Encyclopedia of Environmental Microbiology 2003
DOI: 10.1002/0471263397.env178
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Desert Environments: Soil Microbial Communities in Hot Deserts

Abstract: Soil Water Potential Desert Soil Microbial Abundance Spatial and Temporal Distributions Diversity of Desert Soil Microbes Adaptations to Desert Soil Conditions Practical Applications

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Cited by 9 publications
(7 citation statements)
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“…For example, there is some evidence that environments in which overall microbial abundance is lower have more spatially- and temporally diverse communities ( e.g. , Banerjee et al , 2011 and references reviewed in Kieft, 2003 ).…”
Section: Introductionmentioning
confidence: 99%
“…For example, there is some evidence that environments in which overall microbial abundance is lower have more spatially- and temporally diverse communities ( e.g. , Banerjee et al , 2011 and references reviewed in Kieft, 2003 ).…”
Section: Introductionmentioning
confidence: 99%
“…Therefore, the correlations between the bacterial community and C and N parameters may be location‐specific, and the bacterial community may not be the main driver of the organic C and N cycle under native Caatinga vegetation and grazing exclusion. However, members of the fungal community are more tolerant to dry conditions than bacteria (Kieft, 2003), and it highlights the importance of further studies regarding fungal communities in the Caatinga biome and their relationships with soil functions, especially mycorrhizal fungi (Guo et al, 2016; Macdonald et al, 2015). In addition, by studying both bacteria and fungi, Xun et al (2018) demonstrated that the relationships between the activity of C‐decomposing enzymes and microbial abundance are more important for the fungi community, especially in C‐recalcitrant turnover, while bacteria are more important in labile‐C turnover.…”
Section: Discussionmentioning
confidence: 99%
“…Such acidophilic archaea are among the oldest organisms on Earth (Woese, 1998). Similarly, >75% sulfuric acid corresponds to a very low water activity (a w ) of <0.02 (Gentry and Dahlgren, 2019), substantially below that of even the most saturated brines (Bolhuis et al, 2006) and at best on par with Earth's driest deserts (Kieft, 2003). Sulfuric acid abundances in Venus' aerosols are not based on direct measurements but rather from the index of refraction deduced from polarization data (Hansen and Hovenier, 1974;Rossi et al, 2015), and optical glory feature data (Markiewicz et al, 2014), along with computational simulations (Krasnopolsky, 2015) and compatible with vapor abundances determined from radio occultation profiles (Steffes and Eshleman, 1982).…”
Section: Potential For a Habitable Zone For Polyextremophiles In Venus' Cloudsmentioning
confidence: 99%