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Journal articles on the topic 'Interplanetary science'

Author: Grafiati

Published: 6 September 2023

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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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11

Hooke, Adrian. "The interplanetary Internet." Communications of the ACM 44, no. 9 (2001): 38–40. http://dx.doi.org/10.1145/383694.383703.

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12

Kalinichenko, M. M., N. V. Kuhai, O. O. Konovalenko, et al. "INVESTIGATIONS OF COSMIC SOURCES RADIOEMISSION SCINTILLATIONS DUE TO INTERPLANETARY PLASMA IRREGULARITIES AT THE INSTITUTE OF RADIO ASTRONOMY, NAS UKRAINE." Radio physics and radio astronomy 26, no. 2 (2021): 148–64. http://dx.doi.org/10.15407/rpra26.02.148.

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Purpose: Review of investigations of cosmic sources radioemission scintillations due to interplanetary plasma irregularities made at the Institute of Radio Astronomy of the National Academy of Sciences of Ukraine, from the first observations in the mid-70s until now. Design/methodology/approach: In the course of preparation of this paper, the authors have reviewed, analyzed and summarized the information being published in the home and foreign publications, and reported at scientific conferences. Findings: The investigations of the interplanetary scintillations carried out at the Institute of

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13

Craig, H. "Retention of Helium in Subducted Interplanetary Dust Particles." Science 265, no. 5180 (1994): 1892–93. http://dx.doi.org/10.1126/science.265.5180.1892.

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14

JOKIPII, J. R. "Cosmic Rays: Cosmic Rays In Interplanetary Magnetic Fields." Science 233, no. 4762 (1986): 483. http://dx.doi.org/10.1126/science.233.4762.483.

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15

Rossi, Bruno. "The Interplanetary Plasma." Annual Review of Astronomy and Astrophysics 29, no. 1 (1991): 1–9. http://dx.doi.org/10.1146/annurev.aa.29.090191.000245.

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16

Ballatore, P., J. P. Villain, N. Vilmer, and M. Pick. "The influence of the interplanetary medium on SuperDARN radar scattering occurrence." Annales Geophysicae 18, no. 12 (2000): 1576–83. http://dx.doi.org/10.1007/s00585-001-1576-2.

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Abstract. The effects of the characteristics of the interplanetary medium on the radar scattering occurrence, related to the whole array of SuperDARN radars installed in the Northern Hemisphere, have been studied over a two-year period. Statistically significant correlations of the variation of the scattering occurrence are found with the merging electric field and with the negative Bz component of the interplanetary magnetic field, independent of the seasonal period considered. This result demonstrates that the merging rate (and in particular the reconnection process) between the interplaneta

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17

Janardhan, P., V. Balasubramanian, S. Ananthakrishnan, M. Dryer, A. Bhatnagar, and P. S. McIntosh. "Travelling interplanetary disturbances detected using interplanetary scintillation at 327 MHz." Solar Physics 166, no. 2 (1996): 379–401. http://dx.doi.org/10.1007/bf00149405.

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18

Vilmer, N., M. Pick, R. Schwenn, P. Ballatore, and J. P. Villain. "On the solar origin of interplanetary disturbances observed in the vicinity of the Earth." Annales Geophysicae 21, no. 4 (2003): 847–62. http://dx.doi.org/10.5194/angeo-21-847-2003.

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Abstract. The solar origin of 40 interplanetary disturbances observed in the vicinity of the Earth between January 1997 and June 1998 is investigated in this paper. Analysis starts with the establishment of a list of Interplanetary Mass Ejections or ICMEs (magnetic clouds, flux ropes and ejecta) and of Interplanetary Shocks measured at WIND for the period for which we had previously investigated the coupling of the interplanetary medium with the terrestrial ionospheric response. A search for associated coronal mass ejections (CMEs) observed by LASCO/SOHO is then performed, starting from an est

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19

Lam, H. L., D. H. Boteler, and L. Trichtchenko. "Case studies of space weather events from their launching on the Sun to their impacts on power systems on the Earth." Annales Geophysicae 20, no. 7 (2002): 1073–79. http://dx.doi.org/10.5194/angeo-20-1073-2002.

