61. |
Fukushima, T., Astron. J., 133, 1-10, 2007,
New Two-Body Regularization
|
60. |
Shirai, T., Fukushima, T., and Malkin, Z.,
Earth, Planets, Space, 57, 151-155, 2005,
Detection of Phase Disturbances of Free Core Nutation of the
Earth and their Concurrence with Geomagnetic Jerks
|
59. |
Fukushima, T., Astron. J., 129, Vol.5, 2005,
Efficient Orbit Integration by Linear Transformation for
Kustaanheimo-Stiefel Regularization
|
58. |
Fukushima, T., Astron. J., 129, 1746-1754, 2005,
Efficient Orbit Integration by Kustaanheimo-Stiefel
Regularization using Time Element
|
57. |
Fukushima, T., Astron. J., 129, 1171-1177, 2005,
Efficient Orbit Integration by Orbital Longitude Methods with
Sundmann Transformation on Time Variable
|
56. |
Fukushima, T., Astron. J., 129, 554, 2005,
Erratum: "Efficient Integration of Highly Eccentric Orbits by
Quadruple Scaling Method for Kustaanheimo-Stiefel Regularization"
|
55. |
Fukushima, T., Astron. J., 128, 3108-3113, 2004,
Efficient Integration of Highly Eccentric Orbits by
Quadruple Scaling Method for Kustaanheimo-Stiefel Regularization
|
54. |
Fukushima, T., Astron. J., 128, 3114-3122, 2004,
Efficient Integration of Highly Eccentric Orbits by Single
Scaling Method Applied to Kustaanheimo-Stiefel Regularization
|
53. |
Fukushima, T., Astron. J., 128, 1455-1464, 2004,
Efficient Orbit Integration by Orbital Longitude Method
Using Anti-Focal Anomaly
|
52. |
Fukushima, T., Astron. J., 128, 1446-1454, 2004,
Further Simplification of a Manifold Correction Method for Orbit
Integration
|
51. |
Fukushima, T., Astron. J., 128, 920-922, 2004,
Simplification of a Manifold Correction Method for Orbit Integration
|
50. |
Fukushima, T., Astron. J., 127, 3638-3641, 2004,
Efficient Orbit Integration by Linear Transformation for
Consistency of Kepler Energy, Laplace Integral, and Angular
Momentum Vector
|
49. |
Harada, W., and Fukushima, T.,Astron. J., 127, 531-538, 2004,
New Determination of Planetary Precession
|
48. |
Ohnishi, K., Hosokawa, M., and Fukushima, T., Progr. Theor.
Phys. Suppl., 155, 395-397, 2004,
Macro Lens toward the Galactic Center
|
47. |
Fukushima, T., Astron. J., 126, 3138-3142, 2003,
Efficient Orbit Integration by Scaling and Rotation for
Consistency of Kepler Energy, Laplace Integral, and Angular
Momentum Direction
|
46. |
Fukushima, T., Astron. J., 126, 2567-2573, 2003,
Efficient Orbit Integration by Dual Scaling for Consistency of
Kepler Energy and Laplace Integral
|
45. |
Fukushima, T., Astron. J., 126, 1097-1111, 2003,
Efficient Orbit Integration by Scaling for Kepler Energy Consistency
|
44. |
Fukushima, T., Astron. J., 126, 494-534, 2003,
New Precession Formula
|
43. |
Harada, W., and Fukushima, T., Astron. J., 126, 2557-256, 2003,
Harmonic Decomposition of Time Ephemeris TE405
|
42. |
Neta, B., and Fukushima, T., Comp. and Math. with Appl., 45,
383-390, 2003, Obrechkoff versus Super-Implicit Methods for the
Solution of First and Second Order Initial Value Problems
|
41. |
Soffel, M., Klioner, S.A., Petit, G., Wolf, P., Kopeikin, S.M.,
Bretagnon, P., Brumberg, V.A., Capitaine, N., Damour, T.,
