Jump to content

Mei-Ching Fok

From Wikipedia, the free encyclopedia
Mei-Ching Fok
Alma materChinese University of Hong Kong
Eastern Michigan University
University of Michigan
Scientific career
InstitutionsGoddard Space Flight Center
Universities Space Research Association
Marshall Space Flight Center

Mei-Ching Hannah Fok is a planetary scientist at the Goddard Space Flight Center. She was awarded the NASA Exceptional Scientific Achievement Medal in 2011 and elected a Fellow of the American Geophysical Union in 2019. She has worked on the IMAGE, Van Allen Probes and TWINS missions.

Early life and education

Fok studied physics at the Chinese University of Hong Kong.[1] She was awarded her bachelor's degree in 1980, and remained there to study for a diploma in Education.[1] She earned her diploma in 1984, then moved to Eastern Michigan University for her graduate studies. In 1987, Fok graduated from Eastern Michigan University with a master's degree in physics. She joined University of Michigan, Ann Arbor for her doctorate, which she completed in 1993.[1]

Research and career

In 1993, Fok joined the Marshall Space Flight Center as a Research Associate. She moved to the Universities Space Research Association in 1995, where she spent six years as a staff scientist. In 2001, she joined the Goddard Space Flight Center. She studies the Van Allen radiation belts during geomagnetic storms and active times. She has studied the ring current and their role in magnetosphereionosphere coupling.[2]

Example of her Neutral Atom Imaging work

Fok developed the Comprehensive Inner Magnetosphere–Ionosphere model (CIMI), a bounce-averaged kinetic model that can calculate the plasma fluxes within the ring current regions of the radiation belt.[3][4] Fok's CIMI model is currently being used to predict the fluxes observed by the Van Allen Probes.[5] CIMI takes in information about magnetic fields, electric potentials, quiet-time conductances and solar wind speed, and outputs information about ion fluxes, plasmasphere density and ionospheric potentials.[3] Using the model, Fok found that the main phase pressure of the magnetosphere was not created by the solar wind, but instead dominated by energetic protons from the plasmasphere.[6][7] Fok was awarded the NASA Exceptional Scientific Achievement Medal for her development of CIMI. Her citation read: "For creation of state-of-the-art numerical models that account for the complex couplings between the solar wind, radiation belts, ring current, ionosphere and magnetosphere".[8]

Alongside creating the CIMI model, Fok works on Neutral Atom Imaging, and her modelling tools were used in both the IMAGE and TWINS missions.[1]

Awards and honours

Her awards and honours include;

Selected publications

Her publications include;

  • Fok, Mei-Ching (2001). "Comprehensive computational model of Earth's ring current". Journal of Geophysical Research: Space Physics. 106 (A5): 8417–8424. Bibcode:2001JGR...106.8417F. doi:10.1029/2000JA000235.
  • Fok, Mei-Ching (1996). "Ring current development during storm main phase". Journal of Geophysical Research: Space Physics. 101 (A7): 15311–15322. Bibcode:1996JGR...10115311F. doi:10.1029/96JA01274. hdl:2060/19970022202. S2CID 122248082.
  • Fok, Mei-Ching (1995). "Three‐Dimensional Ring Current Decay Model". Journal of Geophysical Research: Space Physics. 100 (A6): 9619. Bibcode:1995JGR...100.9619F. doi:10.1029/94JA03029. hdl:2060/19960014063. S2CID 53004273.

References

  1. ^ a b c d "Bio – Mei-Ching H Fok". science.gsfc.nasa.gov. Retrieved 2019-08-25.
  2. ^ Mei-ching Fok – Role of Ring Current in M–I Coupling, retrieved 2019-08-25
  3. ^ a b Buzulukova, Natalia (2017-12-01). Extreme Events in Geospace: Origins, Predictability, and Consequences. Elsevier. ISBN 9780128127018.
  4. ^ Fok, M.-C.; Buzulukova, N. Y.; Chen, S.-H.; Glocer, A.; Nagai, T.; Valek, P.; Perez, J. D. (2014). "The Comprehensive Inner Magnetosphere–Ionosphere Model". Journal of Geophysical Research: Space Physics. 119 (9): 7522–7540. Bibcode:2014JGRA..119.7522F. doi:10.1002/2014JA020239. ISSN 2169-9402.
  5. ^ Buzulukova, Natalia (2017-12-01). Extreme Events in Geospace: Origins, Predictability, and Consequences. Elsevier. ISBN 9780128127018.
  6. ^ "How Plasma From Superstorms Affects Near-Earth Space". ScienceDaily. Retrieved 2019-08-25.
  7. ^ "Model Reveals How Plasma from Superstorms Affects Near-Earth Space". phys.org. Retrieved 2019-08-25.
  8. ^ a b "Awards Won – Geospace Physics Laboratory – 673". science.gsfc.nasa.gov. Retrieved 2019-08-25.
  9. ^ "2019 Class of AGU Fellows Announced". Eos. 15 August 2019. Retrieved 2019-08-25.