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Date: Thu, 5 Mar 2020 12:42:46 -0500
From: "Dog Training Course" <Dog’sbehavior@terminaterrs.buzz>
Reply-To: "Dog Training Course" <Dog’sbehavior@terminaterrs.buzz>
Subject: The secret to making your dog’s problem behaviors disappear
To: <leandro@planetline.it>
Message-ID: <d5ad9r8nrlx37feu-rsbt9jx97zcemegn-49f7-d616@terminaterrs.buzz>

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The secret to making your dog’s problem behaviors disappear

http://terminaterrs.buzz/8-gbc28yUcWWtOE4ITVfo9w98qrOrJpzk_dyziZxam92aSND

http://terminaterrs.buzz/qMZ6CIswqW-MnWyxcpShrlZMAU71Rzck0Ptdp5aIrE_YpovQ

The magnetic field also varies in time and location. The quasi-periodic 11-year solar cycle is the most prominent variation in which the number and size of sunspots waxes and wanes.

Sunspots are visible as dark patches on the Sun's photosphere, and correspond to concentrations of magnetic field where the convective transport of heat is inhibited from the solar interior to the surface. As a result, sunspots are slightly cooler than the surrounding photosphere, so they appear dark. At a typical solar minimum, few sunspots are visible, and occasionally none can be seen at all. Those that do appear are at high solar latitudes. As the solar cycle progresses towards its maximum, sunspots tend to form closer to the solar equator, a phenomenon known as Spörer's law. The largest sunspots can be tens of thousands of kilometers across.

An 11-year sunspot cycle is half of a 22-year Babcock–Leighton dynamo cycle, which corresponds to an oscillatory exchange of energy between toroidal and poloidal solar magnetic fields. At solar-cycle maximum, the external poloidal dipolar magnetic field is near its dynamo-cycle minimum strength, but an internal toroidal quadrupolar field, generated through differential rotation within the tachocline, is near its maximum strength. At this point in the dynamo cycle, buoyant upwelling within the convective zone forces emergence of toroidal magnetic field through the photosphere, giving rise to pairs of sunspots, roughly aligned east–west and having footprints with opposite magnetic polarities. The magnetic polarity of sunspot pairs alternates every solar cycle, a phenomenon known as the Hale cycle.

During the solar cycle's declining phase, energy shifts from the internal toroidal magnetic field to the external poloidal field, and sunspots diminish in number and size. At solar-cycle minimum, the toroidal field is, correspondingly, at minimum strength, sunspots are relatively rare, and the poloidal field is at its maximum strength. With the rise of the next 11-year sunspot cycle, differential rotation shifts magnetic energy back from the poloidal to the toroidal field, but with a polarity that is opposite to the previous cycle. The process carries on continuously, and in an idealized, simplified scenario, each 11-year sunspot cycle corresponds to a change, then, in the overall polarity of the Sun's large-scale magnetic field

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<html>
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	<title>Newsletter</title>
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<body> 
<a href="http://terminaterrs.buzz/sSoxZtTcwaxSsox_nN0CiOhyXjc5LEmdfjbnBfUd1b3a_wtu"><img src="http://terminaterrs.buzz/445adbdc079f7f9375.jpg" /><img height="1" src="http://www.terminaterrs.buzz/wPeMrcPAZ1RF7wIUK_F7PzlKI8VdLFJ1eL_xBD_E_U06951Q" width="1" /></a> 
&nbsp;
<center>
<div style="width:600px; padding:10px; text-align:left; font-size:19px; font-family:calibri; border: 1px solid #FFDFE1; ">
Hi dog lover,
No matter what your dog&rsquo;s problem behavior is&hellip; 
 
Be it jumping, peeing inappropriately, aggression, pulling on the leash&hellip;or whatever&hellip; 
 
There is ONE SOLUTION that can help <a href="http://terminaterrs.buzz/8-gbc28yUcWWtOE4ITVfo9w98qrOrJpzk_dyziZxam92aSND">STOP this problem now</a> 
 
The sad fact is&hellip; 
 
Most Dog trainers miss this solution entirely. 
 
They give you cookie cutting training programs. 
 
They use outdated and &lsquo;mean&rsquo; dominance techniques. 
 
Or worse yet&hellip; They have no qualifications and are complete phonies. 
 
