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Books on the topic 'Solar air heating'

Author: Grafiati

Published: 4 June 2021

Last updated: 14 February 2022

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1

Zhongguo tai yang neng jian zhu ying yong fa zhan yan jiu bao gao ke ti zu, ed. Zhongguo tai yang neng jian zhu ying yong fa zhan yan jiu bao gao. Beijing: Zhongguo jian zhu gong ye chu ban she, 2009.

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2

EC Contractors' Meeting (1986 Brussels, Belgium). Solar energy applications to buildings and solar radiation data: Proceedings of the EC Contractors' Meeting held in Brussels, Belgium, 13 and 14 November 1986. Dordrecht: D. Reidel Pub. Co. for the Commission of the European Communities, 1987.

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3

Vu, Brigitte. L'habitat passif. Paris: Eyrolles, 2008.

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4

Kachadorian, James. The passive solar house. White River Junction, Vt: Chelsea Green Pub. Co., 1997.

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5

Sklar, Scott. Consumer guide to solar energy: Easy and inexpensive applications for solar energy. 2nd ed. Chicago: Bonus Books, 1995.

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6

Sklar, Scott. Consumer guide to solar energy: Easy and inexpensive applications for solar energy. Chicago, IL: Bonus Books, Inc., 1991.

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7

Sklar, Scott. Consumer guide to solar energy: Easy and inexpensive applications for solar energy. Chicago: Bonus Books, 1991.

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8

Crume, Richard V. The simply solar house: Green building on a budget. Duvall, Wash: Counterbalance Books, 2007.

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9

Alain, Guinebault, ed. Solar heating in cold regions: A technical guide to developing country applications. London: Intermediate Technology Publications, 1996.

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10

Sklar, Scott. Consumer guide to solar energy: New ways to lower utility costs, cut taxes, and take control of your energy needs. 3rd ed. Chicago: Bonus Books, 2002.

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11

Solar technologies for buildings. Chichester: Wiley, 2003.

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12

Eicker, Ursula. Solar Technologies for Buildings. New York: John Wiley & Sons, Ltd., 2006.

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13

Chandra, Subrato. Cooling with ventilation. Golden, Colo: Solar Energy Research Institute, 1987.

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14

Ewing, Rex A. Got sun? go solar: Get free renewable energy to power your grid-tied home. Masonville, CO: PixyJack Press, 2005.

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15

Ewing, Rex A. Got sun? go solar: Get free renewable energy to power your grid-tied home. Masonville, CO: PixyJack Press, 2005.

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16

Andrén, Lars. Solar installations: Practical applications for the built environment. London: James & James (Science Publishers), 2003.

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17

Got sun? go solar: Harness nature's free energy to heat and power your grid-tied home. 2nd ed. Masonville, CO: PixyJack Press, 2009.

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18

The New Solar Electric Home: The Photovoltaics How-To Book. S.l: aatec Publications, 2005.

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19

1969-, Mösle Peter, and Schwarz Michael 1961-, eds. Green building: Guidebook for sustainable architecture. Heidelberg: Springer, 2010.

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20

1969-, Mösle Peter, and Schwarz Michael 1961-, eds. Green building: Konzepte für nachhaltige Architektur. München: Callwey, 2007.

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21

1945-, Hastings Robert, ed. Solar air systems--built examples. London: James & James, 1999.

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22

Wang, Ruzhu, and Tianshu Ge. Advances in Solar Heating and Cooling. Elsevier Science & Technology, 2016.

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23

Solar Heating and Cooling Systems: Design for Australian Conditions. Elsevier Science Publishing Company, 1985.

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24

Corporation, Carrier, ed. HVAC installation procedures. [USA]: Carrier Corp., 1997.

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25

G, Löf George O., ed. Active solar systems. Cambridge, Mass: MIT Press, 1993.

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26

V, Sarnat͡s︡kiĭ Ė, Chistovich S. A, and Avezov R. R, eds. Sistemy solnechnogo teplo- i khladosnabzhenii͡a︡. Moskva: Stroĭizdat, 1990.

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27

Institute, Environmental Law. Legal Barriers to Solar Heating and Cooling of Buildings. Books for Business, 2000.

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28

Energy Efficient Buildings With Solar And Geothermal Resources. John Wiley & Sons Inc, 2014.

