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Friday, January 19th, 2018

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    12:00a
    Programmable droplets

    MIT researchers have developed hardware that uses electric fields to move droplets of chemical or biological solutions around a surface, mixing them in ways that could be used to test thousands of reactions in parallel.

    The researchers view their system as an alternative to the microfluidic devices now commonly used in biological research, in which biological solutions are pumped through microscopic channels connected by mechanical valves. The new approach, which moves solutions around in computationally prescribed patterns, could enable experiments to be conducted more efficiently, cost-effectively, and at larger scales.

    “Traditional microfluidic systems use tubes, valves, and pumps,” says Udayan Umapathi, a researcher at the MIT Media Lab, who led the development of the new system. “What this means is that they are mechanical, and they break down all the time. I noticed this problem three years ago, when I was at a synthetic biology company where I built some of these microfluidic systems and mechanical machines that interact with them. I had to babysit these machines to make sure they didn’t explode.”

    “Biology is moving toward more and more complex processes, and we need technologies to manipulate smaller- and smaller-volume droplets,” Umapathi says. “Pumps, valves, and tubes quickly become complicated. In the machine that I built, it took me a week to assemble 100 connections. Let’s say you go from a scale of 100 connections to a machine with a million connections. You’re not going to be able to manually assemble that.”

    With his new system, Umapathi explains, thousands of droplets could be deposited on the surface of his device, and they would automatically move around to carry out biological experiments.

    The system includes software that allows users to describe, at a high level of generality, the experiments they wish to conduct. The software then automatically calculates droplets’ paths across the surface and coordinates the timing of successive operations.

    “The operator specifies the requirements for the experiment — for example, reagent A and reagent B need to be mixed in these volumes and incubated for this amount of time, and then mixed with reagent C. The operator doesn’t specify how the droplets flow or where they mix. It is all precomputed by the software.”

    Umapathi and his coauthors — Hiroshi Ishii, the Jerome B. Wiesner Professor of Media Arts and Sciences at MIT; Patrick Shin and Dimitris Koutentakis, MIT undergraduates working in Ishii’s lab; and Sam Gen Chin, a Wellesley undergrad in the lab — describe their new system in a paper appearing this month in the online journal MRS Advances.

    In the past 10 years, other research groups have experimented with “digital microfluidics,” or electrical manipulation of droplets, to conduct biological experiments. But their chips were manufactured using high-end etching techniques that require controlled environments known as clean rooms. Umapathi and his colleagues have focused on getting costs down. Their prototype uses a printed circuit board, a commodity electronic device that consists of a plastic board with copper wiring deposited on top of it.

    The researchers’ chief technical challenge was to design a coating for the surface of the circuit board that would reduce friction, enabling droplets to slide across it, and that would prevent biological or chemical molecules from sticking to it, so that they won’t contaminate future experiments. The circuit board is patterned with an array of electrodes. In the prototype, the researchers coat the board with a much denser array of tiny spheres, only a micrometer high, made from a hydrophobic (water-repellent) material. Droplets skate across the tops of the spheres. The researchers are also experimenting with structures other than spheres, which may work better with particular biological materials.

    Because the device’s surface is hydrophobic, droplets deposited atop it naturally try to assume a spherical shape. Charging an electrode pulls the droplet downward, flattening it out. If the electrode below a flattened droplet is gradually turned off, while the electrode next to it is gradually turned on, the hydrophobic material will drive the droplet toward the charged electrode.

    Moving droplets requires high voltages, somewhere between 95 and 200 volts. But 300 times a second, a charged electrode in the MIT researchers’ device alternates between a high-voltage, low-frequency (1-kilohertz) signal and a 3.3-volt high-frequency (200-kilohertz) signal. The high-frequency signal enables the system to determine a droplet’s location, using essentially the same technology that touch-screen phones do.

    If the droplet isn’t moving rapidly enough, the system will automatically boost the voltage of the low-frequency signal. From the sensor signal, the system can also estimate a droplet’s volume, which, together with location information, allows it to track a reaction’s progress.

    Umapathi believes that digital microfluidics could drastically cut the cost of experimental procedures common in industrial biology. Pharmaceutical companies, for instance, will frequently conduct many experiments in parallel, using robots equipped with dozens or even hundreds of pipettes, little measuring tubes that are rather like elongated eye droppers.

    “If you look at drug discovery companies, one pipetting robot uses a million pipette tips in one week,” Umapathi says. “That is part of what is driving the cost of creating new drugs. I’m starting to develop some liquid assays that could reduce the number of pipetting operations 100-fold.”

    “In the last 15, 20 years, the general trend in pharma has been to move toward smaller volumes, because they have greater multiplexing capability,” says Charles Fracchia, founder and CEO of BioBright, a company that develops information systems to manage the wealth of data generated by modern, high-volume biological experiments. “When it comes to digital microfluidics the way Udayan does it, it’s effectively a cheaper version, and it’s one-sided instead of being sandwiched between two electrodes. I don’t want to call it DIY bio, but it’s lower-cost, simpler instrumentation, easier access. He definitely hit that note a lot better than [earlier systems] did. It’s exciting that he’s managed to do it with lower voltage, and it’s exciting that he can do it with a single electrode.”

