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STEREO 3D

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X-ray Conditions (Flares) 5-min.

X-ray plot

X-ray Conditions (Flares) 1-min.

X-ray plot

Geomagnetic Conditions (Kp)

plot of Kp

Satellite Environment Plot:


Satellite Environment Plot





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Warnings/Alerts issued
in the last 24 hours, if any:

(Key: NOAA Scales)

Warning (1929): Geomagnetic K-index of 4 expected From: 2012 May 16 2310 UTC To: 2012 May 17 0600 UTC Condition: Onset Alert (1578): Geomagnetic K-index of 4 Period: 2100-2400 UTC Threshold Reached on 2012 May 16 2313 UTC


[ live aurora display ]
[ auroral power maps ]

[ d-layer conditions ]

[ latest solar images 1 ]
[ latest solar images 2 ]
[ latest solar images 3 ]

[ active solar regions ]
[ current solar region image ]

[ What is a flare and its class? ]

Recent Space Environment Reports:

+ Reports of Solar & Geophysical Activity
+ Solar & Geophysical Activity Summaries

From the Space Environment Center:

Solar X-ray Flux

+ A 3 day plot of 5-minute solar X-ray flux values measured on the GOES 8 and 10 satellites.
+ A 6-hour 1-min Solar X-ray Flux plot

Satellite Environment Plot

[ Proton Flux ] [Electron Flux ]
[ GEOS Hp ] [ Estimated Kp ]

Additional Resources

+ SpaceW.com Aurora Network
+ D-Layer Absorption Conditions/Predictions
+ 160 Meter Propagation Forecast
+ Solar Physics Department of the Royal Observatory of Belgium, the official keepers of sunspot data.




Solar Activity Forecast
The Forecast of Solar Activity as well as Geomagnetic Activity

Probability of Flares
and Proton Events
EVENT
(Flare/Proton)
0-24 hrs
24-48 hrs
M-class
10%
10%
X-class
01%
01%
Proton
01%
01%
Geomagnetic Activity Probabilities

Middle latitudes
High latitudes

0-24 hrs
24-48 hrs
0-24 hrs
24-48 hrs
Active
01%
01%
01%
01%
Minor Storm
01%
01%
01%
01%
Major-severe Storm
01%
01%
01%
01%



Solar Sunspot Cycle 24 Progress

Solar Cycle 24 Smoothed Sunspot Progress
Solar Cycle 24 10.7-cm Monthly Progress
[ Solar Cycle Details ]

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This page was rendered on 17-May-12 0235 UTC.
This page was first created in 1998.

Current Sunspot Cycle 24 Activity and Space Weather

Sun Spots: 125 as of 05/15/2012 :: 10.7-cm Flux: 131 SFU
(SFU=Solar Flux Units)

NOAA Scales Activity
Range 1 (minor) to 5 (extreme)
NOAA Scale
Past 24 hrs
Current


Planetary A-index (Ap): 9 | Planetary K-index (Kp): 4
Solar Wind: 371 km/s at 3.0 protons/cm3, Bz is -3.0 nT
(May 17, 2012 at 0044 UT)

X-ray Solar Flares:
6h hi [C2.5][0910Z 05/16] 24h hi [C2.5][0910Z 05/16]

Background X-ray Level, Last Six Days

May 15 2012 :: B4.9
May 14 2012 :: B4.3
May 13 2012 :: B4.2
May 12 2012 :: B4.9
May 11 2012 :: B6.1
May 10 2012 :: B6.5




Kp maps of midnight equatorward boundaries

There are maps for four quadrants of the globe:
+ North America,
+ Eurasia,
+ South America and Eastern Pacific, and,
+ Africa-Indian Ocean-Australasia.

The average equatorward boundary of the midnight aurora is shown for levels of magnetic activity ranging from relatively low, Kp=3, to very high, Kp=9. Clicking on the map at that location will give the approximate magnetic latitude for that location. (Keep in mind that aurora can still be viewed when it is positioned 4-5 degrees in latitude away from the viewer although it will appear about 20 degrees above the horizon.) These maps were created using satellite observations to determine the average equatorward boundary of the aurora as a function of the Kp index (see above). Using those data, the typical maximum extent of the aurora toward the equator for the hours around midnight for four levels of geomagnetic activity is displayed.