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Abstract. Active geomagnetic conditions on 12–13, 15–16, and 22–23 September 1999 resulted in geomagnetically induced currents (GIC) measurable in power systems in Canada and the United States. Different solar origins for these three events gave rise to dissimilar interplanetary signatures. We used these events to present three case studies, each tracing an entire space weather episode from its inception on the Sun, propagation through the interplanetary medium, manifestation on the ground as intense magnetic and electric fluctuations, and its eventual impact on technological systems.Key words

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20

Bravo, S., and X. Blanco-Cano. "Signatures of interplanetary transients behind shocks and their associated near-surface solar activity." Annales Geophysicae 16, no. 4 (1998): 359–69. http://dx.doi.org/10.1007/s00585-998-0359-4.

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Abstract. Interplanetary transients with particular signatures different from the normal solar wind have been observed behind interplanetary shocks and also without shocks. In this paper we have selected four well-known transient interplanetary signatures, namely: magnetic clouds, helium enhancements and bidirectional electron and ion fluxes, found in the solar wind behind shocks, and undertaken a correlative study between them and the corresponding solar observations. We found that although commonly different signatures appear in a single interplanetary transient event, they are not necessari

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21

Bradley, J. "An Astronomical 2175 A Feature in Interplanetary Dust Particles." Science 307, no. 5707 (2005): 244–47. http://dx.doi.org/10.1126/science.1106717.

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22

von Hegner, Ian. "Interplanetary transmissions of life in an evolutionary context." International Journal of Astrobiology 19, no. 4 (2020): 335–48. http://dx.doi.org/10.1017/s1473550420000099.

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AbstractThe theory of lithopanspermia proposes the natural exchange of organisms between solar system bodies through meteorites. The focus of this theory comprises three distinct stages: planetary ejection, interplanetary transit and planetary entry. However, it is debatable whether organisms transported within the ejecta can survive all three stages. If the conjecture is granted, that life can indeed be safely transmitted from one world to another, then it is not only a topic pertaining to planetary science but also biological sciences. Hence, these stages are only the first three factors of

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23

Anttila, A., L. G. Kocharov, J. Torsti, and R. Vainio. "Long-duration high-energy proton events observed by GOES in October 1989." Annales Geophysicae 16, no. 8 (1998): 921–30. http://dx.doi.org/10.1007/s00585-998-0921-0.

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Abstract. We consider the prolonged injection of the high-energy (>10 MeV) protons during the three successive events observed by GOES in October 1989. We apply a solar-rotation-stereoscopy approach to study the injection of the accelerated particles from the CME-driven interplanetary shock waves in order to find out how the effectiveness of the particle acceleration and/or escape depends on the angular distance from the shock axis. We use an empirical model for the proton injection at the shock and a standard model of the interplanetary transport. The model can reproduce rather well the ob

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24

Malandraki, O. E., E. T. Sarris, and G. Tsiropoula. "Magnetic topology of coronal mass ejection events out of the ecliptic: Ulysses/HI-SCALE energetic particle observations." Annales Geophysicae 21, no. 6 (2003): 1249–56. http://dx.doi.org/10.5194/angeo-21-1249-2003.

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Abstract. Solar energetic particle fluxes (Ee > 38 keV) observed by the ULYSSES/HI-SCALE experiment are utilized as diagnostic tracers of the large-scale structure and topology of the Interplanetary Magnetic Field (IMF) embedded within two well-identified Interplanetary Coronal Mass Ejections (ICMEs) detected at 56° and 62° south heliolatitudes by ULYSSES during the solar maximum southern high-latitude pass. On the basis of the energetic solar particle observations it is concluded that: (A) the high-latitude ICME magnetic structure observed in May 2000 causes a depression in the solar energ

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25

Lanzerotti, L., T. Armstrong, R. Gold, et al. "Over the southern solar pole: low-energy interplanetary charged particles." Science 268, no. 5213 (1995): 1010–13. http://dx.doi.org/10.1126/science.7754378.

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26

Gurnett, D. A., W. S. Kurth, S. C. Allendorf, and R. L. Poynter. "Radio Emission from the Heliopause Triggered by an Interplanetary Shock." Science 262, no. 5131 (1993): 199–203. http://dx.doi.org/10.1126/science.262.5131.199.

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27

Clemett, S. J., C. R. Maechling, R. N. Zare, P. D. Swan, and R. M. Walker. "Identification of Complex Aromatic Molecules in Individual Interplanetary Dust Particles." Science 262, no. 5134 (1993): 721–25. http://dx.doi.org/10.1126/science.262.5134.721.

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28

Bradley, J. P. "Chemically Anomalous, Preaccretionally Irradiated Grains in Interplanetary Dust from Comets." Science 265, no. 5174 (1994): 925–29. http://dx.doi.org/10.1126/science.265.5174.925.

