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Born on this day in 1929 in Ukraine, Charlotte Froese Fischer is an applied mathematician and computer scientist known for developing the multiconfigurational Hartree–Fock (MCHF) method for atoms. Shortly after she was born, her family fled Ukraine and spent several months in a German refugee camp before immigrating to Canada. There Froese Fischer excelled at school and was awarded a scholarship to attend the University of British Columbia. After earning her BA in mathematics... and chemistry in 1952 and her MA in applied mathematics in 1954, she spent two years at Cambridge University, studying applied mathematics and computing under English mathematician Douglas Hartree. Upon completion of her PhD in 1957, Froese Fischer was offered a position as lecturer at the University of British Columbia, which had just acquired its first computer. Over the next decade, she added computer courses to the university’s curriculum and then helped form the computer science department. Her research focused on numerical methods, particularly for atomic structure calculations. In 1963 Froese Fischer became the first woman scientist awarded an Alfred P. Sloan Foundation research fellowship, which provides funding for promising early-career scientists. In 1991 she was made a fellow of the American Physical Society. Froese Fischer has been an emerita research professor of computer science at Vanderbilt since 1996. (Photo credit: Michel R. Godefroid, Brussels, Belgium)

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In the six years since CERN announced that the Large Hadron Collider had revealed the existence of the Higgs boson, the LHC has uncovered no other previously undiscovered particles. This lack of discovery has narrowed the possible supplements and alternatives to the Standard Model of particle physics. But it has stirred discussion about the naturalness principle, which is the idea that if a theory requires too much "fine tuning", then the theory isn't "natural" and should be discounted.

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It is hard to overstate the anticipation that preceded the opening of the Large Hadron Collider (LHC) 10 years ago. Smashing protons…
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Operation Mousetrap
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Here's a dazzling display captured on 20 July by the Cassini probe orbiting Saturn. You can see an aurora moving from left to right and then curving back around as the planet rotates. (The five-second video contains 70 minutes of footage.) The bright dots are background stars, which shift in position as Cassini stares at one spot on the planet. Credit: NASA/JPL-Caltech/Space Science Institute
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Later on today NASA will be holding another Pluto press conference to announce the next batch of high resolution photos from the New Horizon spacecraft. In the meantime, we have a minor exclusive. One of the most difficult tasks the researchers had was to plot out what areas of Pluto and Charon to investigate during the rapid flyby and model the behavior of the spacecraft and its instruments during this time. They narrowed down the target areas by creating a computer model of the encounter which allowed them to change the parameters. The team then tweaked the parameters to reflect the competing demands of the different research groups. On Tuesday, Hong Kyu Kang, one of the projects engineers, showed me some of the simulations they were carrying out in the weeks leading up to the flyby. We have permission to show you a short extract of the final flight path simulation below. Here's Kang's description of the video: "This is a short part of the LORRI instrument observation as we fly past Pluto. The green squares are LORRI field of view (the are to be imaged) and purple is the LEISA boresight of the RALPH instrument. The turquoise slit is one of the PAN slits for RALPH as is the light red slit. For these observation, RALPH is the main instrument controlling the pointing of the spacecraft and LORRI is considered a "piggy back" ride along observation. The grey cylindrical shapes are the error ellipses that we had when we created these observations." Movie credit: Hong Kyu Kang, New Horizons, APL.
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