Neutral-atom Astronomy: Plasma Diagnostics From The Aurora To The Interstellar Medium

Contents
Preface
List of Tables
List of Figures
List of Acronyms
Symbols and Units for Useful Quantities
Chapter 1. Introduction
	1.1. Members of the Cast
	1.2. Earth’s Magnetosphere
		1.2.1. Earth’s exosphere
	1.3. The Heliosphere
		1.3.1. The interstellar neutral-atom flow in the heliosphere
		1.3.2. Global view of the heliospheric boundary with ENAs
	References
Chapter 2. First Encounters with ENAs
	2.1. The Discovery: From the Telescope to the Accelerator
	2.2. First Diagnostic Use of ENAs in Space
	2.3. Invoking ENAs to Explain New Satellite Observations
	2.4. First ENA Images from Space
	References
Chapter 3. Remote Sensing of Space Plasma Through ENA Observations
	3.1. ENA “Imaging”: Determination of the Spatial, Energy & Elemental Distributions of Remote Ion Populations
	3.2. Ion Distribution Functions and Plasma Processes
		3.2.1. Velocity distributions in thermal equilibrium
		3.2.2. Non-thermal velocity distributions
		3.2.3. Moving distributions and frame transformations
	3.3. Relation Between the Observed ENA Flux and the Remote Ion Distribution
	3.4. Propagation of ENAs and Observational Limits
		3.4.1. ENA trajectories in gravitational fields
		3.4.2. Extinction of ENAs from the source to the observer
		3.4.3. Effects of elastic collisions on the ENA diagnostics
		3.4.4. PUIs as inevitable companions of ENAs
	3.5. Summary
	References
Chapter 4. ENA Instrumentation: General
	4.1. Choosing Vantage Points for ENA Observations
		4.1.1. Viewing the heliosphere: SOHO and IBEX
		4.1.2. Viewing Earth’s magnetosphere: IMAGE and TWINS
	4.2. General Considerations for Space-Borne Particle Instruments
		4.2.1. Particle selection by analyzers
		4.2.2. Particle detectors
			4.2.2.1. Electron multipliers
			4.2.2.2. Solid-state detectors
		4.2.3. Principles of TOF measurements
			4.2.3.1. Combination of TOF and SSD measurements
			4.2.3.2. Combination of TOF and ESA measurements
			4.2.3.3. Intrinsic noise-suppression capability of TOF sensors
			4.2.3.4. TOF spectrographs for neutral atoms
		4.3. ENA-Specific Observational Challenges
			4.3.1. Suppression of charged particles
			4.3.2. Attenuation of EUV
			4.3.3. Conversion of ENAs into ions before their analysis
				4.3.3.1. Conversion of ENAs to positive ions
				4.3.3.2. Conversion of low-energy ENAs or ANAs to negative ions
	References
Chapter 5. ENA Sensor Implementations
	5.1. The Road to ENA Instrumentation
		5.1.1. Common root: two non-ENA instruments of relevance
		5.1.2. First ENA instrument in space
	5.2. Non-TOF ENA Sensors
		5.2.1. The first ANA instrument: GAS on Ulysses
		5.2.2. ENA sensors with MCP single-pulse detection
		5.2.3. ENA sensors with SSD single-pulse detection
	5.3. ENA Spectrographs with TOF Measurement
		5.3.1. ENA cameras for the 10–200 keV range
		5.3.2. ENA cameras for the 0.3–20 keV range
		5.3.3. Neutral atom cameras for the 5–2000 eV range
	References
Chapter 6. ENAs from Magnetospheres and Small Bodies in the Solar System
	6.1. Earth’s Magnetosphere
		6.1.1. The outer magnetosphere
			6.1.1.1. The magnetosheath
			6.1.1.2. The polar cusp
			6.1.1.3. The magnetotail
		6.1.2. The inner magnetosphere
			6.1.2.1. ENA images and their intrinsic challenges
			6.1.2.2. Deconvolution of ENA images
	6.2. Magnetospheres and Ionospheres of Other Planets
		6.2.1. Jupiter and Saturn
			6.2.1.1. Jupiter seen in ENA images
			6.2.1.2. Saturn seen in ENA images
		6.2.2. SW-induced magnetospheres
			6.2.2.1. ENAs at Mars
			6.2.2.2. ENAs at Venus
		6.2.3. Mercury
	6.3. Small Bodies in the Solar System
		6.3.1. ENAs from the Moon
		6.3.2. Smaller bodies and dust
	References
Chapter 7. ENA Diagnostics of the Heliosphere-Interstellar Medium Interaction
	7.1. Getting Acquainted with the Heliosphere
	7.2. Interstellar Neutral Wind through the Heliosphere
		7.2.1. Overview of in-situ diagnostic methods
		7.2.2. Connecting ISN flow observations with the ISM
		7.2.3. Observational challenges and opportunities for the ISN flow
	7.3. The ENA Ribbon, a “Compass” for the Interstellar Magnetic Field
		7.3.1. Ribbon overview
		7.3.2. The Secondary-ENA model as likely explanation
			7.3.2.1. Simplified analytical model
			7.3.2.2. Tests of the Secondary-ENA model
		7.3.3. Challenges and opportunities with the ENA Ribbon
			7.3.3.1. Effectiveness of Ribbon generation and turbulence
			7.3.3.2. Determination of the interstellar magnetic field
			7.3.3.3. Reach of the Solar Wind into the ISM
	7.4. Secondary Interstellar Neutrals
		7.4.1. Extraction of secondary interstellar neutrals
		7.4.2. Challenges and opportunities with secondary interstellar neutrals
	7.5. Globally Distributed ENAs
		7.5.1. Extraction of the globally distributed ENAs
		7.5.2. Challenges and opportunities with the GDF of ENAs
	References
Chapter 8. What Have ENAs Revealed and What is Next?
	8.1. Understanding the Cross-Scale Coupling of the Magnetospheric Systems
	8.2. Surveying Exposed Surfaces in the Solar System: Planets to Dust
	8.3. Understanding the Sun-ISM Interactions and Particle Acceleration on Large Scales
	8.4. Bridging the Temporal and Spatial Divide
	References
Appendix A. Geometrical Factor and Angular Response
	A.1. Geometrical Factor
	A.2. Angular Response
		A.2.1. Example of a calibrated angular response
		A.2.2. Ignoring the angular response, a potential problem
	References
Appendix B. ENA-Beam Calibration Facilities
	B.1. Requirements and General Principles of Operation
		B.1.1. Neutral-atom beams through physical contact
		B.1.2. Neutral-atom beams through photo detachment
		B.1.3. Comparison of different schemes
	References
Index