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29

HORD, C. W., C. A. BARTH, L. W. ESPOSITO, et al. "Galileo Ultraviolet Spectrometer Experiment: Initial Venus and Interplanetary Cruise Results." Science 253, no. 5027 (1991): 1548–50. http://dx.doi.org/10.1126/science.253.5027.1548.

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30

Colwell, J. E. "Capture of Interplanetary and Interstellar Dust by the Jovian Magnetosphere." Science 280, no. 5360 (1998): 88–91. http://dx.doi.org/10.1126/science.280.5360.88.

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31

Baxter, Stepen. "Fast Interplanetary Travel: a Literature Review." Journal of the British Interplanetary Society 76, no. 5 (2023): 163–69. http://dx.doi.org/10.59332/jbis-076-05-163.

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The project to which this paper is a contribution is a prospectus for the integrated industrial development of the Solar System. Fast transit on an interplanetary scale is a prerequisite before such a development can be established. To facilitate this freedom of movement, this study has defined a suite of fast, large-scale interplanetary ships, achievable in the relatively near term. As background, the present paper is a review of the literature on the feasibility of fast, large-scale, nuclear-powered, cargo carrying and/or crewed interplanetary craft, as explored historically from the develop

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32

Baxter, Stephen. "Fast Interplanetary Travel: a Literature Review." Journal of the British Interplanetary Society 76, no. 5 (2023): 163–69. http://dx.doi.org/10.59332/jbis-076-05-0163.

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The project to which this paper is a contribution is a prospectus for the integrated industrial development of the Solar System. Fast transit on an interplanetary scale is a prerequisite before such a development can be established. To facilitate this freedom of movement, this study has defined a suite of fast, large-scale interplanetary ships, achievable in the relatively near term. As background, the present paper is a review of the literature on the feasibility of fast, large-scale, nuclear-powered, cargo-carrying and/or crewed interplanetary craft, as explored historically from the develop

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33

Divine, Neil. "Five populations of interplanetary meteoroids." Journal of Geophysical Research 98, E9 (1993): 17029. http://dx.doi.org/10.1029/93je01203.

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34

Whang, Y. C. "Evolution of interplanetary slow shocks." Journal of Geophysical Research 93, A1 (1988): 251. http://dx.doi.org/10.1029/ja093ia01p00251.

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35

Cane, H. V. "The evolution of interplanetary shocks." Journal of Geophysical Research: Space Physics 90, A1 (1985): 191–97. http://dx.doi.org/10.1029/ja090ia01p00191.

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36

Marchese, Mario. "Interplanetary and pervasive communications." IEEE Aerospace and Electronic Systems Magazine 26, no. 2 (2011): 12–18. http://dx.doi.org/10.1109/maes.2011.5739484.

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37

Xiao, T., Q. Q. Shi, T. L. Zhang, et al. "Cluster-C1 observations on the geometrical structure of linear magnetic holes in the solar wind at 1 AU." Annales Geophysicae 28, no. 9 (2010): 1695–702. http://dx.doi.org/10.5194/angeo-28-1695-2010.

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Abstract. Interplanetary linear magnetic holes (LMHs) are structures in which the magnetic field magnitude decreases with little change in the field direction. They are a 10–30% subset of all interplanetary magnetic holes (MHs). Using magnetic field and plasma measurements obtained by Cluster-C1, we surveyed the LMHs in the solar wind at 1 AU. In total 567 interplanetary LMHs are identified from the magnetic field data when Cluster-C1 was in the solar wind from 2001 to 2004. We studied the relationship between the durations and the magnetic field orientations, as well as that of the scales and

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38

IPATOV, S. I., J. C. MATHER, and P. A. TAYLOR. "Migration of Interplanetary Dust." Annals of the New York Academy of Sciences 1017, no. 1 (2004): 66–80. http://dx.doi.org/10.1196/annals.1311.005.

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39

Watari, S., and T. Detman. "In situ local shock speed and transit shock speed." Annales Geophysicae 16, no. 4 (1998): 370–75. http://dx.doi.org/10.1007/s00585-998-0370-9.

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Abstract. A useful index for estimating the transit speeds was derived by analyzing interplanetary shock observations. This index is the ratio of the in situ local shock speed and the transit speed; it is 0.6–0.9 for most observed shocks. The local shock speed and the transit speed calculated for the results of the magnetohydrodynamic simulation show good agreement with the observations. The relation expressed by the index is well explained by a simplified propagation model assuming a blast wave. For several shocks the ratio is approximately 1.2, implying that these shocks accelerated during p

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40

Chashei, I. V., S. А. Tyul’bashev, and Yu V. Pisanko. "Monitoring of Interplanetary Scintillation and Potential of Short-time Space Weather Forecasting." Meteorologiya i Gidrologiya 3 (2021): 28–37. http://dx.doi.org/10.52002/0130-2906-2021-3-28-37.

