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Radio Propagation : Space Weather : Sunspot Cycle Information

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


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plot of Kp

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Satellite Environment Plot




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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: 22-Oct-2017 UTC

Day-to-Day Conditions Expected for October 2017
Propagation Index
Days
(4)
(3)
(2)
(1)
Above Normal:
2-10,16-18,20-23,29-31
A
A
B
C
High Normal:
1,19,26-28
A
B
C
C-D
Low Normal:
11-12,15
B
C-B
C-D
D-E
Below Normal:
14,24
C
C-D
D-E
E
Disturbed:
13,25
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
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 24 Planetary A Index (Ap) Monthly Progress
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.

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



This page was rendered on 23-Oct-17 0749 UTC.
This page was first created in 1998, by Tomas David Hood (NW7US)

Current Sunspot Cycle 24 Activity and Space Weather

Sun Spots: 13 as of 10/22/2017 :: 10.7-cm Flux: 77 SFU
(SFU=Solar Flux Units)

Space Weather Overview Graphic from SWPC

30 Minutes of Dazzling Sun! Ultra-high Definition 4k View



An Intimate View of the Sun, Every Day of 2015 (Year 6 of SDO) UHD 4k



Watch Five Very Intense X-class X-ray Flares Erupt, Back-to-back!
(From the largest sunspot region in 20+ years...)



Check out the X2.7 X-ray Flare (May 5 2015) - 'Biggest' of 2015, so far



See highlights of the last five years of the Sun, as seen by SDO



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): 6 | Planetary K-index (Kp): 1
Solar Wind: 378 km/s at 7.0 protons/cm3, Bz is 1.0 nT
(Oct 23, 2017 at 0538 UT)

X-ray Solar Flares:
6h hi [B2.2][1208Z 10/22] 24h hi [B2.2][1208Z 10/22]

Background X-ray Level, Last Six Days

Oct 22 2017 :: A7.4
Oct 21 2017 :: A7.8
Oct 20 2017 :: A6.6
Oct 19 2017 :: A5.3
Oct 18 2017 :: A5.7
Oct 17 2017 :: A4.1


Check out the current Aurora Oval and activity.

Here is a video introduction to shortwave / HF amateur radio -- what is it that we amateur radio oprators listen to? If you have not yet been introduced to this world, this is a very basic introduction.






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 Radio Flux Index,
use the following predicted values in this following 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
2017 04
27.3
16.5
14.5
78.5
79.5
77.5
2017 05
26.7
17.9
13.9
78.1
79.1
77.1
2017 06
25.8
19.5
13.5
78.1
80.1
76.1
2017 07
24.5
22.0
12.0
78.1
81.1
75.1
2017 08
23.0
22.1
12.1
77.9
81.9
73.9
2017 09
21.8
23.4
11.4
77.7
81.7
73.7
2017 10
20.9
24.5
10.5
77.4
82.4
72.4
2017 11
20.2
24.5
10.5
77.0
83.0
71.0
2017 12
19.6
25.7
9.7
76.8
83.8
69.8
2018 01
18.8
26.9
8.9
76.3
84.3
68.3
2018 02
17.7
26.6
8.6
75.7
83.7
67.7
2018 03
16.7
26.7
6.7
74.4
83.4
65.4
2018 04
15.5
25.6
5.6
73.1
82.1
64.1
2018 05
14.5
24.5
4.5
72.1
81.1
63.1
2018 06
13.7
23.7
3.7
71.3
80.3
62.3
2018 07
13.4
22.9
2.9
70.6
79.6
61.6
2018 08
13.1
22.2
2.2
69.9
78.9
60.9
2018 09
12.5
21.5
1.5
69.2
78.2
60.2
2018 10
11.8
20.8
0.8
68.6
77.6
60.0
2018 11
11.1
20.1
0.1
68.0
77.0
60.0
2018 12
10.7
19.5
0.0
67.4
76.4
60.0
2019 01
18.9
0.0
66.9
75.9
60.0
2019 02
18.3
0.0
66.3
75.3
60.0
2019 03
17.8
0.0
65.9
74.9
60.0
2019 04
17.3
0.0
65.4
74.4
60.0
2019 05
16.8
0.0
65.0
74.0
60.0
2019 06
16.4
0.0
64.5
73.5
60.0
2019 07
15.9
0.0
64.1
73.1
60.0
2019 08
15.5
0.0
63.8
72.8
60.0
2019 09
15.1
0.0
63.4
72.4
60.0
2019 10
14.8
0.0
63.1
72.1
60.0
2019 11
14.4
0.0
62.8
71.8
60.0
2019 12
14.1
0.0
62.5
71.5
60.0


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 0700Z on 23 Oct, 2017
High Latitude: Normal
Middle Latitude: Normal
Low Latitude: Normal

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


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: 09 - 15 October 2017

Solar activity was at very low levels and spotless with the exception of the emergence of new Region 2684 (N11, L=312, class/area Bxo/010 on 15 Oct) late in the period. 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 at moderate levels on 09-11 Oct, high levels on 12-14 Oct, and very high levels on 15 Oct. The largest flux of the period was 59,298 pfu observed at 15/1645 UTC.

