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I highly recommend the following...

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NEW! ACE HF Pro
This is the best propagation modeling and circuit simulation software for Amateur and Shortwave Radio Operators
ACE-HF Modeling Software


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PropLab Pro
Best ionospheric ray-tracing software for Radio Operators
PropLab Pro Ray-tracing Software


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Hot: STD Space Weather Course
This is an excellent self-study course on Space Weather and Radio Propagation. This is a very in-depth and rich course that will equip you with the knowledge you need for understanding Space Weather, the ionosphere, how radio signals propagate via the ionosphere, and much more. Check it out!
STD Space Weather Course


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Take a listen to the Space Weather Podcast!

NW7US Space Weather / Radio Proapgation Podcast; E4 - Subject: No more sunspots by 2015!? It is possible, if the trend revealed in current sunspot research at Kitt Peak, AZ, continues. Listen now!

Podcast home: NW7US Podcast


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Gain the on-air edge: This article explains how the ANTENNA is the key! -> Read this introduction to Antenna Modeling


STEREO 3D

STEREO 3D IMAGE

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




Main Propagation Menu:

+ Sunspot Cycle/MUF/FOT Tables
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How-To Articles:

- Is HF Propagation Reciprocal?
- De-mystifying HF Radio Propagation and Modeling

Check out the ACE-HF propagation software - the latest is version 2.05. ACE-HF is propagation forecasting and modeling for Amateur Radio as well as for Shortwave radio Listening and general HF operation. This software is even used by the military and other clients around the world. This software is developed and maintained by the same engineers that keep VOACAP up-to-date. As a result, this software is the most accurate user interface integrated with VOACAP. CHECK IT OUT, TODAY. This software is the most accurate modeling software available, and is endorsed by NW7US. Read the details to find out why.



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NW7US Update to CQ Magazine Last Minute Forecast
Updated: 31-Jan-2015 UTC

Day-to-Day Conditions Expected for January 2015
Propagation Index
Days
(4)
(3)
(2)
(1)
Above Normal:
9-20,23-25,28-29,31
A
A
B
C
High Normal:
5-6,8,21-22,26-27,30
A
B
C
C-D
Low Normal:
No days
B
C-B
C-D
D-E
Below Normal:
7
C
C-D
D-E
E
Disturbed:
No days
C-D
D
E
E

To use this chart, please refer to my Propagation Column in CQ Magazine.




Warnings/Alerts issued
in the last 24 hours, if any:
(Key: NOAA Scales)


[ 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
70%
60%
X-class
25%
20%
Proton
25%
20%
Geomagnetic Activity Probabilities

Middle latitudes
High latitudes

0-24 hrs
24-48 hrs
0-24 hrs
24-48 hrs
Active
25%
20%
25%
20%
Minor Storm
25%
20%
25%
20%
Major-severe Storm
25%
20%
25%
20%


Solar Sunspot Cycle 24 Progress

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

Do you want the latest solar conditions sent to you as an RSS feed? Click: XML RSS propagation feed

You will need a newsreader for RSS/XML.

This RSS is Validated:
This Propagation RSS Feed is a Valid RSS feed.

(Use http://hfradio.org/propsupport/prop.rss as your RSS channel url)



This page was rendered on 01-Feb-15 0704 UTC.
This page was first created in 1998, by Tomas David Hood (NW7US)

Current Sunspot Cycle 24 Activity and Space Weather

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Sun Spots: 153 as of 01/31/2015 :: 10.7-cm Flux: 154 SFU
(SFU=Solar Flux Units)

Space Weather Overview Graphic from SWPC

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.


Planetary A-index (Ap): 9 | Planetary K-index (Kp): 3
Solar Wind: 488 km/s at 9.0 protons/cm3, Bz is 4.0 nT
(Feb 01, 2015 at 0652 UT)

X-ray Solar Flares:
6h hi [C2.8][0324Z 02/01] 24h hi [C2.8][0324Z 02/01]

Background X-ray Level, Last Six Days

Jan 31 2015 :: B6.3
Jan 30 2015 :: B8.6
Jan 29 2015 :: B9.4
Jan 28 2015 :: B9.5
Jan 27 2015 :: B9.6
Jan 26 2015 :: B7.0


Check out the current Aurora Oval and activity.

Post by Space Weather and Radio Resources at HFRadio.org.


