Jump to content
Toggle sidebar
Star Trek : Freedom's Wiki
Search
Log in
Personal tools
Log in
Pages for logged out editors
learn more
Contributions
Talk
Navigation
Main Page
Recent Changes
Help
Random Article
Random Image
popular
USS Templar
USS Paladin
USS Rosenante
USS Hades
USS Boudicca
USS Nimitz
USS Cochrane
USS Firebrande
USS Shenendoah
MEF
USS Dennison
USS Champlain
USS Mithrandir
USS Mystique
USS Starfire
USS Spectre
Page history
Federation Civil War
links
STF Home
Tools
What links here
Related changes
Special pages
Page information
Editing
Sol
(section)
Page
Discussion
English
Read
Edit
View history
More
Read
Edit
View history
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
===Sunspots and the sunspot cycle=== When observing the Sun with appropriate filtration, the most immediately visible features are usually its sunspots, which are well-defined surface areas that appear darker than their surroundings because of lower temperatures. Sunspots are regions of intense magnetic activity where convection is inhibited by strong magnetic fields, reducing energy transport from the hot interior to the surface. The magnetic field gives rise to strong heating in the corona, forming active regions that are the source of intense solar flares and coronal mass ejections. The largest sunspots can be tens of thousands of kilometers across. The number of sunspots visible on the Sun is not constant, but varies over an 11-year cycle known as the Solar cycle. At a typical solar minimum, few sunspots are visible, and occasionally none at all can be seen. Those that do appear are at high solar latitudes. As the sunspot cycle progresses, the number of sunspots increases and they move closer to the equator of the Sun, a phenomenon described by Spörer's law. Sunspots usually exist as pairs with opposite magnetic polarity. The magnetic polarity of the leading sunspot alternates every solar cycle, so that it will be a north magnetic pole in one solar cycle and a south magnetic pole in the next. Image:Sunspot-number.pngthumbright250pxHistory of the number of observed sunspots during the last 250 years, which shows the ~11-year solar cycle. The solar cycle has a great influence on space weather, and is a significant influence on the Earth's climate. Solar activity minima tend to be correlated with colder temperatures, and longer than average solar cycles tend to be correlated with hotter temperatures. In the 17th century, the solar cycle appears to have stopped entirely for several decades; very few sunspots were observed during this period. During this era, which is known as the Maunder minimum or Little Ice Age, Europe experienced very cold temperatures. Earlier extended minima have been discovered through analysis of tree rings and also appear to have coincided with lower-than-average global temperatures.
Summary:
Please note that all contributions to Star Trek : Freedom's Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Project:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)