
Solar Terrestrial Dispatch is a world-leader in space weather
forecasting services, as was demonstrated in late October and early November
2003 (Oler, C., "Prediction Performance of Space Weather Forecast
Centers during the Extreme Space Weather Events of October and November 2003,"
published in the peer-reviewed scientific journal "Space
Weather" by the American Geophysical
Union in 2004). A copy of this paper is
available here.
Our expertise is used to provide high-quality space weather
forecast services to many electrical power companies across North America,
guidance to spacecraft operators and consultation to many others.
We have developed a special space weather course designed to
teach individuals without any background how to predict space weather (see
below). Our course was the recipient of the Study-Web Academic Excellence
award.
The course is available on-line as a small group of downloadable
Adobe Acrobat Reader documents comprising over 630 pages of printed material
(for sample pages, click here). You can therefore
choose to study the material on your computer or print it out for study. The
course also includes our workhorse space weather information monitor (SWIM)
software, which is the most comprehensive space and weather information monitor
in the world. The course also includes a copy of our Aurora
Monitor software package, as well as our popular Proplab-Pro
HF Radio Propagation Laboratory software. All software products are optional
elaborate tools that will contribute to your application of the knowledge
obtained through this course.
A list of the topics covered in this home-study course include:
- The Sun
- Basics of the Sun
- Sunspots
- Types of Sunspots
- Sunspot Magnetic Fields
- Solar Radiation and Radio Emissions
- Solar Cycles
- Techniques for Modelling Solar Cycles
- Sources of Information and Imagery
- Interplanetary Space
- The Solar Wind
- Magnetic Fields
- Heliospheric Current Sheet
- Solar Sector Structures
- The Earth
- Magnetosphere
- The quiet magnetosphere
- The disturbed magnetosphere
- Understanding Magnetic Indices
- Magnetic Storms
- Sudden Storm Commencements (SSCs)
- Gradual Storm Commencements
- Geomagnetically Induced Currents
(GICs)
- Effects on Electrical Hydro
Systems
- Effects on Other Long Conductors
- Ionosphere
- Formation of Ionospheric Layers
- Factors Affecting Ionospheric Layers
- Solar Disturbances
- Transient Solar Coronal Mass Ejections
(CMEs)
- Types and Structures of Coronal
Mass Ejections
- Understanding the Importance of
CME Structures
- Inferring CME Structures from Available
Solar Data
- Coronal Mass Ejection Detection
Methods
- Using IMPACT (software) to Aid in
CME Disturbance Predictions
- Solar Cycle Dependencies
- Solar Flares
- Basic Nature of Flares
- Types of Flares
- Flare Rating Systems
- Significance of Proton Flares
- Ground Level Events (GLEs)
- Fast Transit Events
- Interpreting Magnetograms
- Determining Magnetic Shear and Flare
Susceptability
- Solar Flare (and Proton Flare) Prediction
Techniques
- Solar Flare Related Coronal Mass
Ejection Prediction Techniques
- Sources of Solar Flare Information
- Solar Coronal Holes
- Coronal Hole Basics
- Recurrence
- Solar Cycle Correlations
- Associations with Near-Relativistic
Electrons
- Coronal Hole Related Disturbance
Prediction Techniques
- Filament Eruptions
- Filaments and Prominences
- Eruptive and Non-Eruptive Activity
- Filament-Associated Coronal Mass
Ejections
- Filament-Related Disturbance Prediction
Techniques
- Auroral Activity
- Basic Theory of the Northern/Southern
Lights
- Behavioral Characteristics of the Auroral
Ovals
- Sensitivity to Solar Disturbances
- Affects on Satellite Health and Radio
Communications
- Mathematical Models of the Auroral Zones
- Auroral Activity Prediction Techniques
- Information Sources
- Conditions Affecting Satellite Health
- Atmospheric Drag
- Surface Charging Anomalies
- Deep Dialectric Charging Anomalies
- Interplanetary Shocks
- Magnetopause Crossings
- Postulated Sun/Earth Climate Connections
- Possible Long-Term Climatic Trends
- Rainfall
- Temperatures
- Atmospheric Pressure
- Storm Tracks
- Ozone Correlations
- Possible Short-Term Meteorological Trends
- Pressure and Winds
- Lightning