If you are using software utilities such as Ace-HF, that require a "smoothed" sunspot number
(Referred to as the SSN), or the smoothed 10.7-cm flux index,
use the following predicted values in this table:

Predicted SMOOTHED Sunspot Number And Radio Flux Values
With Expected Ranges
YR/MO
Smoothed Sunspot Number
Predicted/High/Low
Smoothed 10.7 cm Radio Flux
Predicted/High/Low
2014 07
77.0
79.8
77.8
144.5
145.5
143.5
2014 08
75.3
79.0
75.0
141.1
142.1
140.1
2014 09
73.1
77.7
71.7
138.0
140.0
136.0
2014 10
71.1
78.0
68.0
135.8
138.8
132.8
2014 11
69.4
76.9
66.9
134.3
138.3
130.3
2014 12
67.7
77.1
65.1
133.7
137.7
129.7
2015 01
65.7
77.4
63.4
132.6
137.6
127.6
2015 02
63.8
76.4
62.4
131.2
137.2
125.2
2015 03
62.4
75.6
59.6
129.4
136.4
122.4
2015 04
61.4
75.2
57.2
126.2
134.2
118.2
2015 05
59.9
74.5
56.5
122.5
130.5
114.5
2015 06
57.6
73.9
53.9
118.5
127.5
109.5
2015 07
55.1
72.0
52.0
115.6
124.6
106.6
2015 08
53.1
70.4
50.4
114.1
123.1
105.1
2015 09
51.7
68.7
48.7
112.6
121.6
103.6
2015 10
50.5
67.0
47.0
111.0
120.0
102.0
2015 11
49.4
65.3
45.3
109.5
118.5
100.5
2015 12
48.1
63.6
43.6
107.9
116.9
98.9
2016 01
46.8
61.9
41.9
106.3
115.3
97.3
2016 02
45.5
60.2
40.2
104.8
113.8
95.8
2016 03
44.0
58.5
38.5
103.2
112.2
94.2
2016 04
42.1
56.9
36.9
101.7
110.7
92.7
2016 05
40.4
55.2
35.2
100.2
109.2
91.2
2016 06
39.5
53.6
33.6
98.7
107.7
89.7
2016 07
38.7
52.0
32.0
97.2
106.2
88.2
2016 08
38.0
50.4
30.4
95.8
104.8
86.8
2016 09
37.1
48.8
28.8
94.3
103.3
85.3
2016 10
35.7
47.3
27.3
92.9
101.9
83.9
2016 11
33.8
45.7
25.7
91.5
100.5
82.5
2016 12
32.2
44.3
24.3
90.2
99.2
81.2
To understand more about the Maximum Usable Frequencies, and related
science, please read the MUF Basics Page.


Global HF Propagation Conditions
Global HF Propagation Conditions for 0600Z on 01 Feb, 2015
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


Global Ionospheric Map - Critical Frequencies - foF2 (Created with PropLab PRO)
Critical foF2 map (2014 June 08 at 1000 UTC)

At 0805 UTC, on 9 August 2011, a strong magnitude X6.9 X-ray flare -- the strongest yet in this current solar cycle (Cycle 24) -- 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: 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 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: 01 - 07 December 2014

Solar activity ranged from low to high levels with the majority of activity occurring from Region 2222 (S19, L=085, class/area Ekc/770 on 04 December). Region 2222 produced a total of 54 C-flares and 5 M-flares since it began its transit on the visible disk on 26 November. The largest flares of the period were an M1/1n at 01/0641 UTC, an M1/1n at 04/0810 UTC, a long duration M6 at 04/1825 UTC, an M1 at 04/1941 UTC, and another M1 at 05/1225 UTC. Region 2222 continued to be in a growth phase through 04 December, when it began to decay. By the end of the period, the region was a large Hkx/alpha group with approximately 640 millionths of area. No Earth-directed coronal mass ejections were observed.

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit was normal levels on 02 December, moderate levels on 01 and 03-06 December, and reached high levels on 07 December. Maximum flux values of 2,030 pfu were observed at 07/1755 UTC.

Geomagnetic field activity ranged from quiet to minor storm levels. Solar wind parameters measured at the ACE satellite were indicative of two negative polarity coronal hole high speed streams (CH HSS). The first began just after midday on 01 December. Solar wind speeds gradually increased from approximately 430 km/s to near 630 km/s while total field reached a peak of around 14 nT. Solar wind speed declined by 03 December, but remained enhanced around 400 km/s to 550 km/s through the majority of the period. By early on 06 December, total field increased to a maximum of 25 nT along with an increase in density as a co-rotating interaction region (CIR) began to influence the geomagnetic field. Solar wind speed showed an increase late on 06 December and through 07 December to a maximum around 800 km/s as a southern polar coronal hole extension became geoeffective. The geomagnetic field responded with quiet to unsettled levels on 02-03 and 05 December, quiet to active levels on 01, 04, and 06 December, and unsettled to minor storm (G1-Minor) on 07 December.



Monthly and smoothed sunspot number - The monthly mean sunspot number (blue) and 13-month smoothed monthly sunspot number (red) for the last five cycles. You can see that this current cycle, Cycle 24, is a weak cycle, compared to the last few.

(Click to see actual size)
Monthly and smoothed sunspot number chart

Daily and monthly sunspot number (last 13 years)

Daily sunspot number (yellow), monthly mean sunspot number (blue), smoothed monthly sunspot number (red) for the last 13 years and 12-month ahead predictions of the monthly smoothed sunspot number:

SC (red dots) : prediction method based on an interpolation of Waldmeier's standard curves; It is only based on the sunspot number series.

