Sandra Chapman

British astrophysicist From Wikipedia, the free encyclopedia

Sandra C. Chapman CPhysis FInstP FRAS a British astrophysicist who is Professor of Physics and Director of the Centre for Fusion, Space and Astrophysics at the University of Warwick. Her research considers nonlinear physics and planetary magnetospheres.

Early life and education

Chapman studied physics at Imperial College London, where she was awarded an Exhibition Scholarship.[1] She was diagnosed with temporal lobe epilepsy during her undergraduate degree.[2] She remained at Imperial for her doctoral research, which considered the release of lithium in the near Earth plasma environment.[3]

Research and career

Chapman joined the University of Warwick in 1995. In 2000 she became the first woman to become a professor of physics at the University of Warwick.[4]

Chapman studies the dynamical interactions of planetary magnetospheres. She has shown that they release energy in unpredictable intervals, and behave as multi-scale, coupled systems. Her research on magnetic storms informed the strategy of the Magnetospheric Multiscale Mission.[5] Alongside her scientific research, Chapman is an artist, and in 2003 held a NESTA fellowship[6] to create art with the British Antarctic Survey.[7][8][9]

To perform her investigations, Chapman makes use of non-linear physics.[10] She has applied her understanding to the aurora,[11] to quantify the risk of extreme space weather[12][13] and to better understand solar activity.[14] In 2017, she was awarded a Fulbright Program Fellowship to spend a year at Boston University and identify ways to protect the planet from space weather.[15]

Chapman was a 2003-2004 Harvard Radcliffe Institute Fellow[16] and the International Space Science Institute 2023 Johannes Geiss Fellow.[17]

In 2022, Chapman was awarded the Royal Astronomical Society Chapman Medal.[18]

Awards and honours

Selected publications

  • H. Karimabadi; V. Roytershteyn; M. Wan; et al. (January 2013). "Coherent structures, intermittent turbulence, and dissipation in high-temperature plasmas". Physics of Plasmas. 20 (1): 012303. doi:10.1063/1.4773205. ISSN 1070-664X. Wikidata Q60707157.
  • K H Kiyani; S C Chapman; Yu V Khotyaintsev; M W Dunlop; F Sahraoui (14 August 2009). "Global scale-invariant dissipation in collisionless plasma turbulence". Physical Review Letters. 103 (7): 075006. arXiv:0906.2830. doi:10.1103/PHYSREVLETT.103.075006. ISSN 0031-9007. PMID 19792654. Wikidata Q60707278.{{cite journal}}: CS1 maint: article number as page number (link)
  • X. Litaudon; S. Abduallev; M. Abhangi; et al. (15 June 2017). "Overview of the JET results in support to ITER". Nuclear Fusion. 57 (10): 102001. doi:10.1088/1741-4326/AA5E28. ISSN 0029-5515. Wikidata Q57645458.

References

Related Articles

Wikiwand AI