Coherent signal arraying of voyager-Neptune radio occultation data : data analysis and improvement of physical measurements ボイジャー海王星電波科学データのコヒーレントな重ね合せ : データ解析及び観測精度の向上

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著者

    • 水野, 英一 ミズノ, エイイチ

書誌事項

タイトル

Coherent signal arraying of voyager-Neptune radio occultation data : data analysis and improvement of physical measurements

タイトル別名

ボイジャー海王星電波科学データのコヒーレントな重ね合せ : データ解析及び観測精度の向上

著者名

水野, 英一

著者別名

ミズノ, エイイチ

学位授与大学

東京大学

取得学位

博士 (理学)

学位授与番号

甲第9209号

学位授与年月日

1991-06-24

注記・抄録

博士論文

目次

  1. Contents / p7 (0005.jp2)
  2. 1 Introduction / p1 (0009.jp2)
  3. 1.1 Radio occupation experiments with Jupiter,Saturn,and Uranus / p2 (0010.jp2)
  4. 1.2 Radio occultation experiment with Neptune / p7 (0012.jp2)
  5. 1.3 Contributions in dissertation work / p11 (0014.jp2)
  6. 1.4 Overview / p12 (0015.jp2)
  7. 2 Voyager-Neptune Encounter Experiment / p17 (0017.jp2)
  8. 2.1 Experiment summary / p17 (0017.jp2)
  9. 2.2 Geometry / p18 (0018.jp2)
  10. 2.3 Transmission of the signal / p20 (0019.jp2)
  11. 2.4 Reception of the signal / p24 (0021.jp2)
  12. 3 Arraying Method / p37 (0027.jp2)
  13. 3.1 Principle of coherent arraying / p37 (0027.jp2)
  14. 3.2 Limitations in arraying / p43 (0030.jp2)
  15. 3.3 Interpretation of the observables / p59 (0038.jp2)
  16. 3.4 Reduction of noise bandwidth / p60 (0039.jp2)
  17. 3.5 Synchronization of the sample timing between the different stations / p68 (0043.jp2)
  18. 3.6 Differential phase / p73 (0045.jp2)
  19. 4 Results and Comparison / p77 (0047.jp2)
  20. 4.1 Interpretation of unarrayed data / p77 (0047.jp2)
  21. 4.2 Differential phase / p83 (0050.jp2)
  22. 4.3 Comparison of the 8.4 GHz data before and after arraying / p86 (0052.jp2)
  23. 4.4 Comparison of the 2.3 GHz Data before and after Arraying / p90 (0054.jp2)
  24. 4.5 Discussion / p94 (0056.jp2)
  25. 5 Physics with Radio Occultation Data / p99 (0058.jp2)
  26. 5.1 The effect of Neptune's ionosphere on radio occultation data / p99 (0058.jp2)
  27. 5.2 Temperature-pressure profile of Neptune's neutral atmosphere deduced from the Usuda 2.3 GHz data / p116 (0067.jp2)
  28. 6 Summary and Conclusions / p123 (0070.jp2)
  29. 6.1 Summary of results / p124 (0071.jp2)
  30. 6.2 Conclusions / p125 (0071.jp2)
  31. 6.3 Future Work / p126 (0072.jp2)
  32. A Temperatute-Pressure Profile of a Spherically Symmetric Planet / p129 (0073.jp2)
  33. B Optimal Arrayed SNR of η Signals with Noise / p133 (0075.jp2)
  34. C Geometry in Arraying / p137 (0077.jp2)
  35. C.1 Receiving station locations / p137 (0077.jp2)
  36. C.2 Cartesian coordinate system / p139 (0078.jp2)
  37. C.3 EME50 coordinate system / p142 (0080.jp2)
  38. C.4 Light time equation / p145 (0081.jp2)
  39. C.5 Doppler frequency / p146 (0082.jp2)
  40. D Interpolation of Data by Polynomials / p149 (0083.jp2)
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各種コード

  • NII論文ID(NAID)
    500000098325
  • NII著者ID(NRID)
    • 8000000098554
  • DOI(NDL)
  • NDL書誌ID
    • 000000262639
  • データ提供元
    • NDL-OPAC
    • NDLデジタルコレクション
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