Fukushima, T., et al., Astron. J., 126, 2687-2706, 2003,
The IAU 2000 Resolutions for Astrometry, Celestial Mechanics,
and Metrology in the Relativistic Framework: Explanatory Supplement
|
40. |
Hosokawa, M., Jauncey, D., Reynolds, J., Tzioumis, A., Ohnishi, K.,
and Fukushima, T., Astrophys. J., 580, L43-L46, 2002,
Possible Fluctuation of the Position of Sagittarius A* Relative to
Extragalactic Radio Sources
|
39. |
Arakida, H., and Fukushima, T., Astron. J. 121, 1764-1767, 2001,
Long-Term Integration Error of Kustaanheimo-Stiefel Regularized
Orbital Motion II: Method of Variation of Parameters
|
38. |
Fukushima, T., Astron. J., 122, 482-486, 2001,
Global Rotation of Non-Rotating Origin
|
37. |
Fukushima, T., Astron. J., 121, 1768-1775, 2001,
Reduction of Round-off Errors in Symplectic Integrators
|
36. |
Fukushima, T., J. Geod. Soc. Japan, 47, 213-218, 2001,
Longitude Origins on Moving Equator
|
35. |
Shirai, T., and Fukushima, T., Geophys. Res. Lett., 28, 3553-3556,
2001, Detection of Excitations of Free Core Nutation of the Earth
and their Concurrence with Huge Earthquakes
|
34. |
Shirai, T., and Fukushima, T., Astron. J., 121, 3270-3283, 2001,
Construction of New Forced Nutation Theory of Non-Rigid Earth
|
33. |
Shirai, T., and Fukushima, T., J. Geod. Soc. Japan, 47,
198-203, 2001, Did Huge Earthquakes excite Free-Core Nutation of
the Eartth?
|
32. |
Arakida, H., and Fukushima, T., Astron. J., 120, 3333-3339, 2000,
Long-Term Integration Error of Kustaanheimo-Stiefel Regularized
Orbital Motion
|
31. |
Shirai, T., and Fukushima, T., Astron. J., 119, 2475-2480, 2000,
Numerical Convolution in the Time Domain and Its Application to
the Nonrigid-Earth Nutation Theory
|
30. |
Fukushima, T., J. Geodesy, 73, 603-610, 1999,
Fast Transform from Geocentric to Geodetic Coordinates
|
29. |
Fukushima, T., Celest. Mech. Dyn. Astron., 75, 201-226, 1999,
Fast Procedures Solving Universal Kepler's Equation
|
28. |
Fukushima, T., Celest. Mech. Dyn. Astron., 73, 231-241, 1999,
Parallel/Vector Integration Methods for Dynamical Astronomy
|
27. |
Hosokawa, M., Ohnishi, K., and Fukushima, T., Astron. Astrophys.,
351, 393-397, 1999, Uncertainty of Pulsar Time Scale due to the
Gravitational Time Delay of Intervening Stars and MACHOs
|
26. |
Irwin, A., and Fukushima, T., Astron. Astrophys., 348, 642-652,
1999, A Numerical Time Ephemeris of the Earth
|
25. |
Fukushima, T., Celest. Mech., 70, 115-130, 1998,
A Fast Procedure Solving Gauss' Form of Kepler's Equation
|
24. |
Fukushima, T., Astron. J., 113, 2325-2328, 1997,
Vector Integration of Dynamical Motions by the Picard-Chebyshev Method
|
23. |
Fukushima, T., Astron. J., 113, 1920-1924, 1997,
A procedure Solving the Extended Kepler's Equation for the
Hyperbolic Case
|
22. |
Fukushima, T., Astron. J., 113, 1909-1914, 1997,
Picard Iteration Method, Chebyshev Polynomial Approximation,
and Global Numerical Integration of Dynamical Motions
|
21. |
Fukushima, T., Celest. Mech. Dyn. Astron., 68, 121-137, 1997,
A Method Solving Kepler's Equation for Hyperbolic Case
|
20. |
Fukushima, T., Celest. Mech. Dyn. Astron., 66, 309-319, 1997,
