Academic literature on the topic 'Interplanetary science'

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Journal articles on the topic "Interplanetary science"

1

DONN, B. "Interplanetary Dust: Properties and Interactions of Interplanetary Dust." Science 233, no. 4764 (1986): 673. http://dx.doi.org/10.1126/science.233.4764.673.

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2

Exarhos, G., and X. Moussas. "On the heliolatitudinal variation of the galactic cosmic-ray intensity. Comparison with Ulysses measurements." Annales Geophysicae 21, no. 6 (2003): 1341–45. http://dx.doi.org/10.5194/angeo-21-1341-2003.

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Abstract. We study the dependence of cosmic rays with heliolatitude using a simple method and compare the results with the actual data from Ulysses and IMP spacecraft. We reproduce the galactic cosmic-ray heliographic latitudinal intensity variations, applying a semi-empirical, 2-D diffusion-convection model for the cosmic-ray transport in the interplanetary space. This model is a modification of our previous 1-D model (Exarhos and Moussas, 2001) and includes not only the radial diffusion of the cosmic-ray particles but also the latitudinal diffusion. Dividing the interplanetary region into "s
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3

Martin-Mur, T. J., G. L. Kruizinga, P. D. Burkhart, F. Abilleira, M. C. Wong, and J. A. Kangas. "Mars Science Laboratory Interplanetary Navigation." Journal of Spacecraft and Rockets 51, no. 4 (2014): 1014–28. http://dx.doi.org/10.2514/1.a32631.

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4

Martin-Mur, Tomas J., Gerard L. Kruizinga, and Mau C. Wong. "Mars science laboratory interplanetary navigaton analysis." Journal of Aerospace Engineering, Sciences and Applications 4, no. 2 (2012): 107–20. http://dx.doi.org/10.7446/jaesa.0402.10.

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5

Zweibel, E. G. "The Solar Wind: Interplanetary Magnetohydrodynamics." Science 272, no. 5261 (1996): 495b—496b. http://dx.doi.org/10.1126/science.272.5261.495b.

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6

CHRISTOFFERSEN, R., and P. R. BUSECK. "Refractory Minerals in Interplanetary Dust." Science 234, no. 4776 (1986): 590–92. http://dx.doi.org/10.1126/science.234.4776.590.

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7

ZOLENSKY, M. E. "Reports Refractory Interplanetary Dust Particles." Science 237, no. 4821 (1987): 1466–68. http://dx.doi.org/10.1126/science.237.4821.1466.

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8

Hand, Eric. "Interplanetary small satellites come of age." Science 361, no. 6404 (2018): 736–37. http://dx.doi.org/10.1126/science.361.6404.736.

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9

Watari, S., M. Vandas, and T. Watanabe. "Formation of a strong southward IMF near the solar maximum of cycle 23." Annales Geophysicae 22, no. 2 (2004): 673–87. http://dx.doi.org/10.5194/angeo-22-673-2004.

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Abstract. We analyzed observations of the solar activities and the solar wind parameters associated with large geomagnetic storms near the maximum of solar cycle 23. This analysis showed that strong southward interplanetary magnetic fields (IMFs), formed through interaction between an interplanetary disturbance, and background solar wind or between interplanetary disturbances are an important factor in the occurrence of intense geomagnetic storms. Based on our analysis, we seek to improve our understanding of the physical processes in which large negative Bz's are created which will lead to im
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10

Smith, D. E. "Two-Way Laser Link over Interplanetary Distance." Science 311, no. 5757 (2006): 53. http://dx.doi.org/10.1126/science.1120091.

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