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Next: Contents

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• Contents
• Introduction
  • Summary of Science Objectives
  • Diagnostics
• Instrument Overview
  • Telescope Assembly
  • Spectrometer Assembly
    • Detectors
    • On-Board Image Processing
  • Sun Sensor
  • Wavelength Coverage
  • Flight Software
• Intensities and Count Rates
  • Introduction
  • Estimates of Line Intensities in Coronal Holes
    • Spectral line intensities
    • Assumed Solar Wind Plasma Parameters
    • Calculated Line Intensities
    • Measured HI Ly-a Intensities in Coronal Holes
  • Measured HI Ly- intensities and estimated OVI intensities in coronal streamers
  • Relationships between ultraviolet intensity and count rate
• UVCS Operations
  • Introduction
  • Operations Management and Staffing
    • Overview
    • Instrument Operation Team
    • Mission Planning Team
    • Data Processing Team
    • Instrument/Calibration Team
    • Engineering Team
  • Workstations
• Instrument Operation Modes
  • Description of Operations
  • Observation Sequences
    • Coronal Observation 1
    • Coronal Observation 2
    • Coronal Observation 3
    • Coronal Observation 4
    • Coronal Observation 5
    • Coronal Observation 6
    • Synoptic Observation
    • Offset-Pointing Observation
    • Stellar Observation
    • Disk Observation 1
    • Disk Observation 2
• Data Processing and Analysis Software
  • Data Products
  • Data Analysis Software
  • Database Software
  • Analysis Tools
• Observation Programs
  • Observational Goals for the UVCS
    • Diagnostic Tools
    • Physical Description of Various Coronal Structures
    • Physical processes
    • Instrument Oriented Objectives
    • Coordinated Observations
    • Stellar Observations
    • Solar System Observations
  • Examples of UVCS Observations
    • Doppler Dimming Determination of Coronal Outflow Velocities
    • Electron Coronal Density Irregularity

      from Measurements of K-Coronal and Lyman Lines Brightnesses

    • Small-Scale Temporal Variability in the Corona
    • Modeling the Three-Dimensional Solar Corona from White Light Data
    • The Temperature Gradient in Coronal Holes
    • Studies of Fine Scale Structures in Coronal Holes -- Polar Plumes
    • Modeling the Solar Wind in Coronal Holes
    • Modeling the Solar Wind in Quiet Regions
    • Solar Wind Properties as a Function of Bright Points Characteristics
    • Dynamics of Protons and Heavy Ions in Solar Wind Acceleration Regions
    • Stationary Coronal Streamers and Cusps
    • Coronal Transients in UV Spectral Lines
    • Observations of Plasmoids in the Solar Corona
    • Study of UV Line Emission from Coronal Millimetre Wave Sources (CMMs)
    • Abundances of Elements in the Outer Corona
    • Alfven Wave Acceleration of the Solar Wind
    • Study of Magnetic Reconnection Processes in the Extended Solar Corona
    • High Temperature Gas Above Flares and Surges
    • Contribution of ARs to the solar wind mass and energy flux.
    • Physics of Shock Waves
    • Rotation of the Extended Solar Corona
    • Energy Transport by Suprathermal Electrons
    • Intensity Calibration of the WLC
    • Instrument Calibration with Stellar Observations
    • Optical Signatures Related to Solar Radio Events
    • Coordinated Observations with UVCS and LASCO
    • Stellar Observations with UVCS
    • UV Observations of the F-Corona
    • Observations of Transits of the Inner Planets within the Field of View of UVCS
  • Ground-based Observations in support of the UVCS science
• Recommended Atomic Data
• Data Access and Publication Rights
  • Data Product Availability
  • Data Distribution
    • Catalog Retrieval and Distribution
    • Data Retrieval and Distribution
    • Support for Co-Investigator and Guest Investigator Processing
    • Export Data Formats and Media
  • Data Rights, Access and Publication Policy
• Instrument Characterization
• References
• Appendix
  • UVCS Team
  • General References for UVCS
  • List of Acronyms
• About this document ...

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