata and robotic AI.Kollauwanderer (talk)17:14, 24 September 2017 (UTC)[reply]