5,616 research outputs found
The moon impact probe on Chandrayaan-1
A unique, stand alone micro satellite called the Moon impact pobe (MIP), designed to impact at a predecided location near the South Pole of the moon was a part of the Chandrayaan-1 mission. The MIP has two technology and one scientific experiments, viz. a Moon Imaging System (MIS) for surface photography along its path, a Radar Altimeter for terrain topography at close distance (<5 km) and a Mass Spectrometer, CHACE (Chandra's Altitudinal Composition Explorer), for measuring the neutral composition on the sunlit side of the moon. A description of the various sub-systems of the MIP and of the instruments is presented in this article
The moon impact probe on Chandrayaan-1
A unique, stand alone micro satellite called the Moon impact pobe (MIP), designed to impact at a predecided location near the South Pole of the moon was a part of the Chandrayaan-1 mission. The MIP has two technology and one scientific experiments, viz. a Moon Imaging System (MIS) for surface photography along its path, a Radar Altimeter for terrain topography at close distance (<5 km) and a Mass Spectrometer, CHACE (Chandra's Altitudinal Composition Explorer), for measuring the neutral composition on the sunlit side of the moon. A description of the various sub-systems of the MIP and of the instruments is presented in this article
Investigation of Cs surface layer formation in Cs-SIMS with TOF-MEIS and SIMS
In this report, cesiumsurface layers formed by Cs+ ion bombardment on silicon and phenylalanine (Phe) sampleswere analyzed by TOF-MEIS and ToF-SIMS. Si wafers were bombarded with 500 eV Cs+ ions, then were subsequently bombarded with five different Cs+ fluences corresponding to the transient and equilibrium regimes. The Phe layers were evaporated on Si wafers, up to 100 nm thickness. The samples were subsequently bombarded at four different fluences. For Phe, TOF-MEIS shows the formation of a sharp Cs surface layer of ∼0.5 nm thickness, on which the peak height increases with Cs+ ion bombardment and a long Cs tail builds up, penetrating deep into the subsurface. For Si, a similar Cs surface peak forms, but it saturates quickly compared to Phe.</p
PiLa-CS Professional Learning Community - Workshop 2 Resources
During the Summer of 2021 and 2022, the Participating in Literacies and Computer Science (PiLa-CS) Research Practice Partnership convened and supported a community of practice to learn more about how to enable better CS teaching for emergent bilinguals. These are materials from Workshop 2 of the PLC.Sponsored by the National Science Foundation under NSF grant CNS-1738645 and DRL-1837446. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation
Africa Is Much Bigger Than You Think It Is
Historically, Africa has tended to be misrepresented in maps. In the commonly used Mercator method of mapping a sphere (the Earth) onto a at plane (a map), countries further away from the equator are distorted and enlarged. Consequently, Africa is diminished and presented as smaller than it actually is. This work seeks to correct this misrepresentation by showing the continent in relation to something we associate as being large - the Moon. Both images are to the same scale and sized correctly relative to each other
Translanguaging Pedagogy in CS Ed
Episode 3: Translanguaging pedagogy in CS Education
This video looks at how multilingual students already use translanguaging in their computer science classes and discusses how CS educators can further support them with translanguaging pedagogy, a framework that prompts teachers to consider their stance, design, and shifts.
Featuring team members from Participating in Literacies and Computer Science (PiLa-CS), https://www.pila-cs.orgEpisode 3: Translanguaging pedagogy in CS Education
This video looks at how multilingual students already use translanguaging in their computer science classes and discusses how CS educators can further support them with translanguaging pedagogy, a framework that prompts teachers to consider their stance, design, and shifts.
Featuring team members from Participating in Literacies and Computer Science (PiLa-CS), https://www.pila-cs.orgSponsored by the National Science Foundation under NSF grant CNS-1738645 and DRL-1837446. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation
Alkali element constraints on Earth-Moon relations
Given their range of volatilities, alkali elements are potential tracers of temperature-dependent processes during planetary accretion and formation of the Earth-Moon system. Under the giant impact hypothesis, no direct connection between the composition of the Moon and the Earth is required, and proto-lunar material does not necessarily experience high temperatures. Models calling for multiple collisions with smaller planetesimals derive proto-lunar materials mainly from the Earth's mantle and explicitly invoke vaporization, shock melting and volatility-related fractionation. Na/K, K/Rb, and Rb/Cs should all increase in response to thermal volatization, so theories which derive the Moon substantially from Earth's mantle predict these ratios will be higher in the Moon than in the primitive mantle of the Earth. Despite the overall depletion of volatile elements in the Moon, its Na/K and K/Rb are equal to or less than those of Earth. A new model presented here for the composition of Earth's continental crust, a major repository of the alkali elements, suggests the Rb/Cs of the Moon is also less than that of Earth. Fractionation of the alkali elements between Earth and Moon are in the opposite sense to predictions based on the relative volatilities of these elements, if the Moon formed by high-T processing of Earth's mantle. Earth, rather than the Moon, appears to carry a signature of volatility-related fractionation in the alkali elements. This may reflect an early episode of intense heating on Earth with the Moon's alkali budget accreting from cooler material
PiLa-CS Professional Learning Community - Design Journal Template
During the Summer of 2021 and 2022, the Participating in Literacies and Computer Science (PiLa-CS) Research Practice Partnership convened and supported a community of practice to learn more about how to enable better CS teaching for emergent bilinguals. These are materials from from the PLC for a Design Journal to act as a planing template for teachers.Sponsored by the National Science Foundation under NSF grant CNS-1738645 and DRL-1837446. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation
Arizona Then and Now: Exploring Arizona's Five Cs Through Photography
abstract: Arizona Then and Now: Exploring Arizona's Five Cs Through Photography is a photographic exploration of the evolution of Arizona's five Cs: cotton, copper, citrus, cattle, and climate. This project first looks to the past to see how these five elements shaped the state of Arizona. Photographs were taken across the valley of these elements, or lack thereof, discovering what Arizona has transformed into in the process. Each chapter of the book begins with a brief history of the element focused on in that chapter, followed by an analytical thought about the photographs taken and how the element has evolved. Each chapter shows two historical photographs followed by a series of photographs taken during the project that the author thought depicted what is seen today. The book ends on a final positive note about how the five Cs are not dead, but soon could be completely taken over. This project was a way for a non-art major to explore the state that she grew up while also challenging herself by more than just taking pictures. The photographs displayed in the book depict a sampling of what the author saw that is left of the five Cs
IR-improved DGLAP-CS QCD parton showers in Pythia8
AbstractWe introduce the recently developed IR-improved DGLAP-CS theory into the showers in Pythia8, as this Monte Carlo event generator is in wide use at LHC. We show that, just as it was true in the IR-improved shower Monte Carlo Herwiri, which realizes the IR-improved DGLAP-CS theory in the Herwig6.5 environment, the soft limit in processes such as single heavy gauge boson production is now more physical in the IR-improved DGLAP-CS theory version of Pythia8. This opens the way to one’s getting a comparison between the actual detector simulations for some of the LHC experiments between IR-improved and unimproved showers as Pythia8 is used in detector simulations at LHC whereas Herwig6.5, the environment of the only other IR-improved DGLAP-CS QCD MC in the literature, Herwiri1.031, is not any longer so used. Our achieving the availability of the IR-improved DGLAP-CS Pythia8 then is an important step in the further development of the LHC precision theory program under development by the author and his collaborators
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