Geomagnetic field activity ranged from quiet to G2 (Moderate) storm levels. The period began with solar wind speeds between 300-400 km/s and total field ranging from 1-5 nT on 09-10 Oct. The geomagnetic field was at quiet levels on 09 Oct and quiet to unsettled levels on 10 Oct. By late on 10 Oct, total field and solar wind speed began to increase as a polar connected, positive polarity, coronal hole high speed stream (CH HSS) became geoeffective. Total field increased to 12 nT at 11/1115 UTC and solar wind speed gradually increased to a maximum of 737 km/s at 14/0550 UTC. Solar wind speed slowly decreased thereafter to near 550 km/s by the end of the period. The geomagnetic field responded with unsettled to G1 (Minor) geomagnetic storm levels on 11-12 Oct and 14-15 Oct. Quiet to G2 (Moderate) storm levels were observed on 13 Oct.



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 Z: Bz: nT
Bx: nT | By: nT | Total: nT
Most recent satellite polar pass:
Centered on // : UTC
Aurora Activity Level was at UTC
visit noaa for latest.

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





Outlook:
(valid from 1230UT, 22 Oct 2017 until 24 Oct 2017)

22 Oct 2017 10.7-cm Flux: 077 / Ap: 008
23 Oct 2017 10.7-cm Flux: 077 / Ap: 007
24 Oct 2017 10.7-cm Flux: 077 / Ap: 007

Forecast:

Solar Flares:
C-class flares expected, (probability >=50%)
Geo-Disturbance:
Quiet (A<20 and K<4)
Solar Proton Event:
Quiet

Comment from the SIDC (RWC Belgium): New NOAA region 2685 (identical to returning region 2682, rotating into view at the East limb) is currently the only sunspot region on the solar disk as seen from Earth. Returning region 2683 produced a B3.3 flare from behind the East limb, peaking at 21:06 UT on October 21. A filament eruption near 20W 20N was observed in GONG and AIA images around 18:13 UT on October 21, apparently without corresponding Coronal Mass Ejection (CME). C flares are possible in the next 24 hours (55% probability), with a chance for an M flare (15% probability). No Earth-directed CMEs were observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels. Solar wind speed registered by DSCOVR increased from about 380 to a maximum of about 510 km/s around 2h UT on October 22, and then gradually decreased to current values around 430 km/s. The magnitude of the Interplanetary Magnetic Field (IMF) varied between about 2 and 12 nT, with current values around 3.5 nT. The IMF was directed towards the Sun and Bz had a negative excursion around -5 nT between about 21:30 and 23:30 UT. Quiet to active conditions (K Dourbes between 1 and 4; NOAA Kp between 1 and 3) were registered in the past 24 hours. Quiet to unsettled geomagnetic levels (K Dourbes < 4) are expected on October 22, 23 and 24. TODAY'S ESTIMATED ISN : 012, BASED ON 20 STATIONS.

(Comments issued on 22 Oct 2017, 1230UT)



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
16 October - 11 November 2017

Solar activity is expected to be at very low levels. A chance for C-flares is likely on 19 Oct-03 Nov with the return of old Regions 2682 (S10, L=126) and 2683 (N13, L=111).

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at high to very high levels on 16-18 Oct and again on 27 Oct and 11 Nov. High levels are expected on 19-21 Oct, 25-26 Oct, 28 Oct-01 Nov and on 08-10 Nov due to recurrent CH HSS influences.

Geomagnetic field activity is expected to be at unsettled to active levels on 16-22 Oct, 24-29 Oct, 01-02 Nov, and 07-11 Nov. G1 (Minor) geomagnetic storm levels are likely on 24-25 Oct and 07-11 Nov and G2 (Moderate) levels are likely on 25 Oct and 10 Nov due to recurrent CH HSS effects.



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

foF2 Map from IPS, Australia

Space Weather + Ham Radio Resources


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
showing plasma rain on the Sun!



Check out this amazing NASA SDO (Solar Dynamics Observatory) video
showing a prominence the Sun:



Don't forget to join the Space Weather and Radio Propagation Facebook Page.


Summary & Medium Range Forecasts


Grey-line Terminator Map



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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






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.

Check out these articles:


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

Layout, analysis, commentary, and certain forecasts and content is
Copyright, 2017, Tomas David Hood (NW7US), all rights reserved.
No part, except for the space weather 'banners', may be copied without express permission.

Last Update: January 04, 2017