A Method Solving Kepler's Equation without Transcendental Function
Evaluations
|
19. |
Fukushima, T., Celest. Mech. Dyn. Astron., 66, 107-114, 1997,
Reference Systems
|
18. |
Hosokawa, M., Ohnishi, K., and Fukushima, T., Astron. J., 114,
1508-1516, 1997, Fluctuation of Extragalactic Reference Frame
due to Gravitational Lensing in Our Galaxy
|
17. |
Ito, T., and Fukushima, T., Astron. J., 114, 1260-1267, 1997,
Parallelized Extrapolation Method and its Application to the
Orbital Dynamics
|
16. |
Fukushima, T., Astron. J., 112, 2858-2861, 1996,
A Fast Procedure Solving Kepler's Equation for Elliptic Case
|
15. |
Fukushima, T., Astron. J., 112, 1298-1301, 1996,
Reduction of Round-off Errors in the Extrapolation Methods and
its Application to the Integration of Orbital Motion
|
14. |
Fukushima, T., Astron. J., 112, 1263-1277, 1996,
Generalization of Encke's Method and its Application to the
Orbital and Rotational Motions of Celestial Objects
|
13. |
Fukushima, T., Astron. Astrophys., 294, 895-906, 1995,
Time Ephemeris
|
12. |
Ohnishi, K., Hosokawa, M., Fukushima, T., and Takeuti, M.,
Astrophys. J., 448, 271-280, 1995,
Variation of Gravitational Delay in Pulsar Timing Observation
due to Proper Motion of Foreground Stars and Measurement of Stellar Mass
|
11. |
Fukushima, T., Astron. Astrophys., 291, 320-323, 1994,
Lunar VLBI Observation Model
|
10. |
Brumberg, E. and Fukushima, T., Celest. Mech. Dyn. Astron., 60,
69-89, 1994,
Expansions of Elliptic Motion based on Elliptic Function Theory
|
9. |
Fukushima, T., Celest. Mech. Dyn. Astron., 60, 57-68, 1994,
New Canonical Variables for Orbital and Rotational Motions
|
8. |
Fukushima, T, and Ishizaki, H., Celest. Mech. Dyn. Astron., 59,
237-251, 1994,
Numerical Computation of Incomplete Elliptic Integrals of a
General Form
|
7. |
Fukushima, T, and Ishizaki, H., Celest. Mech. Dyn. Astron., 59,
149-159, 1994, Elements of Spin Motion
|
6. |
Hosokawa, M., Ohnishi, K., Fukushima, T., and Takeuti, M.,
Astron. Astrophys., 278, L27-L30, 1993, Parallactic Variation of
Gravitational Lensing and Measurement of Stellar Mass
|
5. |
Seildelmann, P.K., and Fukushima, T., Astron. Astrophys., 265,
833-838, 1992, Why New Time Scales?
|
4. |
Fukushima, T., Astron. Astrophys., 244, L11-L12, 1991,
Geodesic Nutation
|
3. |
Fukushima, T., Celest. Mech., 45, 73-76, 1989, Tests of the
Extrapolation Method for the Numerical Integration of the
Keplerian Motion
|
2. |
Fukushima, T., Celest. Mech., 44, 61-75, 1988,
The Fermi Coordinate System in the Post-Newtonian Framework
|
1. |
Fukushima, T., Fujimoto, M.-K., Kinoshita, H., and Aoki, S.,
Celest. Mech., 36, 215-230, 1986,
A System of Astronomical Constants in the Post-Newtonian Framework
|
21. |
Fukushima, T., Proc. Journees 2000, in preparation, 2001,
Report on Astronomical Constants
|
20. |
Fukushima, T., Highlights of Astronomy, 12B, in preparation, 2001,
Report on Astronomical Constants
|
19. |
Fukushima, T., Hosokawa, M., Ohnishi, K., Jauncey, D., Reynolds,
J., and Tzioumis., Highlights of Astronomy, 12B, in preparation,
