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CYCLE 25 FORECASTED TO BE LOWEST IN 200 YRS

WHAT IS A GRAND SOLAR MINIMUM?

Before we explain what a Grand Solar Minimum is, we must first understand what a Solar Cycle is.

Roughly every 11 years, the Sun’s magnetic field completely flips. This means that the Sun’s north and south poles switch places. It then takes approximately another 11 years for the Sun’s north and south poles to flip back again.  The solar cycle affects activity on the surface of the Sun, such as sunspots which are caused by the Sun’s magnetic fields. As the magnetic fields change, so does the amount of activity on the Sun’s surface.

[embedyt] https://www.youtube.com/watch?v=M85W_POXqWs[/embedyt]

This visualization represents the constant changing of the Sun’s magnetic field over the course of four years. Video credit: NASA’s Scientific Visualization Studio

One way to track the solar cycle is by counting the number of sunspots. The beginning of a solar cycle is a solar minimum, when the Sun has the least sunspots.

Over time, solar activity—and the number of sunspots—increases.

The middle of the solar cycle is the solar maximum, or when the Sun has the most sunspots.

As the cycle ends, it fades back to the solar minimum and then a new cycle begins.

 

 

 

Images of the Sun during one solar cycle. Solar maximum occurred during 2001 while 1996 and 2006 were near solar minimum. Image credit: NASA

Here is an image I have assembled using images from the SDO in Cycle 24:

© GSM 2019
A day in the life of our Sun

Now that you have the basic concept what a typical Solar Minimum & Solar Maximum is in a Solar Cycle, let’s discuss a Grand Minimum.

This graph shows the number of sunspots seen each year for 400 years (from 1600 to 2000). There were almost no sunspots during the Maunder Minimum. During the Dalton Minimum, there were fewer sunspots than normal. Click on image for full size Image courtesy NASA

 

A Grand Solar Minimum occurs when several solar cycles exhibit lesser than average activity for decades or centuries. Solar cycles still occur during these grand solar minimum periods but are at a lower intensity than usual. Grand solar minima have shown some correlation with global and regional climate changes.

Approximate dates of

Solar Minimums & Maximums

~ ~ ~ ~ Event ~ ~ ~ ~

~ ~ ~ Start ~ ~ ~

~ ~ ~ End ~ ~ ~

Homeric Minimum

950BC

800BC

Roman Warm Period

250 BC

AD 400

Medieval Warm Period

950

1040

Oort minimum

1040

1080

Medieval maximum

1100

1250

Wolf minimum

1280

1350

Spörer Minimum

1450

1550

Maunder Minimum

1645

1715

Dalton Minimum

1790

1820

Glassberg Minimum

1880

1914

Modern Maximum

1914

2007

Click on the different Maximum & Minimums for more info above.

Take a look at what we will be adding more of soon:

What is a Super Grand Solar Minimum?

Grand Minima & Climate

Where to live?

Prepping for a Grand Minimum?

and much more so stay tuned!