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dc.contributor.authorKankelborg, Charles C.
dc.contributor.authorCourrier, Hans T.
dc.contributor.authorDe Pontieu, Bart
dc.contributor.authorWülser, Jean-Pierre
dc.date.accessioned2019-03-27T19:25:25Z
dc.date.available2019-03-27T19:25:25Z
dc.date.issued2018-09
dc.identifier.citationCourrier, Hans, Charles C. Kankelborg, Bart De Pontieu, and Jean-Pierre Wülser. "An on Orbit Determination of Point Spread Functions for the Interface Region Imaging Spectrograph.." Solar Physics 293, no. 9 (September 2018). DOI:10.1007/s11207-018-1347-9.en_US
dc.identifier.issn0038-0938
dc.identifier.urihttps://scholarworks.montana.edu/xmlui/handle/1/15349
dc.description.abstractDecades of research into the Bacteria and Archaea living in geothermal spring ecosystems have yielded great insight into the diversity of life and organismal adaptations to extreme environmental conditions. Surprisingly, while microbial eukaryotes (protists) are also ubiquitous in many environments, their diversity across geothermal springs has mostly been ignored. We used high-throughput sequencing to illuminate the diversity and structure of microbial eukaryotic communities found in 160 geothermal springs with broad ranges in temperature and pH across the Taupō Volcanic Zone in New Zealand. Protistan communities were moderately predictable in composition and varied most strongly across gradients in pH and temperature. Moreover, this variation mirrored patterns observed for bacterial and archaeal communities across the same spring samples, highlighting that there are similar ecological constraints across the tree of life. While extreme pH values were associated with declining protist diversity, high temperature springs harbored substantial amounts of protist diversity. Although protists are often overlooked in geothermal springs and other extreme environments, our results indicate that such environments can host distinct and diverse protistan communities.en_US
dc.language.isoenen_US
dc.rightsCC BY: This license lets you distribute, remix, tweak, and build upon this work, even commercially, as long as you credit the original creator for this work. This is the most accommodating of licenses offered. Recommended for maximum dissemination and useen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/legalcodeen_US
dc.titleAn on Orbit Determination of Point Spread Functions for the Interface Region Imaging Spectrograph.en_US
dc.typeArticleen_US
mus.citation.issue9en_US
mus.citation.journaltitleSolar Physicsen_US
mus.citation.volume293en_US
mus.identifier.categoryPhysics & Mathematicsen_US
mus.identifier.doi10.1007/s11207-018-1347-9en_US
mus.relation.collegeCollege of Letters & Scienceen_US
mus.relation.departmentPhysics.en_US
mus.relation.universityMontana State University - Bozemanen_US
mus.data.thumbpage23en_US


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CC BY: This license lets you distribute, remix, tweak, and build upon this work, even commercially, as long as you credit the original creator for this work. This is the most accommodating of licenses offered. Recommended for maximum dissemination and use
Except where otherwise noted, this item's license is described as CC BY: This license lets you distribute, remix, tweak, and build upon this work, even commercially, as long as you credit the original creator for this work. This is the most accommodating of licenses offered. Recommended for maximum dissemination and use