2015年11月24日星期二

Share:Editorial: America’s science legacy


This video accompanies Science’s editorial, “America’s science legacy” by Neil deGrasse Tyson. In his editorial, Tyson celebrates the 150th Anniversary of Abraham Lincoln’s Gettysburg Address but also reflects on how Lincoln set a course for science to impact the future wellbeing of the nation. Tyson shares his 272-word speech “The Seedbed,” inspired by the 1863 Gettysburg Address. Published earlier this year, it is an impassioned reminder of the importance of science to America’s future.    

Full story source:http://bit.ly/1MzGQcd

2015年11月22日星期日

Comprehensive Approach to Research Writing and Publication

Authors:
Felix Kutsanedzie ,  Sylvester Achio ,  Edmund Ameko
ISBN:
978-1-940366-51-7
Published Date:
September, 2015
Publisher:
Description
The main objective of this book is to help students, would-be-research fellows and lecturers to get a good grasp of the technicalities involved in the act of research writing and publishing. It starts with a chapter that introduces the readers to the various constituents of research proposal writing by explaining the various technical terms and how to handle them in practice.

The book gives a comprehensive way of approaching the research reporting thus making it a must read book for all tertiary students preparing for the project report write ups, and detailed explanation on how to do reference both in-text and out-of-text for the APA format.

The later chapters of this book concentrated things to do to get ones findings from a research disseminated to the targeted clientele of the research.
If you like, read this book in SciencePG for free:http://bit.ly/1KCNcDv

2015年11月20日星期五

In electrifying advance, researchers create circuit within living plants

Swedish researchers have assembled electronics inside the stems and leaves of rose cuttings.
Swedish researchers have assembled electronics inside the stems and leaves of rose cuttings.
Talk about flower power. Researchers have crafted flexible electronic circuits inside a rose. Eventually such circuitry may help farmers eavesdrop on their crops and even control when they ripen. The advance may even allow people to harness energy from trees and shrubs not by cutting them down and using them for fuel, but by plugging directly into their photosynthesis machinery.
Flexible electronics are made from pliable organic materials. That makes them potentially compatible with tissues and has spurred research efforts to use them to diagnose and treat diseases. “Organic electronics is booming in the area of medical applications,” says Magnus Berggren, a materials scientist and electrical engineer at Linköping University, Norrköping, in Sweden and a leader in devising such medical applications.
About 15 years ago one of Berggren’s plant biology colleagues asked whether it would be possible to place electronics inside trees in order to eavesdrop on the biochemical processes going on there. If so, perhaps they could control, for example, precisely when a tree flowers. “We thought it was a joke,” Berggren says. After all, he notes, biologists have made steady strides in genetic engineering techniques to control myriad biochemical functions in plants. However, genetically engineered plants have a much harder time being approved for release in Sweden than they do in the United States. “We felt those technologies were never going to make it into the forests and fields here,” Berggren says. So a couple of years ago he and his colleagues decided to give electronic plants a second look.
Their idea was to use the plants’ own architecture and biology to help them assemble devices on the inside. To do so, they aimed to assemble polymer-based “wires” on the inside of a plant’s xylem, the tubelike channel that transports water up a plant’s stem to the leaves. They thought that if they could dissolve conducting polymer building blocks in water, perhaps plants could pull them up the channels and link them together into wires.
Berggren and his colleagues tried more than a dozen different polymer electronic building blocks. They dissolved them in water, then placed roses—either with intact roots or cut at the stem—in the water to see whether the organics would be wicked upward. All of the building blocks either clogged the base of the stem or didn’t assemble into wires.
Finally they tried an organic electronic building block called PEDOT-S:H. Each of these building blocks consists of a short, repeating chain of a conductive organic molecule with short arms coming off each link of the chain. Each of the arms sports a sulfur-containing group linked to a hydrogen atom. Berggren’s group found that when they placed them in the water, the rose stems readily pulled the short polymer chains up the xylem channels. The intact plants pulled the organics up through the roots as well, though much more slowly, Berggren says. Once inside, the chemistry in those channels pulled the hydrogen atoms off the short arms, a change that prompted the sulfur groups on neighboring chains to bind together. The upshot was that the myriad short polymer chains quickly linked themselves together into continuous strings as long as 10 centimeters. The researchers then added electronic probes to opposite ends of these strings, and found that they were, in fact, wires, conducting electricity all down the line.
Once that worked, Berggren’s team added other electronic patches on the surface of their rose stems to create transistors that were able to switch the current in a wire on and off. As they report today in Science Advances, they went on to use a set of different techniques to show they could get leaves to take up organic electronics, essentially creating an array of pixels. By applying different voltages to the pixels, they could change their colors to create a living display.
“It sounds really cool,” says Zhenan Bao, an organic electronics expert at Stanford University in Palo Alto, California. Though after a quick read of the paper, Bao says she’s not clear what the application would be.
Berggren says he, too, is just beginning to try to sort that out. One possibility, he says, is to embed electronic sensors in a few plants in a field to detect when they begin to release hormones that initiate the process of flowering or other changes in the plant. This could allow growers to better time watering and fertilizer applications to aid the plants. In time, he adds, it may even be possible to use plant electronics to speed or delay the onset of flowering to protect them from coming harsh weather. Finally, he says, perhaps in the distant future it may be possible to harness plants’ photosynthesis abilities to generate electricity directly, enabling us to reap the sun’s power without destroying the plants.  
Story source:http://bit.ly/219riU4

