Space Weather Study Using Multipoint Techniques

Lyu, L.-H.

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Table of contents
  • Contentsxi
  • Prefacev
  • Opening Address of the COSPAR President to the COSPAR Colloquium on Space Weather Study Using Multi-vii
  • Part I: Keynote Speech1
  • Chapter 1. Predicting Geomagnetic Storms as a Space Weather Project3
  • Part II: Solar Observations and Modeling Session21
  • Chapter 2. Descriptions of Coronal Streamer Structures During the Rising Phase of Cycle 2323
  • Chapter 3. Taiwan Oscillation Network: Probing the Solar Interior31
  • Chapter 4. Space Weather Study Using Combined Coronagraphic and in Situ Observations39
  • Chapter 5. The SECCHI Solar Plasma Imager for STEREO49
  • Chapter 6. Tomographic Analysis of Solar Wind Structure Using Interplanetary Scintillation55
  • Chapter 7. Polar Plumes in Coronal Expansion61
  • Chapter 8. Solar Coronal Heating and Weak Fast Shocks69
  • Chapter 9. An Algorithm of Calculation for the Motion of Looplike Coronal Mass Ejections73
  • Part III: Interplanetary Observations and Modeling Session85
  • Chapter 10. Upstream Shocks and Interplanetary Magnetic Cloud Speed and Expansion: Sun, Wind, and Ea87
  • Chapter 11. Electromagnetic Electron and Proton Cyclotron Waves in Geospace: A Cassini Snapshot97
  • Chapter 12. Models for the Size and Shape of the Earth’s Magnetopause and Bow Shock127
  • Part IV: Magnetospheric Observations and Modeling Session137
  • Chapter 13. Interplanetary Shock Effects on the Nightside Auroral Zone, Magnetosphere, and Ionospher139
  • Chapter 14. Development of an Integrated Predictive MHD Space Weather Model from the Solar Surface t149
  • Chapter 15. Substorms and Magnetic Storms From the Satellite Charging Perspective163
  • Chapter 16. Propagation of Sudden Impulses in the Magnetosphere: Linear and Nonlinear Waves175
  • Chapter 17. Multi-spacecraft Studies in aid of Space Weather Specification and Understanding181
  • Part V: Low-Altitude-Satellite Observations and Modeling Session191
  • Chapter 18. The Electron Density Distribution in the Polar Cap: Its Variability With Seasons, and it193
  • Chapter 19. Two-Level Mesopause and its Variations From UARS-HRDI Temperature Data203
  • Part VI: Ground-Based Observations and Modeling Session207
  • Chapter 20. The Application of High Latitude Ionosphere Radars for Space Weather Research209
  • Chapter 21. Magnetospheric Substorms: An Inner-Magnetospheric Modeling Perspective221
  • Chapter 22. High-Latitude Electrodynamics from a Multi-Array Nonlinear Geomagnetic Model231
  • Chapter 23. Magnetic Impulse Events and Related Pc 1 Waves in the Cusp and LLBL Region Observed by a237
  • Chapter 24. Simultaneous Ground-based Observations of Electric and Magnetic Field Variations Near th243
  • Chapter 25. Global Positioning System Studies of Ionospheric Irregularities249
  • Chapter 26. Equatorial Pc5 Associated With Moving Current Vortices in the High Latitude Ionosphere255
  • Chapter 27. System Phase Bias Estimation of the Chung-Li VHF Radar259
  • Part VII: ROCSAT Program Session265
  • Chapter 28. Effects of Lightning on the Middle and Upper Atmosphere: Some New Results267
  • Chapter 29. Fine Structure of Sprites and Proposed Global Observations275
  • Chapter 30. Spatial and Temporal Structures of Sprites and Elves Observed by Array Photometers283
  • Chapter 31. Observation of Angel Sprites289
  • Chapter 32. The Atmospheric Correction Algorithm of ROCSAT-1/OCI Data295
  • Chapter 33. First Measurement of Scintillation and Attenuation of 19.5 GHz Beacon Signal for Experim301
  • Chapter 34. A New Method of Retrieving Water Vapor Content Using Ground-Based Radiometer with Single307
  • Part VIII: COSMIC Research Program Session313
  • Chapter 35. Modeling, Tracking and Inverting the Tropospheric Radio Occultation Signals315
  • Chapter 36. Active Limb Sounding of Atmospheric Refractivity and dry Temperature Profiles by GPS/MET325
  • Chapter 37. A Study on the COSMIC Electron Density Profile329
  • Chapter 38. Space Geodesy and Climate Change Studies Using COSMIC Mission335
  • Chapter 39. Global Ionosphere Dynamics Inferred From Topside Sounding341
  • Part IX: Summary Session347
  • Chapter 40. Does Space Weather Really Matter on the Ground?349
  • Author Index359
Book details
  • Vendor Elsevier S & T
  • SKU 9780080440576
  • ISBN-13 9780080541518
  • Author Lyu, L.-H.
  • Category Technology & Engineering
  • Subject Aeronautics & Astronautics

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Magnetic storms may cause damage to satellites, radiation hazard to astronauts, disruption of radio communications, and interruption of ground electric power lines. Space weather prediction becomes an important issue to be addressed in the twenty-first century. International Solar Terrestrial Program (ISTP) employs five satellites to probe the solar wind and magnetosphere, providing valuable information for space weather prediction. The Asia-Pacific region is becoming one of the economic centers in the world. The continuous drive for scientific and technological progress in parallel is evidenced by the establishment of many space research organizations in many countries of this area. In Taiwan, the National Space Program Office (NSPO) established her third satellite program -- COSMIC (Constellation Obsering Systems for Meteorology, Ionosphere and Climate), which is a science experiment to demonstrate the utility of atmospheric radio limb soundings from a constellation of six low-earth orbiting satellites in operational weather prediction, space weather monitoring, and climate monitoring and research.
In order to provide a forum to discuss the many new results in this rapid-moving field and to forge international collaborations, a three-day COSPAR Colloquium on "Space Weather Study Using Multipoint Techniques" was held. This colloquium have provided a forum for experts from the international community to present new results on the timely topic "space weather".