Space Weather and Geomagnetic Conditions
131
131
Global HF Propagation Conditions
Global HF Propagation Conditions for 0200Z on 17 May, 2012
High Latitude: Fair-Normal
Middle Latitude: Normal
Low Latitude: Normal

Geomagnetic Latitude Ranges:
High: 60-90 degrees
Middle: 20-60 degrees
Low: 0-20 degrees


Good news:The Provisional International monthly mean Sunspot Number for October 2011 is 88.0 (eighty-eight point zero), up from September's 78.0 (seventy-eight point zero). That's the highest so far in the new sunspot cycle, Cycle 24. Numbers, starting with August 2009: 0.0, 4.3, 4.8, 4.1, 10.8, 13.2, 18.8, 15.4, 8.0, 8.7, 13.6, 16.1, 19.6, 25.2, 23.5, 21.5, 14.4, 18.8, 29.6, 55.8, 54.4, 41.6, 37.0, 43.9, 50.6, 78.0, and now, 88.0.

Here is a chart that compares Sunspot Cycle 23 with Sunspot Cycle 24. It seems, actually, that Sunspot Cycle 24 is not too different than Cycle 23, in comparison of growth and progression.

Comparison of Sunspot Cycle 23 with Cycle 24; smoothed monthly sunspot numbers

At 0805 UTC, on 9 August 2011, a strong magnitude X6.9 X-ray flare erupted on the northwestern solar limb. Here is a HD Movie of the event:



Videos of Interest - Space Weather, Solar Dynamics Observatory, STEREO, and more... from the NW7US YouTube Channel. (Click on the small image to launch the video...)

Video: Voyager Finds Magnetic Foam at Solar Systems Edge
Video: Voyager Finds Magnetic Foam at Solar Systems Edge

Video: The First 360 View of Our Sun - NASA STEREO
Video: The First 360 View of Our Sun - NASA STEREO

Video: Solar Dynamics Observatory - Overview
Video: Solar Dynamics Observatory - An Overview

Video: A New Look Inside the Sun (SDO HMI)
Video: A New Look Inside the Sun (SDO HMI)

Video: The Extreme Ultraviolet Variability Experiment (EVE)
Video: The Extreme Ultraviolet Variability Experiment (EVE)

Video: The Atmospheric Imaging Assembly (AIA)
Video: The Atmospheric Imaging Assembly (AIA)



Video: Fantastic Aurora: Inside the Sun to Earth's Poles
Video: Fantastic Aurora: Inside the Sun to Earth's Poles

Video: Hearing the Northern Lights!
Video: Hearing the Northern Lights!



Video: Zoom View of Prominence Eruption and X-Ray Flare - M2.5 Magnitude - June 7 2011
Video: Zoom View of Prominence Eruption and X-Ray Flare - M2.5 Magnitude - June 7 2011

Video: X-Ray Flare, Coronal Mass Ejection, Proton Storm - M2.5 Magnitude - June 7 2011
Video: X-Ray Flare, Coronal Mass Ejection, Proton Storm - M2.5 Magnitude - June 7 2011 (Close-up of the video, above)

Video: Stunning Close-up View of M3 X-Ray Flare 24 February 2011
Video: Stunning Close-up View of M3 X-Ray Flare 24 February 2011



Video: June 2011 20-meter (14-Mhz) JT65A Coverage Map of NW7US Radio Signal
Video: June 2011 20-meter (14-Mhz) JT65A Coverage Map of NW7US Radio Signal



The Solar Dynamics Observatory (SDO) Latest Solar Images
Click on an image for full-sized view





SDO - Solar Dynamics Observatory     SDO - Solar Dynamics Observatory

D Region Absorption Predictions (D-RAP) Global Map

Map, Above: Conditions in the D region of the ionosphere have a dramatic effect on high frequency (HF) communications and low frequency (LF) navigation systems. The global D Region Absorption Predictions (D-RAP) depicts the D region at high latitudes where it is driven by particles as well as low latitudes, where photons cause the prompt changes.

Note: At times, images may appear broken or missing, when SDO is working on the AIA/HMI instruments.


The NW7US Current Sunspot and Geophysical Activity Report
The observations, prognastications, and comments by NW7US
NW7US is Tomas David Hood, Propagation and Space Weather Columnist
for CQ Communications

More about Background X-rays

The hard X-ray energy present from the wavelengths of 1 to 8 Angstroms provide the most effective ionizing energy throughout all of the ionospheric layers in our atmosphere. The GEOS satellites measure these wavelengths and the resulting measurements are reported as the "background X-ray level" throughout the day. A daily average is reported, as well.