- Storm Systems
- Ozone Responses
- Radio Propagation
- Basic Theory (Non-Technical)
- Characteristics and Components of
Radio Signals
- Understanding Plasmas
- Importance of Electron Collisions
- Appleton/Hartree Contributions
- Signal Polarization and Coupling
- Ionospheric Absorption
- Deviative Absorption
- Non-Deviative Absorption
- Fading
- Multipathing
- Travelling Ionospheric Disturbances
- Solar Related Disturbances
- Structure of the Ionosphere
- Ionospheric Layers
- Importance of Sporadic-E
- Effects of Spread-F
- Solar-Cycle Dependencies
- Models of the Ionosphere
- Simple Mathematical Models
- Numerical Maps
- CCIR
- URSI
- The International Reference
Ionosphere (IRI)
- Others
- Probing the Ionosphere
- Probing Techniques
- Probing Instruments
- Sources of Ionosonde Information
- Basic Ray-Tracing Concepts
- Ordinary vs Extraordinary Signals
- Becoming Familiar with Ray-Tracing
Software
- Ray-Tracing in Three-Dimensions
- Ray-Tracing Software Considerations
- Preparing for 3D Ray-Tracings
- Performing 3D Ray-Tracings
- Studying 3D Ray-Tracing Results
- Vertical Radio Signal Propagation
- Signal Reflection Behavior
- Critical Frequencies
- Ray-Tracing Vertically-Incident
Signals
- Oblique Radio Signal Propagation
- Signal Refraction/Reflection Characteristics
- Effects of Geomagnetic Activity
- Effects of Solar Activity
- Ray-Tracing Obliquely Incident Radio
Signals
- Determination of Maximum Usable
Frequencies
- Simple Empirical Methods
- Ray-Tracing Techniques
- Effects of Sporadic-E
- Non-Great-Circle (NGC) Propagation
- Responsible Conditions
- Compensation Methods
- Ray-Tracing Techniques to Analyze
NGC Propagation
- Chordal-Hop and Inter-Layer Ducting
Propagation
- Advantages and Disadvantages
- Analysis using Ray-Tracing Techniques
- Searching for and Exploiting Exotic
Propagation Paths
- Properties of Exotic Paths
- Searching for Exotic Paths using
3D Ray-Tracing Techniques
- Determining the Most Reliable
Exotic Radio Paths
- Ionospheric Disturbances
- Solar Related Disturbances
- Solar Flares and Related Coronal
Mass Ejections
- Coronal Holes and High Speed
Solar Wind Streams
- Filament Related Coronal Mass
Ejections
- Impact of Flare Related Radio
Noise Bursts
- Short Wave Fadeouts
- Sudden Phase Anomalies
- Sudden Frequency Deviations
- Devastating Effects of Polar Cap
Absorption
- Disturbances and their Effects on
Satellite Communications
- Radio Propagation Prediction Methods
- Short-Term Forecasting Techniques
- Medium-Term Forecasting Techniques
- Long-Term Forecasting Techniques
- Sources of Forecasting Information
- Applied Forecasting Techniques
- Climatology
- Pattern Recognition
- Compiling Necessary Information
- Exploiting Databases
- Computer Related Aids
- Studying Real-Life Examples
- Developing Experience and "Intuition"
- Field Experience
- We present you with some specific historic
real-life scenarios. Using the information and techniques studied in this
course, you are asked to develop your own space-weather and radio-propagation
predictions. The actual real-life impacts are then studied and compared
with your forecasts.
- We present you with several hypothetical
(possible future) examples and ask you to develop your own forecasts.
- Course Completed
Although this course is largely self-taught, we will provide support if you
run into difficulties. There are no prerequisites.
The course is available on-line for immediate purchase by following the instructions
below. It may also be purchased by FAXing us the payment
form.
Purchasing the Course
Please choose one of the following course packages.
- The course alone (no software), delivered over the Internet.
- Price: $250 USD
- Pay Online by clicking the PayPal button:
- The course with all software, delivered over the Internet.
- Price: $300 USD
- Pay Online by clicking the PayPal button:
- The course with all software, delivered on CDROM.
- Price: $350 USD
- Pay Online by clicking the PayPal button:
Note: All software requires Windows-based platforms. SWIM
requires Windows XP, 2000 or NT4. The STD Aurora
Monitor software can be used in place of SWIM for those who are running
Windows 95, 98 or Me. Proplab-Pro requires Windows 95, 98, NT4, 2000 or XP (non-laptop).