2001, Possible Fluctuation of the Position of Sgr A* relative to
extragalactic
|
18. |
Fukushima, T., Proc. IAU Coll., 180, 417, 2000,
Report on Astronomical Constants
|
17. |
Fukushima, T., Proc. IAU Coll., 173, 309, 1999,
Symmetric Multistep Methods Revisted: II Numerical Experiments
|
16. |
Fukushima, T., Proc. Celest. Mech. Symp., 31, 343, 1999,
Super Implicit Multistep Methods
|
15. |
Sato, K., Nishikawa, J., Yoshizawa, M., Fukushima, T.,
Machida, Y., Honma, Y., Kuwabara, R., Suzuki, S., Torii, Y.,
Kubo, K., Matsuda, K., and Iwashita, H., Proc. SPIE, 3350, 212,
1998, Development of the Optical and Infrared Interferometer MIRA-I.2
|
14. |
Machida, Y., Nishikawa, J., Sato, K., Fukushima, T., Yoshizawa, M.,
Honma, Y., Torii, Y., Matsuda, K., Kubo, K., Ohashi, M., Suzuki,
S., and Iwashita, H., Proc. SPIE, 3350, 202, 1998,
MIRA-I Project: Development of the Mitaka Optical and Infrared
Stellar Interferometer
|
13. |
Nishikawa, J., Sato, K., Fukushima, T., Yoshizawa, M., Machida, Y.,
and Honma, Y., Proc. SPIE, 3350, 184, 1998,
MIRA-II, MIRA-III, and MIRA-SG Projects: the Future Plan of
Long-Baseline Optical/IR Interferometers in Japan
|
12. |
Fukushima, T., Proc. IAU Coll., 172, 231, 1998,
Parallel/Vector Integration Methods for Dynamical Astronomy
|
11. |
Brumberg, V.A., Bretagnon, P., Capitaine, N., Damour, T.,
Eubanks, T.M., Fukushima, T., Guinot, B., Klioner, S.A.,
Kopeikin, S.M., Krivov, A.V., Seidelmann, P.K., and Soffel, M.H.,
Highlights of Astronomy, 11B, 194, 1998,
General Relativity and the IAU Resolutions
|
10. |
Dehant, V., and Fukushima T., Highlights of Astronomy,
11B, 151, 1998, Introduction of JD3: on 'Precession, Nutation,
and Astronomical Constants in the Dawn of the 21st Century'
|
9. |
Dehant, V., and Fukushima T., Highlights of Astronomy, 11B, 149,
1998, Precession-Nutation and Astronomical Constants in the Dawn
of the 21st Century
|
8. |
Fukushima, T., Proc. Celest. Mech. Symp., 30, 229, 1998,
Symmetric Multistep Methods Revisted
|
7. |
Sato, K., Nishikawa, J., Yoshizawa, M., Fukushima, T., Machida, Y.,
and Miyamoto, M., Highlights of Astronomy, 11B, 29, 1998,
Astrometry with Optical and Infrared Interferometer
|
6. |
Nishikawa, J., Sato, K., Fukushima, T., Yoshizawa, M., Machida, Y.,
and Miyamoto, M., Highlights of Astronomy, 11B, 28, 1998,
Milliarcsecond Astrometric Interferometer: Mitaka Optical and
Infrared Array (MIRA)
|
5. |
Yoshizawa, M., Sato, K., Nishikawa, J., Fukushima, T., and
Miyamoto, M., ESASP, 402, 795, 1997,
An Optical/Infrared Astrometric Satellite Project LIGHT
|
4. |
Yoshizawa, M., Sato, K., Nishikawa, J., Fukushima, T., and
Miyamoto, M., Proc. IAU Coll., 165, 561, 1997,
Two Astrometric Projects: LIGHT and MIRA
|
3. |
Fukushima, T., Proc. IAU Symp., 172, 461, 1996,
IAU Standards - its Future. (Lecture)
|
2. |
Fukushima, T., Proc. IAU Symp., 172, 245, 1996,
A Numerilca Scheme to Integrate the Rotational Motion of a Rigid Body
|
1. |
Ito, T., Kinoshita, H., Nakai, H., and Fukushima, T.,
Proc. Celest. Mech. Symp., 28, 123, 1996,
Numerical Experiments to Inspect the Long-Term Stability of the
Planetary Motion (-1)
|