PhD thesis - Institute for Space Research - University of Calgary

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164 C: Attitude Solution Figure C.2: Same as Figure C.1 but for the Y components. Figure C.3: Same as Figure C.1 but for the Z components (spin-axis, parallel to B 0. The science magnetometer data and model fit have both have a quadratic subtracted to make the differences easier to see.
165 Figure C.4: (top) Angular separation between perpendicular components of model and observed magnetic field vectors. (Perpendicular means perpendicular to the spin axis). This is an indication of the spin-phase error. (bottom) Total angular error between model and observed magnetic field vectors.
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THE UNIVERSITY OF CALGARY High-reso
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Abstract Low-energy (E k ∼ 10 −
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gave practical advice on how to coa
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3 The Suprathermal Ion Imager 27 3.
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List of Tables 3.1 Whalen analyzer
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4.7 GOES 10 H P magnetic field at g
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List of Acronyms 2-D two dimensiona
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List of Symbols ◦ degree ‖ para
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V f V P V S ε ϑ v v v d v r v th
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Chapter 1 Introduction The main obj
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Chapter 2 Background 2.1 The aurora
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2.2.1: The ionosphere 5 Figure 2.2:
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2.3: Basic concepts of charged-part
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2.3.1: Charged-particle acceleratio
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2.4: In-situ observations of partic
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2.5: Ion heating by plasma waves 13
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2.5.3: Alfvén waves 15 interact wi
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2.6: Velocity distributions 17 ∫
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2.7: Overview of plasma diagnostic
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2.7: Overview of plasma diagnostic
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2.8: Space and time ambiguities 23
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2.9: Objectives of this thesis 25 d
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28 3: The Suprathermal Ion Imager (
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30 3: The Suprathermal Ion Imager t
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32 3: The Suprathermal Ion Imager
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34 3: The Suprathermal Ion Imager a
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36 3: The Suprathermal Ion Imager F
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40 3: The Suprathermal Ion Imager e
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42 3: The Suprathermal Ion Imager P
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44 3: The Suprathermal Ion Imager O
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48 3: The Suprathermal Ion Imager t
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50 3: The Suprathermal Ion Imager 3
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58 3: The Suprathermal Ion Imager S
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Chapter 4 The GEODESIC mission The
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4.1: Flight overview 63 ter provide
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4.1: Flight overview 65 Figure 4.3:
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4.1: Flight overview 67 spheric foo
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4.2: The solar wind 69 localized tr
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4.3: The magnetotail 71 period of s
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4.5: The ground-level magnetic fiel
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4.5: The ground-level magnetic fiel
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Chapter 5 Results from the Suprathe
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5.1: General ion distribution prope
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5.1: General ion distribution prope
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5.1.1: Payload floating potential 8
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5.1.1: Payload floating potential 8
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5.1.2: Comparisons between model an
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5.1.3: Automated estimates of bulk
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5.1.4: Comparison between v i and E
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5.1.5: Bulk ion drift parallel to B
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5.1.6: Polarization drift 99 (a) (b
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5.1.7: Automated estimates of mean
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5.2: Core ion interactions with pla
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5.2.2: Alfvén waves 105 curve in F
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5.2.2: Alfvén waves 107 Figure 5.2
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5.2.3: Lower-Hybrid Solitary Struct
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5.2.3: Lower-Hybrid Solitary Struct
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Page 146 and 147: 120 6: Discussion perturbations δB
Page 148 and 149: 122 6: Discussion pling scale of
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Page 152 and 153: 126 6: Discussion will be Doppler-s
Page 154 and 155: 128 7: Conclusions and suggestions
Page 160 and 161: 134 Bibliography Carlson, C. W., an
Page 162 and 163: 136 Bibliography auroral arc by Aur
Page 164 and 165: 138 Bibliography Lund, E. J., E. Mo
Page 166 and 167: 140 Bibliography Pietrowski, D., K.
Page 168 and 169: 142 Bibliography Wahlund, J., A. I.
Page 170 and 171: 144 A: Modeling ion distributions E
Page 172 and 173: 146 A: Modeling ion distributions T
Page 174 and 175: 148 A: Modeling ion distributions F
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Page 178 and 179: 152 A: Modeling ion distributions p
Page 180 and 181: 154 A: Modeling ion distributions w
Page 183 and 184: Appendix B Uncertainties in velocit
Page 185: B.2: Forward-modeled velocity momen
Page 188 and 189: 162 C: Attitude Solution plane defi
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PhD thesis - Institute for Space Research - University of Calgary

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