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#RadiativeForcing

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HistoPol (#HP) 🏴 🇺🇸 🏴<p><span class="h-card" translate="no"><a href="https://troet.cafe/@worthuelse" class="u-url mention" rel="nofollow noopener" target="_blank">@<span>worthuelse</span></a></span> </p><p><a href="https://mastodon.social/tags/Methan" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>Methan</span></a> <a href="https://mastodon.social/tags/GHGs" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>GHGs</span></a> <br><a href="https://mastodon.social/tags/Oxidation" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>Oxidation</span></a> <a href="https://mastodon.social/tags/THG" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>THG</span></a></p><p>(2/n)</p><p>...Methan in CO2 umwandelt, wird das Treibhausgasproblem durch a) den kumulativen Effekt und b) die Transformation in Wasser und Kohlendioxid als noch potentere Treibhausgase noch größer (s/:super!/s)</p><p>ad b) Keine Ahnung, ob es das schon gibt, aber müsste man aufgrund der verschiedenen Treibhausgase und des <a href="https://mastodon.social/tags/RadiativeForcing" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>RadiativeForcing</span></a>-Efekts 1) nicht Umdenken und 👉von "Treibhausgasäquivalenten" reden? 👈<br>Die "Hälfte" von der du da redest, wird...</p>
Dr. John Barentine FRAS<p>New research on the potential for radiative forcing of the climate from satellite re-entry debris: "We find that reentry-ablated alumina particles have ... a cooling radiative forcing of approximately -0.378mW/m2."</p><p><a href="https://essopenarchive.org/doi/full/10.22541/essoar.170110669.90121203" rel="nofollow noopener" translate="no" target="_blank"><span class="invisible">https://</span><span class="ellipsis">essopenarchive.org/doi/full/10</span><span class="invisible">.22541/essoar.170110669.90121203</span></a></p><p><a href="https://astrodon.social/tags/Space" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>Space</span></a> <a href="https://astrodon.social/tags/Satellites" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>Satellites</span></a> <a href="https://astrodon.social/tags/SpaceSustainability" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>SpaceSustainability</span></a> <a href="https://astrodon.social/tags/RadiativeForcing" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>RadiativeForcing</span></a> <a href="https://astrodon.social/tags/Geoengineering" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>Geoengineering</span></a></p>
Daniele de Rigo<p>10/</p><p>"This strongly absorbing organic aerosol species is water insoluble, resists daytime photobleaching and increases in absorptivity with night-time atmospheric processing" [3] so that the "parameterizations of brown carbon in climate models" may "need to be revised to improve the estimation of <a href="https://hostux.social/tags/smoke" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>smoke</span></a> <a href="https://hostux.social/tags/aerosol" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>aerosol</span></a> <a href="https://hostux.social/tags/RadiativeForcing" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>RadiativeForcing</span></a> and associated <a href="https://hostux.social/tags/warming" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>warming</span></a>", with potential consequences for the current <a href="https://hostux.social/tags/ClimateChange" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>ClimateChange</span></a> estimates</p>
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