    6:00a
    Solar eclipse caused bow waves in Earth's atmosphere

    The celebrated Great American Eclipse of August 2017 crossed the continental U.S. in 90 minutes, and totality lasted no longer than a few minutes at any one location. The event is well in the rear-view mirror now, but scientific investigation into the effects of the moon's shadow on the Earth's atmosphere is still being hotly pursued, and interesting new findings are surfacing at a rapid pace. These include significant observations by scientists at MIT’s Haystack Observatory in Westford, Massachusetts.

    Eclipses are not particularly rare, but it is unusual for one to cross the entire continental U.S. as happened in August. By studying an eclipse’s effects on the electron content of the upper atmosphere, scientists are learning more about how our planet's complex and interlocked atmosphere responds to space weather events, such as solar flares and coronal mass ejections, that can have severe effects on signal information and communication paths, and can impact navigation and positioning services.

    The ionosphere is the layer of the atmosphere containing charged particles created primarily by solar radiation. It allows long-distance radio wave propagation and communication over the horizon and affects essential satellite-based transmissions in navigation systems and on-board aircraft. Since the ionosphere is the medium in which radio waves travel and is affected by solar variations, understanding its features is important for our modern technological society. The ionosphere is host to a huge number of naturally occurring waves, from small to large in size and strength, and eclipse shadows in particular can leave behind a large number of newly created waves as they travel across the planet.

    One kind of these new waves, known as ionospheric bow waves, has been predicted for more than 40 years to exist in the wake of an eclipse passage. Researchers at MIT's Haystack Observatory and the University of Tromsø in Norway confirmed the existence of ionospheric bow waves definitively for the first time during the August 2017 event. An international team led by Haystack Observatory scientists studied ionospheric electron content data collected by a network of more than 2,000 GNSS (Global Navigation Satellite System) receivers across the nation. Based on this work, Haystack’s Shunrong Zhang and colleagues published an article in December in the journal Geophysical Research Letters on the results showing the newly detected ionospheric bow waves.

    Geospace research scientists at Haystack Observatory were able to observe the eclipse bow wave phenomenon for the first time in the atmosphere with unprecedented detail and accuracy, thanks to the vast network of extremely sensitive GNSS receivers now in place across the U.S. The observed ionospheric bow waves are much like those formed by a ship; the moon's shadow travels so quickly that it causes a sudden temperature change as the atmosphere is rapidly cooled and then reheated as the eclipse passes. 

    “The eclipse shadow has a supersonic motion which [generates] atmospheric bow waves, similar to a fast-moving river boat, with waves starting in the lower atmosphere and propagating into the ionosphere,” the description by Zhang and his colleagues states. “Eclipse passage generated clear ionospheric bow waves in electron content disturbances emanating from totality primarily over central/eastern United States. Study of wave characteristics reveals complex interconnections between the sun, moon, and Earth's neutral atmosphere and ionosphere.”

    GNSS receivers collect very accurate, high-resolution data on the total electron content (TEC) of the ionosphere. The rich detail provided by this data informed a separate study on eclipse effects in the same issue of Geophysical Research Letters by the Haystack research team and international colleagues. Haystack Observatory Associate Director and lead author Anthea Coster and her co-authors describe the continental size and timing of eclipse-triggered TEC depletions observed over the U.S. and observed increased TEC over the Rocky Mountains that is likely related to the generation of mountain waves in the lower atmosphere during the eclipse. The reason for this effect — which was not predicted or anticipated before the eclipse — is being investigated by the geospace science community.

    “Since the first days of radio communications more than 100 years ago, eclipses have been known to have large and sometimes unanticipated effects on the ionized part of Earth’s atmosphere and the signals that pass through it,” says Phil Erickson, assistant director at Haystack and lead for the atmospheric and geospace sciences group. “These new results from Haystack-led studies are an excellent example of how much still remains to be learned about our atmosphere and its complex interactions through observing one of nature’s most spectacular sights — a giant active celestial experiment provided by the sun and moon. The power of modern observing methods, including radio remote sensors distributed widely across the United States, was key to revealing these new and fascinating features.”

    The Haystack eclipse studies, including the bow wave observations, drew the attention of national science media outlets, including National Geographic, Newsweek, Gizmodo, and many others. One of Zhang’s readers, an eighth grader from Minnesota, asked some interesting questions:

    Q: Was there any prior evidence to show that the waves would be arriving during the eclipse?

    A: There were prior studies on the waves based on very limited spatial coverage of the observations. The Great American Eclipse provided unprecedented spatial coverage to view unambiguously the complete wave structures.

    Q: Did these waves emit any seismic activity? Did they have a frequency that they could be detected on?

    A: No, they didn’t. In fact we believe these waves were originated from the middle atmosphere [about 50 kilometers] but we observed them in the upper atmosphere at approximately 300 kilometers. They were very weak-pressure fluctuations if we observe the waves from the ground. This kind of wave was produced by eclipse-related cooling processes; there might be other ways to induce similar waves in the upper atmosphere.

    Q: On the path of totality, were the waves stronger? Did they have any different effect anywhere else?

    A: Yes, we found that they existed mostly along and within a few hundreds of kilometers from the totality central path. They were first seen in central U.S., then vanished in the central-eastern U.S. They were able to travel for about one hour at a speed of approximately 300 meters per second, slower than the moon shadow’s speed.

    Haystack scientists will continue to analyze atmospheric data from the eclipse and expect to report other findings shortly. The next major eclipse across North America will occur in April 2024.

    GPS TEC data products and access through the Madrigal distributed data system are provided to the community by MIT with support from U.S. National Science Foundation grant AGS-1242204 and NASA grant NNX17AH71G for eclipse scientific support.

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