2015年11月18日星期三

Physical, Thermal, and Spectroscopic Characterization of Biofield Energy Treated Potato Micropropagation Medium

Authors: Mahendra Kumar Trivedi1, Alice Branton1, Dahryn Trivedi1, Gopal Nayak1, Khemraj Bairwa2, Snehasis Jana2, *

Abstract: Potato Micropropagation Medium (PMM) is the growth medium used for in vitro micropropagation of potato tubers. The present study was intended to assess the effect of biofield energy treatment on the physical, thermal and spectroscopic properties of PMM. The study was attained in two groups i.e. control and treated. The control group was remained as untreated, while the treated group was received Mr. Trivedi’s biofield energy treatment. Finally, both the samples (control and treated) were evaluated using various analytical techniques such as X-ray diffractometry (XRD), differential scanning calorimetry (DSC), thermogravimetric analysis- differential thermal analysis (TGA-DTA), UV-Vis spectrometry, and Fourier transform infrared (FT-IR) spectroscopy. The XRD analysis showed the crystalline nature of both control and treated samples of PMM. The X-ray diffractogram showed the significant increase in the intensity of XRD peaks in treated sample as compared to the control. The XRD analysis revealed 6.64% increase in the average crystallite size of treated PMM with respect to the control. The DSC analysis showed about 8.66% decrease in the latent heat of fusion in treated sample with respect to the control. The TGA-DTA analysis exhibited about 4.71% increase in onset temperature of thermal degradation after biofield treatment with respect to the control, while the maximum thermal degradation temperature (Tmax) was also increased (5.06%) in treated sample with respect to the control. This increase in Tmax might be correlated with increased thermal stability of treated sample as compared to the control. The UV spectroscopic study showed the slight blue shift in λmax of treated sample with respect to the control. FT-IR spectrum of control PMM showed the peak at 3132 cm-1 (C-H stretching) that was observed at higher wavenumber i.e. at 3161 cm-1 in the treated sample. Other vibrational peaks in the treated sample were observed in the similar region as that of the control. Altogether, the XRD, DSC, TGA-DTA, UV-Vis, and FT-IR analysis suggest that Mr. Trivedi’s biofield energy treatment has the impact on physicochemical properties of PMM. This treated PMM might be more effective as a micropropagation medium as compared to the control.
Keywords: Biofield Energy Treatment, Potato Micropropagation Medium, X-ray Diffraction, Differential Scanning Calorimetry (DSC), UV-vis Spectroscopy, Fourier Transform Infrared Spectroscopy