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29

Eicker, Ursula. Energy Efficient Buildings with Solar and Geothermal Resources. Wiley & Sons, Incorporated, John, 2014.

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30

W, Neal R., Wood R. A, McCabe T. F, JBF Scientific Corporation, and Electric Power Research Institute, eds. Thermal performance and economic benefits of residential passive solar systems. Palo Alto, Calif: Electric Power Research Institute, 1985.

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31

Kachadorian, James. Passive Solar House: The Complete Guide to Heating and Cooling Your Home. Chelsea Green Publishing Company, 2006.

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32

Hayama, Shigeso. Tenjo reidanbo no susume: Kankyo enerugi jidai ni mukete (Chikuma raiburari). Chikuma Shobo, 1990.

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33

Drost, M. K. Volumetric receiver development: A heat transfer and design evaluation of an advanced air heating solar thermal central receiver concept. 1985.

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34

1956-, Santamouris M., ed. Solar thermal technologies for buildings: The state of the art. London: James & James (Science Publishers) Ltd., 2003.

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35

A, Beattie Donald, ed. History and overview of solar heat technologies. Cambridge, Mass: MIT Press, 1997.

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36

The Simply Solar House: Green Building on a Budget. Counterbalance Books, 2007.

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37

Building Services & Equipment Vol. 3: Pipe-Sizing, Drainage, Electrical Installations, Ventilation, Air Conditioning, Lighting & Solar Heating. 3rd ed. Trans-Atlantic Publications, 1994.

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38

Guinebault, Alain, and Jean-Francois Rozis. Solar Heating in Cold Regions: A Technical Guide to Developing Country Applications. Practical Action, 1996.

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39

Solar energy in building renovation. London: James & James, 1997.

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40

R, Mancini T., Worek William M, American Society of Mechanical Engineers. Winter Meeting, and American Society of Mechanical Engineers. Solar Energy Division., eds. Solar energy in the 1990s: Presented at the Winter Annual Meeting of the American Society of Mechanical Engineers, Dallas, Texas, November 25-30, 1990. New York, N.Y: The Society, 1990.

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41

Chandra, Subrato. Cooling with ventilation. Solar Energy Research Institute, 1986.

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42

Hacyan, M. Solar Energy Based Heating and Air Conditioning for the Pernod Plant in Dardilly, France (Commission of the European Communities). European Communities, 1986.

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43

Oregon. Dept. of Energy., ed. Oregon residential energy tax credit: Tax credits for premium efficiency appliances, heating, ventilization, air conditioning systems, premium efficiency water heaters, hybrid and alternative fuel vehicles, solar and geothermal heating systems, solar and wind systems. Salem, OR: Oregon Dept. of Energy, 2004.

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44

Ewing, Rex A. Got Sun? Go Solar: Get Free Renewable Energy to Power Your Grid-Tied Home. PixyJack Press, LLC, 2005.

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45

Davidson, Joel, and fran Orner. New Solar Electric Home: The Photovoltaics How-to Handbook. 3rd ed. Stonefield Publishing, 2005.

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46

Yang, Kun. Observed Regional Climate Change in Tibet over the Last Decades. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190228620.013.587.

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The Tibetan Plateau (TP) is subjected to strong interactions among the atmosphere, hydrosphere, cryosphere, and biosphere. The Plateau exerts huge thermal forcing on the mid-troposphere over the mid-latitude of the Northern Hemisphere during spring and summer. This region also contains the headwaters of major rivers in Asia and provides a large portion of the water resources used for economic activities in adjacent regions. Since the beginning of the 1980s, the TP has undergone evident climate changes, with overall surface air warming and moistening, solar dimming, and decrease in wind speed. Surface warming, which depends on elevation and its horizontal pattern (warming in most of the TP but cooling in the westernmost TP), was consistent with glacial changes. Accompanying the warming was air moistening, with a sudden increase in precipitable water in 1998. Both triggered more deep clouds, which resulted in solar dimming. Surface wind speed declined from the 1970s and started to recover in 2002, as a result of atmospheric circulation adjustment caused by the differential surface warming between Asian high latitudes and low latitudes.The climate changes over the TP have changed energy and water cycles and has thus reshaped the local environment. Thermal forcing over the TP has weakened. The warming and decrease in wind speed lowered the Bowen ratio and has led to less surface sensible heating. Atmospheric radiative cooling has been enhanced, mainly through outgoing longwave emission from the warming planetary system and slightly enhanced solar radiation reflection. The trend in both energy terms has contributed to the weakening of thermal forcing over the Plateau. The water cycle has been significantly altered by the climate changes. The monsoon-impacted region (i.e., the southern and eastern regions of the TP) has received less precipitation, more evaporation, less soil moisture and less runoff, which has resulted in the general shrinkage of lakes and pools in this region, although glacier melt has increased. The region dominated by westerlies (i.e., central, northern and western regions of the TP) received more precipitation, more evaporation, more soil moisture and more runoff, which together with more glacier melt resulted in the general expansion of lakes in this region. The overall wetting in the TP is due to both the warmer and moister conditions at the surface, which increased convective available potential energy and may eventually depend on decadal variability of atmospheric circulations such as Atlantic Multi-decadal Oscillation and an intensified Siberian High. The drying process in the southern region is perhaps related to the expansion of Hadley circulation. All these processes have not been well understood.