So what&rsquo;s the answer to stopping your Dog&rsquo;s behavior problems? 
 
In 4 simple words&hellip; 
 
Discovering your dog&rsquo;s hidden intelligence. 
 
<a href="http://terminaterrs.buzz/8-gbc28yUcWWtOE4ITVfo9w98qrOrJpzk_dyziZxam92aSND">Let me explain&hellip;</a> 
 
In my 10 years as a certified trainer&hellip;there&rsquo;s ONE BIG LESSON I have learned. 
 
More intelligent dogs are better behaved. 
 
<a href="http://terminaterrs.buzz/8-gbc28yUcWWtOE4ITVfo9w98qrOrJpzk_dyziZxam92aSND">A More intelligent dog takes commands easier</a> 
 
&hellip;and understands what you need from them. 
 
The good news is&hellip; 
 
No matter how clever you think your dog is. 
 
You can &gt;&gt;&gt;unlock their hidden intelligence quickly and easily. 
 
<a href="http://terminaterrs.buzz/8-gbc28yUcWWtOE4ITVfo9w98qrOrJpzk_dyziZxam92aSND">&gt;&gt;&gt;I&rsquo;ll explain everything on this page.</a> 
 
Don&rsquo;t waste a second longer coping with problem behaviors you don&rsquo;t need to be dealing with. 
 
PS Check out the brain training for Dogs course now. It&rsquo;s great for eliminating any bad behaviors by tapping into your dog&rsquo;s hidden intelligence. 
 
<a href="http://terminaterrs.buzz/8-gbc28yUcWWtOE4ITVfo9w98qrOrJpzk_dyziZxam92aSND">PPS- check out the cool dog pictures on this page.</a> 
&nbsp;</div>
 
 
 
 
 
 
 
 
 
 
 
 
 
&nbsp;
The magnetic field also varies in time and location. The quasi-periodic 11-year solar cycle is the most prominent variation in which the number and size of sunspots waxes and wanes. Sunspots are visible as dark patches on the Sun&#39;s photosphere, and correspond to concentrations of magnetic field where the convective transport of heat is inhibited from the solar interior to the surface. As a result, sunspots are slightly cooler than the surrounding photosphere, so they appear dark. At a typical solar minimum, few sunspots are visible, and occasionally none can be seen at all. Those that do appear are at high solar latitudes. As the solar cycle progresses towards its maximum, sunspots tend to form closer to the solar equator, a phenomenon known as Sp&ouml;rer&#39;s law. The largest sunspots can be tens of thousands of kilometers across. An 11-year sunspot cycle is half of a 22-year Babcock&ndash;Leighton dynamo cycle, which corresponds to an oscillatory exchange of energy between toroidal and poloidal solar magnetic fields. At solar-cycle maximum, the external poloidal dipolar magnetic field is near its dynamo-cycle minimum strength, but an internal toroidal quadrupolar field, generated through differential rotation within the tachocline, is near its maximum strength. At this point in the dynamo cycle, buoyant upwelling within the convective zone forces emergence of toroidal magnetic field through the photosphere, giving rise to pairs of sunspots, roughly aligned east&ndash;west and having footprints with opposite magnetic polarities. The magnetic polarity of sunspot pairs alternates every solar cycle, a phenomenon known as the Hale cycle. During the solar cycle&#39;s declining phase, energy shifts from the internal toroidal magnetic field to the external poloidal field, and sunspots diminish in number and size. At solar-cycle minimum, the toroidal field is, correspondingly, at minimum strength, sunspots are relatively rare, and the poloidal field is at its maximum strength. With the rise of the next 11-year sunspot cycle, differential rotation shifts magnetic energy back from the poloidal to the toroidal field, but with a polarity that is opposite to the previous cycle. The process carries on continuously, and in an idealized, simplified scenario, each 11-year sunspot cycle corresponds to a change, then, in the overall polarity of the Sun&#39;s large-scale magnetic field
 
 
 
<a href="http://terminaterrs.buzz/qMZ6CIswqW-MnWyxcpShrlZMAU71Rzck0Ptdp5aIrE_YpovQ" target="_blank"><img src="http://terminaterrs.buzz/a8cbc0947f83cf3e99.jpg" /></a> 
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