Just like X-ray flares, the background hard X-ray level is measured in watts per square meter (W/m2), reported using the categories, A, B, C, M, and X. These letters are multipliers; each class has a peak flux ten times greater than the preceding one. Within a class there is a linear scale from 1 to 9.

If one records the daily background X-ray levels for the course of a sunspot cycle, one would discover that the background X-ray levels remained at the A class level during the sunspot cycle minumum. During the rise and fall of a solar cycle, the background X-ray energy levels remained mostly in the B range. During peak solar cycle periods, the background energy reached the C and sometimes even M levels.

Armed with this information, can we discover any clues as to the current status of Sunspot Cycle 24? Below is a graph plotting the background hard X-ray energy reported by the GEOS satellites since the end of Sunspot Cycle 22. Clearly, we see a noticeable rise in Cycle 24 activity. We're seeing the energy mostly in the B level more often, supporting the view that Cycle 24 is alive and moving along toward an eventual sunspot cycle peak in several years.

Overall, the monthly average background 'hard' X-ray level is rising (as seen by the following plot), showing a change from deep solar cycle minimum. We are certainly in the rising phase of Sunspot Cycle 24. While it has been a slow up-tick over the last eighteen months, I expect to see a more rapid rise during mid to late 2011.

Background X-ray (1 to 8 Angstrom) Plot



Highlights of Solar and Geomagnetic Activity
Covering the period: 07 - 13 May 2012

Solar activity ranged from low to moderate levels. Region 1476 (N10, L=180, class/area=Fkc/1050 on 09 May) was responsible for almost all x-ray flare activity during the week. It produced a total of 55 C-class flares, 6 M-class flares, and 69 optical flares. Region 1476 began the week as an Fkc type group with a beta-gamma magnetic configuration. By the 8th, it had grown in extent (17 degrees), spot count (35), and complexity (beta-gamma-delta) and produced an M1/1F flare at 1308 UTC. It reached its maximum areal coverage of 1050 millionths on the 9th when it produced an M4/1n at 1232 UTC, an M1/1b at 1408 UTC, and another M4 at 2105 UTC. The maximum extent and spot count (20 degrees, 50 spots) followed on the 10th when Region 1476 produced the largest of the flares, an M5/2b at 0418 UTC. The flare was accompanied by a three minute 10cm burst (690 sfu) at 10/0417 UTC and a Type IV emission at 10/0402 UTC, followed by a weak earth-directed Coronal Mass Ejection (CME). Later that day, Region 1476 produced an M1 at 2026 UTC, the last M-class event of the week. The region then began a slow but steady decline in areal coverage, longitudinal extent and spot count, although it sustained its beta-gamma-delta magnetic configuration.

Earlier in the week, the only M-class event not produced by Region 1476 was an M1/1n flare observed from Region 1471 (S21, L=276, class/area=Eho/320 on 02 May) at 07/1431 UTC. This flare was also accompanied by a 10cm burst (230 sfu) at 10/1415 UTC and a Type IV emission at 07/1409 UTC. STEREO-Ahead imagery suggested an earth-directed CME. The following day, two more potentially earth-directed, weak CMEs were observed in STEREO-A COR2 imagery.

Region 1477 (S24, L=140, class/area Dso/150 on 09 May) was split to form new Region 1478 (S24, L=135, class/area=Hsx/090 on 10 May) on 10 May. Similarly, Region 1479 (N15, L=105, class/area Dso/130 on 12 May) was split to form new Region 1482 (N14, L=100, class/area=Dso/080 on 13 May). Both of these divisions resulted from careful analysis of magnetogram data. After the split, Region 1477 became an Hsx type group with L=144, and Region 1479 became an Hxs type group near L=109.

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was at high levels on the 10th through the 13th, and at moderate levels for the remainder.

Geomagnetic field activity ranged from quiet to active conditions with minor to major storm periods observed at high latitudes. The week began with quiet conditions on 7th and the majority of the 8th. Around 08/0400 UTC, a solar sector boundary crossing from positive to negative was observed at the ACE spacecraft. By midday, the solar wind speed at ACE began to rise, marking the arrival of a coronal hole high speed stream (CH-HSS). Significant southward Bz began around 1730 UTC and reached a minimum of -13 nT late on the 8th before beginning a gradual return to neutral conditions late on the 10th. The geomagnetic field responded with active conditions from the last synoptic period on the 8th through the 9th. Minor to major storm levels were observed at high latitudes on the 9th. Activity subsided to mostly unsettled levels on the 10th, followed by mostly quiet conditions on the 11-12 May. The solar wind speed at ACE remained above 500 km/s until around 13/0000 UTC. Conditions were mostly unsettled on the 13th. Although there were a number of CMEs identified as potentially earth-directed, there was no definitive indication of CME arrival reflected in the ACE data suggesting the transient signatures were obliterated in the high speed stream.