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47

Trieloff, Mario. Noble Gases. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190647926.013.30.

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This is an advance summary of a forthcoming article in the Oxford Encyclopedia of Planetary Science. Please check back later for the full article.Although the second most abundant element in the cosmos is helium, noble gases are also called rare gases. The reason is that they are not abundant on terrestrial planets like our Earth, which is characterized by orders of magnitude depletion of—particularly light—noble gases when compared to the cosmic element abundance pattern. Indeed, such geochemical depletion and enrichment processes make noble gases so versatile concerning planetary formation and evolution: When our solar system formed, the first small grains started to adsorb small amounts of noble gases from the protosolar nebula, resulting in depletion of light He and Ne when compared to heavy noble gases Ar, Kr, and Xe: the so-called planetary type abundance pattern. Subsequent flash heating of the first small mm to cm-sized objects (chondrules and calcium, aluminum rich inclusions) resulted in further depletion, as well as heating—and occasionally differentiation—on small planetesimals, which were precursors of larger planets and which we still find in the asteroid belt today from where we get rocky fragments in form of meteorites. In most primitive meteorites, we even can find tiny rare grains that are older than our solar system and condensed billions of years ago in circumstellar atmospheres of, for example, red giant stars. These grains are characterized by nucleosynthetic anomalies and particularly identified by noble gases, for example, so-called s-process xenon.While planetesimals acquired a depleted noble gas component strongly fractionated in favor of heavy noble gases, the sun and also gas giants like Jupiter attracted a much larger amount of gas from the protosolar nebula by gravitational capture. This resulted in a cosmic or “solar type” abundance pattern, containing the full complement of light noble gases. Contrary to Jupiter or the sun, terrestrial planets accreted from planetesimals with only minor contributions from the protosolar nebula, which explains their high degree of depletion and basically “planetary” elemental abundance pattern. Indeed this depletion enables another tool to be applied in noble gas geo- and cosmochemistry: ingrowth of radiogenic nuclides. Due to heavy depletion of primordial nuclides like 36Ar and 130Xe, radiogenic ingrowth of 40Ar by 40K decay, 129Xe by 129I decay, or fission Xe from 238U or 244Pu decay are precisely measurable, and allow insight in the chronology of fractionation of lithophile parent nuclides and atmophile noble gas daughters, mainly caused by mantle degassing and formation of the atmosphere.Already the dominance of 40Ar in the terrestrial atmosphere allowed C. F v. Weizsäcker to conclude that most of the terrestrial atmosphere originated by degassing of the solid Earth, which is an ongoing process today at mid ocean ridges, where primordial helium leaves the lithosphere for the first time. Mantle degassing was much more massive in the past; in fact, most of the terrestrial atmosphere formed during the first 100 million years of Earth´s history, and was completed at about the same time when the terrestrial core formed and accretion was terminated by a giant impact that also formed our moon. However, before that time, somehow also tiny amounts of solar noble gases managed to find their way into the mantle, presumably by solar wind irradiation of small planetesimals or dust accreting to Earth. While the moon-forming impact likely dissipated the primordial atmosphere, today´s atmosphere originated by mantle degassing and a late veneer with asteroidal and possibly cometary contributions. As other atmophile elements behave similar to noble gases, they also trace the origin of major volatiles on Earth, for example, water, nitrogen, sulfur, and carbon.

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