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Observations and initial analysis of interplanetary scintillation data are briefly described in the framework of the program for the solar wind monitoring with the modernized LPI LPA radio telescope that started in 2014. The examples of detecting interplanetary coronal mass injections (ICME) and co-rotating interaction regions (СIR) of different-speed flows are presented. It is shown that in the first case, enhancements in the scintillation level in extended sounded regions of solar wind are observed 20–30 hours before the arrival of the disturbances to the Earth; in the second case, the eveni

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41

Malandraki, O., E. T. Sarris, and P. Trochoutsos. "Probing the magnetic topology of coronal mass ejections by means of Ulysses/HI-SCALE energetic particle observations." Annales Geophysicae 18, no. 2 (2000): 129–40. http://dx.doi.org/10.1007/s00585-000-0129-4.

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Abstract. In this work, solar flare energetic particle fluxes (Ee ≥ 42 keV) observed by the HI-SCALE instrument onboard Ulysses, a spacecraft that is probing the heliosphere in 3-D, are utilized as diagnostics of the large-scale structure and topology of the interplanetary magnetic field (IMF) embedded within two well-identified interplanetary coronal mass ejection (ICME) structures. On the basis of the energetic solar flare particle observations firm conclusions are drawn on whether the detected ICMEs have been detached from the solar corona or are still magnetically anchored to it when they

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42

Nielsen, E., and F. Honary. "Observations of ionospheric flows and particle precipitation following a Sudden Commencement." Annales Geophysicae 18, no. 8 (2000): 908–17. http://dx.doi.org/10.1007/s00585-000-0908-y.

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Abstract. On May 4, 1998, at 0227 UT an interplanetary shock crossed the WIND spacecraft, and half an hour later a Sudden Commencement occurred. Coinciding with the Sudden Commencement a rapid intensification of the flux of particle precipitation into the ionosphere was observed. Evidence is presented that the ionospheric electric fields were influenced by the associated dynamic variations of the ionospheric conductivities. Following the initial phase the ionospheric flow speeds increased rapidly over the next 20 min to more than 2000 m/s, in agreement with an increased effective coupling of t

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43

Feng, HengQiang, GuoQing Zhao, and JieMin Wang. "Small interplanetary magnetic flux rope." Science China Technological Sciences 63, no. 2 (2019): 183–94. http://dx.doi.org/10.1007/s11431-018-9481-1.

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44

Floss, C. "Carbon and Nitrogen Isotopic Anomalies in an Anhydrous Interplanetary Dust Particle." Science 303, no. 5662 (2004): 1355–58. http://dx.doi.org/10.1126/science.1093283.

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45

Reiner, M. J., J. Fainberg, and R. G. Stone. "Large-Scale Interplanetary Magnetic Field Configuration Revealed by Solar Radio Bursts." Science 270, no. 5235 (1995): 461–64. http://dx.doi.org/10.1126/science.270.5235.461.

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46

Kortenkamp, S. J. "A 100,000-Year Periodicity in the Accretion Rate of Interplanetary Dust." Science 280, no. 5365 (1998): 874–76. http://dx.doi.org/10.1126/science.280.5365.874.

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47

Yamakawa, Hiroshi. "Optimal Radially Accelerated Interplanetary Trajectories." Journal of Spacecraft and Rockets 43, no. 1 (2006): 116–20. http://dx.doi.org/10.2514/1.13317.

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48

Feynman, Joan, T. P. Armstrong, L. Dao-Gibner, and S. Silverman. "New interplanetary proton fluence model." Journal of Spacecraft and Rockets 27, no. 4 (1990): 403–10. http://dx.doi.org/10.2514/3.26157.

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49

Zubrin, Robert M., and Dana G. Andrews. "Magnetic sails and interplanetary travel." Journal of Spacecraft and Rockets 28, no. 2 (1991): 197–203. http://dx.doi.org/10.2514/3.26230.

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50

Garrett, Henry B., S. J. Drouilhet, John P. Oliver, and R. W. Evans. "Interplanetary Meteoroid Environment Model Update." Journal of Spacecraft and Rockets 36, no. 1 (1999): 124–32. http://dx.doi.org/10.2514/2.3424.

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