CM (red dashes) : method (from K. Denkmayr and P. Cugnon) combining a regression technique applied to the sunspot number series with the aa geomagnetic index used as a precursor (improved predictions during the minimum phase between solar cycles).

(Click to see actual size)
Daily and monthly sunspot number (last 13 years)

What is 'Space Weather'? Click on these two information slides to view them in full size:

What is Space Weather? Slide 1 of 2 What is Space Weather? Slide 2 of 2




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 2014 Dec 09 1853Z: Bz: -3.9 nT
Bx: -3.7 nT | By: 0.4 nT | Total: 5.4 nT
Most recent satellite polar pass:
Centered on 12/09/2014 : 1725 UTC
Aurora Activity Level was 4 at 1725 UTC
visit noaa for latest.

Real-Time Solar Wind data dials:

Solar Wind Dials
Auroral Power Map:

North Pole Auroral


[ 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



Outlook:
(valid from 1230UT, 31 Jan 2015 until 02 Feb 2015)

31 Jan 2015 10.7-cm Flux: 156 / Ap: 014
01 Feb 2015 10.7-cm Flux: 152 / Ap: 034
02 Feb 2015 10.7-cm Flux: 148 / Ap: 019

Forecast:

Solar Flares:
Active (M-class flares expected, probability >=50%)
Geo-Disturbance:
Minor storm expected (A>=30 or K=5)
Solar Proton Event:
Quiet

Comment from the SIDC (RWC Belgium): Flaring activity declined with only a few low-level C-class flares, and the strongest event produced by NOAA 2277 at the beginning of the period (M2.4 peaking at 12:16UT). NOAA 2268 simplified significantly. NOAA 2277 kept most of its mixed magnetic polarity portions. No earth- directed CMEs have been observed. The x-ray background flux has decreased to the B6-level. The larger than 10 MeV flux is still enhanced, but started a gradual decline after 21:00UT. There remains a chance on an isolated M-class flare. Solar wind speed ranged mostly between 390 and 450 km/s. Bz varied between -7 and +7 nT, with a sustained negative period from 16:00 till 20:00UT. Unsettled to locally active (K Dourbes = 4) conditions were recorded between 18:00 and 24:00UT. The solar wind is expected to be further disturbed with the arrival of the HSS of the extension of a southern polar CH late on 31 January or on 01 February. The geomagnetic field is expected to range from quiet to active conditions, with a possibility of a minor geomagnetic storm. TODAY'S ESTIMATED ISN : 102, BASED ON 13 STATIONS.

(Comments issued on 31 Jan 2015, 1201UT)



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 07 Dec 2014)

Solar Forecast:

Solar activity is expected to be low with a chance for M-class flares on days one, two, and three (08 Dec, 09 Dec, 10 Dec).

Geomagnetic Forecast:

The geomagnetic field is expected to be at quiet to minor storm levels on day one (08 Dec), quiet to active levels on day two (09 Dec) and quiet levels on day three (10 Dec).


Forecast of Solar and Geomagnetic Activity
08 December - 03 January 2015

Solar activity is expected to be at low levels with a chance for M-class flaring (R1-R2, Minor to Moderate) for the forecast period as region 2222 continues to rotate off the visible disk as well as the return of old Region 2209 (S13, L=251) on 08 December.

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is expected to reach high levels from 08-22 and again on 03 January due to CH HSS influence.

Geomagnetic field activity is expected to be at unsettled to minor storm (G1-Minor) on 08 December and 03 January due to CIR/CH HSS activity. Unsettled, with possible active, levels are expected on 09, 12-15, 17-20, 28-29 December due to recurrent CH HSS effects. Quiet to unsettled with possible isolated active periods are expected from 31 December through 02 January due to possible recurrent extended periods of negative Bz as part of a variable current sheet.



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

C2 LASCO Image
C3 LASCO Image

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Check out this amazing NASA SDO (Solar Dynamics Observatory) video
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Summary & Medium Range Forecasts


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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




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'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.

NOTE: The certificate is no longer being offered. The course, never-the-less, still provides you with a very well-rounded knowledge base with which you can understand and work with space weather and radio propagation data.

Purchasing the Course

path Please choose one of the following course packages.
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NOTE: After you finish ordering, through PayPal, please allow me time to process your order. I am not always in front of my computer, so it may take a while for me to finish the processing of your order. I shall e-mail you the moment I have processed the order, and will give you specific directions on how to download the Course file(s). PLEASE BE PATIENT WITH ME!

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


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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.

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

Layout, analysis, commentary, and certain forecasts and content is
Copyright, 2014, Tomas David Hood (NW7US), all rights reserved.
No part, except for the space weather 'banners', may be copied without express permission.

Last Update: December 22, 2014