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Where are we in the new cycle, Sunspot Cycle 24?

As you can see in the following plots of Sunspot Cycle 23 (the previous sunspot cycle), the last cycle (like any sunspot cycle, often has wide swings in sunspot counts from one month to the next. It is not unusual to see what we're now seeing; it seems typical in every sunspot cycle to see such wide swings up and then back down in the number of observed sunspots. This monthly variation is seen during this new cycle, Sunspot Cycle 24. Also note that Cycle 24 is not very different from Cycle 23.

(Click for full-size)

Cycle 23 Monthly Plot by NW7US shows wide variations
Cycle 23 and 24 Monthly Plots - start of each cycle - by NW7US shows wide variations





View of numbered sunspot regions and plages (if any)
Source: http://www.solarmonitor.org/.
(Click for large view)

Active Regions and Plages

Active sunspot regions, and plages, identified by SIDC

SIDC Solar Disc with active regions and plages


Latest GOES 15 Image of the Sun

Latest GOES-15 Image of the Sun


STEREO IMAGES
STEREO Behind Image
What is coming
SOHO EIT 195 Image
Current View
STEREO Ahead Image
What was...


Real Time Solor Wind and Aurora:

On 2012 May 17 0228Z: Bz: N/A nT
Bx: N/A nT | By: N/A nT | Total: N/A nT
Most recent satellite polar pass:
Centered on 05/16/2012 : 2256 UTC
Aurora Activity Level was 8 at 2256 UTC
visit noaa for latest.



[ See this current Aurora Oval Map ]

This is a video of the simulation from May 27-28, 2011, showing
the Geomagnetic disturbance caused by the solar wind




All NICT images are Copyright@NICT,
used by express, written permission from NICT




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Space Weather and Propagation Forecast
Prepared by the US Dept. of Commerce, NOAA,
and the Space Weather Prediction Center

Three Day Forecast of Solar and Geomagnetic Activity
(as of 2200Z on 16 May 2012)

Solar Forecast:

Solar activity is expected to be very low to low for the next 3 days (17-19 May).

Geomagnetic Forecast:

With the exception of an isolated unsettled or active period early on day 1 (17 May) from an expected solar sector boundary crossing, geomagnetic field conditions are expected to be mostly quiet throughout the period (17-19 May).


Forecast of Solar and Geomagnetic Activity
14 May - 09 June 2012

Solar activity is expected to be at low to moderate levels throughout the period, with moderate activity most likely with the return of Old Region 1476 on 31 May.

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at normal levels except on 14 May, 23-29 May, and 06-09 June. The high levels are expected in response to the presence of recurrent coronal hole high speed streams.

Geomagnetic field activity is expected to be quiet to unsettled with occasional active periods. The unsettled to active periods are associated with the geoeffective periods of recurrent CH-HSSs on 14 May, 21-23 May, and 05-08 June. Unsettled to occasionally active conditions are also expected on 14 May with the anticipated arrival of a CME from 12 May.




Real-time foF2 map from IPS (Ionospheric Prediction Service), Australian Space Weather Agency

foF2 Map from IPS, Australia

Space Weather Page



Click on image to
view larger versions

The following images
are from SOHO

SOHO Extreme ultraviolet Imaging Telescope (EIT) full-field Fe IX, X 171 Å image from NASA Goddard Space Flight Center
SOHO Extreme ultraviolet Imaging Telescope (EIT) full-field He II 195 Å images from NASA Goddard Space Flight Center
SOHO Extreme ultraviolet Imaging Telescope (EIT) full-field Fe XV 284 Å images from NASA Goddard Space Flight Center
SOHO Extreme ultraviolet Imaging Telescope (EIT) full-field He II 304 Å images from NASA Goddard Space Flight Center
SDO HMI Quick-Look Magnetogram
C2 LASCO Image
C3 LASCO Image
SDO/HMI Quick-Look Continuum (IGR)

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Additional Views of the Sun

Be sure to check the Date shown in each photo - is it today's date?
(click to enlarge)

Current Numbered Sunspots / MDI MagnetogramCatania Solar Disc

H-Alpha View 1H-Alpha View 2



Space Weather Information Monitor Software - sample screen shot Interested in keeping tabs on ALL of the current Space Weather information? Check out the Space Weather Information Monitor Software (SWIM) - support the NW7US / HFRadio.org Propagation Resource Center and purchase your copy of SWIM, today.

