Emma Bunce

Emma J. Bunce (born 1975) is an astrophysicist and Professor of Planetary Plasma Physics at the University of Leicester.^[1] She holds a Royal Society Wolfson Research Merit Award. She studies the magnetospheres of Saturn and Jupiter. She is principal investigator (PI) on the European Space Agency BepiColombo mission, was deputy lead on the Jupiter Icy Moons Explorer proposal, and co-investigator on the Cassini–Huygens mission.

Early life and education

Bunce grew up in Worthing.^[2] In 1989 she watched the Horizon BBC documentary on Neptune with images taken by Voyager 1 and was inspired to become a space scientist.^[3] She was educated at Worthing College, which she graduated in 1994.^[2] She studied physics with space science at the University of Leicester and earned her Master of Physics (MPhys) degree in 1998.^[2] In 1998 Bunce began her doctoral training with Stan Cowley, investigating the magnetosphere of Jupiter.^[2] Her thesis, Large-scale current systems in the Jovian Magnetosphere, looked at the radial current systems of the middle magnetosphere of Jupiter.^[4] She used data from Pioneer 10, Pioneer 11, Voyager 1, Voyager 2 and Ulysses.^[5] The interaction between Jupiter and the surrounding plasma environment is influenced by the magnetic field. On Jupiter, the plasma is mainly produced in the volcanic moon Io.^[5]

Research and career

After her graduate studies, Bunce worked as a postdoctoral researcher investigating the Kronian magnetosphere of Saturn in preparation for Cassini–Huygens.^[5] In 2003 Bunce was awarded a Particle Physics and Astronomy Research Council fellowship to study the magnetosphere of Saturn.^[2] She continued to study Jupiter’s polar auroral emissions.^[6][7] In 2005 she was awarded funding from the Royal Astronomical Society to attend the Magnetoshpere of the Outer Planets conference.^[8] She was appointed to the faculty at the University of Leicester in 2005.^[2]

Bunce was part of the Cassini–Huygens magnetometer team.^[9] She was the first to analyse the UV aurorae of Saturn using the Hubble Space Telescope.^[10][11] The magnetosphere of Saturn rotates rapidly and plasma is produced via sputter of the icy moons.^[2] She monitored the magnetospheric currents of Saturn in situ, identifying that there was a connection between the auroral oval and upward-directed field-aligned currents that flow near open and closed field lines.^[11] She observed the interaction of the solar wind with the magnetosphere of Saturn.^[12] In 2009 she was elected to the Royal Astronomical Society Council.^[13] That year she delivered the Royal Astronomical Society Harold Jeffreys Lecture.^[12] She discussed her work Jupiter-like aurorae found on saturn.^[14]

She was promoted to reader in 2009 and professor in 2013.^[2] She organised a celebration of ten years of Cassini–Huygens in 2014.^[15] She is the Principal Investigator of the Mercury Imaging X-ray Spectrometer (MIXS) instrument.^{[16][17][18][19]} MIXS was built in Leicester, launched in 2015 and will travel to mercury.^[20][21] She delivered the 2016 National Space Academy keynote lecture.^[22] She is the principal investigator on the European Space Agency BepiColombo mission (to Mercury) and deputy lead on the Jupiter Icy Moons Explorer.^[23] BepiColombo will help to explain some of the mysteries of Mercury, including finding volatile sulphur and potassium.^[24][25] She contributed to the book Mathematical Methods for the Physical Sciences: A University Level Introduction in 2018.^[26]

References