2015年11月6日星期五

Share:NASA mission reveals speed of solar wind stripping Martian atmosphere

Date:
November 5, 2015
Source:
NASA
Summary:
NASA's Mars Atmosphere and Volatile Evolution (MAVEN) mission has identified the process that appears to have played a key role in the transition of the Martian climate from an early, warm and wet environment that might have supported surface life to the cold, arid planet Mars is today.
Artist's rendering of a solar storm hitting Mars and stripping ions from the planet's upper atmosphere.
Credit: NASA/GSFC
NASA's Mars Atmosphere and Volatile Evolution (MAVEN) mission has identified the process that appears to have played a key role in the transition of the Martian climate from an early, warm and wet environment that might have supported surface life to the cold, arid planet Mars is today.
MAVEN data have enabled researchers to determine the rate at which the Martian atmosphere currently is losing gas to space via stripping by the solar wind. The findings reveal that the erosion of Mars' atmosphere increases significantly during solar storms. The scientific results from the mission appear in the Nov. 5 issues of the journals Science and Geophysical Research Letters.
"Mars appears to have had a thick atmosphere warm enough to support liquid water which is a key ingredient and medium for life as we currently know it," said John Grunsfeld, astronaut and associate administrator for the NASA Science Mission Directorate in Washington. "Understanding what happened to the Mars atmosphere will inform our knowledge of the dynamics and evolution of any planetary atmosphere. Learning what can cause changes to a planet's environment from one that could host microbes at the surface to one that doesn't is important to know, and is a key question that is being addressed in NASA's journey to Mars."
MAVEN measurements indicate that the solar wind strips away gas at a rate of about 100 grams (equivalent to roughly 1/4 pound) every second. "Like the theft of a few coins from a cash register every day, the loss becomes significant over time," said Bruce Jakosky, MAVEN principal investigator at the University of Colorado, Boulder. "We've seen that the atmospheric erosion increases significantly during solar storms, so we think the loss rate was much higher billions of years ago when the sun was young and more active."
In addition, a series of dramatic solar storms hit Mars' atmosphere in March 2015, and MAVEN found that the loss was accelerated. The combination of greater loss rates and increased solar storms in the past suggests that loss of atmosphere to space was likely a major process in changing the Martian climate.
The solar wind is a stream of particles, mainly protons and electrons, flowing from the sun's atmosphere at a speed of about one million miles per hour. The magnetic field carried by the solar wind as it flows past Mars can generate an electric field, much as a turbine on Earth can be used to generate electricity. This electric field accelerates electrically charged gas atoms, called ions, in Mars' upper atmosphere and shoots them into space.
MAVEN has been examining how solar wind and ultraviolet light strip gas from of the top of the planet's atmosphere. New results indicate that the loss is experienced in three different regions of the Red Planet: down the "tail," where the solar wind flows behind Mars, above the Martian poles in a "polar plume," and from an extended cloud of gas surrounding Mars. The science team determined that almost 75 percent of the escaping ions come from the tail region, and nearly 25 percent are from the plume region, with just a minor contribution from the extended cloud.
Ancient regions on Mars bear signs of abundant water -- such as features resembling valleys carved by rivers and mineral deposits that only form in the presence of liquid water. These features have led scientists to think that billions of years ago, the atmosphere of Mars was much denser and warm enough to form rivers, lakes and perhaps even oceans of liquid water.
Recently, researchers using NASA's Mars Reconnaissance Orbiter observed the seasonal appearance of hydrated salts indicating briny liquid water on Mars. However, the current Martian atmosphere is far too cold and thin to support long-lived or extensive amounts of liquid water on the planet's surface.
"Solar-wind erosion is an important mechanism for atmospheric loss, and was important enough to account for significant change in the Martian climate," said Joe Grebowsky, MAVEN project scientist from NASA's Goddard Space Flight Center in Greenbelt, Maryland. "MAVEN also is studying other loss processes -- such as loss due to impact of ions or escape of hydrogen atoms -- and these will only increase the importance of atmospheric escape."
The goal of NASA's MAVEN mission, launched to Mars in November 2013, is to determine how much of the planet's atmosphere and water have been lost to space. It is the first such mission devoted to understanding how the sun might have influenced atmospheric changes on the Red Planet. MAVEN has been operating at Mars for just over a year and will complete its primary science mission on Nov. 16.
To view an animation simulating the loss of atmosphere and water on Mars:
For more information and images on Mars' lost atmosphere, visit:
For more information about NASA's MAVEN mission, visit:

Story Source:
The above post is reprinted from materials provided by NASANote: Materials may be edited for content and length.

Journal References:
  1. B. M. Jakosky. MAVEN Explores the Martian Upper Atmosphere.Science, 2015; 350 (6261): 643 DOI: 10.1126/science.aad3443
  2. Bruce M. Jakosky, Joseph M. Grebowsky, Janet G. Luhmann, David A. Brain. Initial results from the MAVEN mission to MarsGeophysical Research Letters, 2015; DOI: 10.1002/2015GL065271
Full story source: http://bit.ly/1GOrguj