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Find out the full details about the Space Weather Information Monitor Software (SWIM).








Purchase the STD Internet Space Weather & Radio Propagation Forecasting Course


Solar Terrestrial Dispatch (STD) 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.

STD 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.

STD has developed a special space weather course designed to teach individuals without any background how to predict space weather (see below). The STD Space Weather 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, if you choose the option, also includes the STD workhorse, Space Weather Information Monitor (SWIM) software, which is the most comprehensive space and weather information monitor in the world. The course (if you choose the option, below) also includes the STD's powerful and 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.

Purchasing the Course

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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
    • The STD SW Course presents 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.
    • The Course presents you with several hypothetical (possible future) examples and ask you to develop your own forecasts.
  • Course Completed


Although this course is largely self-taught, STD will provide support if you run into difficulties. There are no prerequisites.



Check out these books on Radio Propagation:

+ The New Shortwave Propagation Handbook (Paperback) - by George Jacobs, Theodore J. Cohen, R. B. Rose. The NEW Shortwave Progagation Handbook may well be the only book you'll need on the subject of ionospheric propagation! It is a "must read" for Radio Amateurs, Shortwave Listeners, and radio communicators of any type who need to make the most productive use of the radio spectrum, regardless of the time of day, the season of the year, or the state of the sunspot cycle. It will become your ever-present companion a the operating table as you master the art of shortwave radio progagation.

+ How Radio Signals Work (Paperback) - by Jim Sinclair. This book provides a basic understanding of the way radio signals work-without becoming bogged down with the technicalities. It covers all kinds of radio signal types--including mobile communications, short-wave, satellite, and microwave. No detailed knowledge of electronics or mathematics is required. A-Z coverage of radio signals including satellites, mobile communications, and short-wave radio. No math or electronics background necessary.

+ Introduction to RF Propagation (Hardcover) - by John S. Seybold. This book provides readers with a solid understanding of the concepts involved in the propagation of electromagnetic waves and of the commonly used modeling techniques. While many books cover RF propagation, most are geared to cellular telephone systems and, therefore, are limited in scope. This title is comprehensive-it treats the growing number of wireless applications that range well beyond the mobile telecommunications industry, including radar and satellite communications.

I write the propagation columns for the following magazines:

CQ Magazine CQ Magazine America's fastest growing magazine for the active ham radio operator. CQ is the world's leading independent magazine devoted to amateur radio. For more than a half-century, CQ has been on ham radio's leading edge -- the first to promote mobile operating (in the 1950s), semiconductors (in the 1960s) and packet radio -- the original e-mail (in the 1980s). The amateur satellite program got its start with an idea in the pages of CQ!

CQ VHF Magazine CQ VHF Magazine It is back! May 2002 saw the return of this quarterly magazines that focuses on amateur radio above 50 MHz. Articles and columns target both the beginner as well as the expert.

Popular Communications Magazine Popular Communications Magazine Exciting reading for the shortwave and scanner listener. It features authoritative information on scanner monitoring of police, fire, utility and aircraft transmissions as well as short wave listening, monitoring short wave digital, fax and teletype broadcasts, cb radio, alternative radio, clandestine radio, telephones and wiretapping, bugging, surveillance, pirate broadcasters, military communications, amateur radio, satellite tv reception, radio history and nostalgia.

Monitoring Times Magazine Monitoring Times Magazine Contains news, information, and tips on getting more out of radio listening. Do you own a radio, a shortwave receiver, a scanning receiver, or a ham radio? Then Monitoring Times® is your magazine! Open a copy of MT, and you will find 92 pages of news, information, and tips on getting more out of your radio listening. In fact, it's the most comprehensive radio hobby magazine in the U.S. Packed with up-to-date information concisely written by the top writers in the field, Monitoring Times® is your foremost guide to profiles of broadcasting and communications installations; home projects; and tips on monitoring everything from air, sea, and space to distant ports of call.



Data and images courtesy of IPS Australia, NOAA, NASA, SWPC, SIDC

Layout, analysis, commentary, and certain forecasts and content is
Copyright, 2012, Tomas David Hood (NW7US), all rights reserved.
No part, except for the space weather 'banners', may be copied without express permission.

Last Update: May 12, 2012