Mikko Kaasalainen

Mikko Kaasalainen

Mikko K.J. Kaasalainen is a Finnish applied mathematician and mathematical physicist. He is currently professor of mathematics at the department of mathematics at Tampere University of Technology. Kaasalainen has mostly worked on inverse problems and their applications especially in astrophysics, as well as on dynamical systems.

Contents

Education and career

Kaasalainen received an MSc in theoretical physics at the University of Helsinki in 1990, moving shortly afterwards to the University of Oxford, Merton College, where he completed his DPhil in theoretical physics in 1994, supervised by James Binney. After a series of post-doctoral and senior positions in Europe, he moved to the University of Helsinki and to his present institute in 2009. He leads a research group in the Finnish Centre of Excellence in Inverse Problems Research.

Kaasalainen was awarded the first Pertti Lindfors prize of the Finnish Inverse Problems Society in 2001. The asteroid 16007 Kaasalainen is named in his honour.

Research

Kaasalainen's research interests mostly focus on mathematical modelling in various fields ranging from remote sensing and space research to planetary and galactic dynamics. Typically, the models and mathematical methods Kaasalainen has developed with his colleagues are connected with inverse problems. Two such topics feature prominently in Kaasalainen's research:

  • Asteroid lightcurve inversion,[1] i.e., the reconstruction of the shapes and spin states of asteroids from their brightness measurements (lightcurves), based on mathematical results and uniqueness and stability theorems [2][3][4] that have been transformed into modelling algorithms with which a multitude of otherwise unresolvable asteroids can now be mapped.[5][6] This method has also been used in the direct verification of the Yarkovsky–O'Keefe–Radzievskii–Paddack effect in our solar system.[7][8][9][10][11][12][13][14][15][16]
  • Analysis of large dynamical systems, where torus construction methods [17][18] in phase space allow a compact representation or approximation of the dynamics of the observed system (such as a galaxy).

References

  1. ^ M. Kaasalainen et al. (2001): Optimization methods for asteroid lightcurve inversion. II. The complete inverse problem. Icarus 153, 37.
  2. ^ M. Kaasalainen et al. (1992): Interpretation of lightcurves of atmosphereless bodies. I. General theory and new inversion schemes. Astronomy and Astrophysics 259, 318.
  3. ^ M. Kaasalainen and L. Lamberg (2006): Inverse problems of generalized projection operators. Inverse Problems 22, 749.
  4. ^ L. Lamberg and M. Kaasalainen (2001): Numerical solution of the Minkowski problem. J. Comp. Appl. Math. 137, 213.
  5. ^ Asteroid model website
  6. ^ Minor Planet Observer website
  7. ^ M. Kaasalainen et al. (2007):Acceleration of the rotation of asteroid 1862 Apollo by radiation torques. Nature 446, 420.
  8. ^ W. F. Bottke (2007): Spun in the sun. Nature 446, 382.
  9. ^ D. P. Rubincam and S. J. Paddack (2007): As Tiny Worlds Turn. Science 316, 211.
  10. ^ New York Times 13 March 2007: Prediction Proved: Light Speeds an Asteroid as it Spins
  11. ^ BBC news 7 March 2007: Light puts asteroids into a spin
  12. ^ National Geographic 7 March 2007: Asteroids Spin Faster due to Solar Power, Studies Show
  13. ^ New Scientist 10 March 2007: Sun sends bumpy asteroids into a spin
  14. ^ Die Welt 8 March 2007: Sonnenstrahlen lassen Asteroiden schneller kullern
  15. ^ London Science Museum Web Exhibitions: Sun puts asteroids in a spin
  16. ^ Corriere della Sera 8 March 2007: Asteroidi piu pericolosi per la Terra con il motore solare naturale
  17. ^ M. Kaasalainen and J. Binney (1994): Construction of invariant tori and integrable Hamiltonians. Physical Review Letters 73, 2377.
  18. ^ M. Kaasalainen (1995): Construction of invariant tori in chaotic regions. Physical Review E 52, 1193.

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