

























![Chaco Culture National Historical Park is a United States national historical park hosting the densest and most exceptional concentration of pueblos in the American Southwest. The park is located in northwestern New Mexico, between Albuquerque and Farmington, in a remote canyon cut by the Chaco Wash. Containing the most sweeping collection of ancient ruins north of Mexico, the park preserves one of the United States' most unique cultural and historic areas.[2] Chaco Culture National Historical Park is a United States national historical park hosting the densest and most exceptional concentration of pueblos in the American Southwest. The park is located in northwestern New Mexico, between Albuquerque and Farmington, in a remote canyon cut by the Chaco Wash. Containing the most sweeping collection of ancient ruins north of Mexico, the park preserves one of the United States' most unique cultural and historic areas.[2]](http://cdn7.wn.com/pd/7f/5f/b6f54502fd2bdde397cc7826ca45_small.jpg)



The solar cycle, or the solar magnetic activity cycle, is a periodic change in the amount of irradiation from the sun that is experienced on Earth. It has a period of about 11 years, and is one component of solar variation, the other being aperiodic fluctuations. Solar variation causes changes in space weather and to some degree weather and climate on Earth. The cycle is observed by counting the frequency and placement of sunspots visible on the Sun. Powered by a hydromagnetic dynamo process, driven by the inductive action of internal solar flows, the solar cycle:
Until recently it was thought that there were 28 cycles in the 309 years between 1699 and 2008, giving an average length of 11.04 years, but recent research has showed that the longest of these (1784–99) seems actually to have been two cycles, so that the average length is only around 10.66 years. Cycles as short as 9 years and as long as 14 years have been observed. Significant variations in amplitude also occur. Solar maximum and solar minimum refer respectively to epochs of maximum and minimum sunspot counts. Individual sunspot cycles are partitioned from one minimum to the next.
Following the numbering scheme established by Wolf, the 1755–1766 cycle is traditionally numbered "1". The period between 1645 and 1715, a time during which very few sunspots were observed, is a real feature, as opposed to an artifact due to missing data, and coincides with the Little Ice Age. This epoch is now known as the Maunder minimum, after Edward Walter Maunder, who extensively researched this peculiar event, first noted by Gustav Spörer. In the second half of the nineteenth century it was also noted (independently) by Richard Carrington and by Spörer that as the cycle progresses, sunspots appear first at mid-latitudes, and then closer and closer to the equator until solar minimum is reached. This pattern is best visualized in the form of the so-called butterfly diagram, first constructed by the husband-wife team of E. Walter and Annie Maunder in the early twentieth century (see graph below). Images of the Sun are divided into latitudinal strips, and the monthly-averaged fractional surface of sunspots calculated. This is plotted vertically as a color-coded bar, and the process is repeated month after month to produce this time-latitude diagram.
The physical basis of the solar cycle was elucidated in the early twentieth century by George Ellery Hale and collaborators, who in 1908 showed that sunspots were strongly magnetized (this was the first detection of magnetic fields outside the Earth), and in 1919 went on to show that the magnetic polarity of sunspot pairs:
Hale's observations revealed that the solar cycle is a magnetic cycle with an average duration of 22 years. However, because very nearly all manifestations of the solar cycle are insensitive to magnetic polarity, it remains common usage to speak of the "11-year solar cycle".
Half a century later, the father-and-son team of Harold Babcock and Horace Babcock showed that the solar surface is magnetized even outside of sunspots; that this weaker magnetic field is to first order a dipole; and that this dipole also undergoes polarity reversals with the same period as the sunspot cycle (see graph below). These various observations established that the solar cycle is a spatiotemporal magnetic process unfolding over the Sun as a whole.
One of the main authorities is SIDC (the Solar Influences Data Analysis Center) which is located in Belgium, and works with agencies such as NASA and ESA.
The most important information today comes from SOHO (a project of international cooperation between ESA and NASA), such as the MDI magnetogram, where the solar "surface" magnetic field can be seen.
The basic causes of the solar variability and solar cycles are still under debate, with some researchers suggesting a link with the tidal forces due to the gas giants Jupiter and Saturn, or due to the solar inertial motion. Another cause of sun spots can be solar jet stream "torsional oscillation".
The dipolar component of the solar magnetic field is observed to reverse polarity around the time of solar maximum, and reaches peak strength at the time of solar minimum. Sunspots, on the other hand, are produced from a strong toroidal (longitudinally-directed) magnetic field within the solar interior. Physically, the solar cycle can be thought of as a regenerative loop where the toroidal component produces a poloidal field, which later produces a new toroidal component of sign such as to reverse the polarity of the original toroidal field, which then produces a new poloidal component of reversed polarity, and so on.
TSI is higher at solar maximum, even though sunspots are darker (cooler) than the average photosphere. This is caused by magnetized structures other than sunspots during solar maxima, such as faculae and active elements of the "bright" network, that are brighter (hotter) than the average photosphere. They collectively overcompensate for the irradiance deficit associated with the cooler but less numerous sunspots. The primary driver of TSI changes on solar rotational and sunspot cycle timescales is the varying photospheric coverage of these radiatively active solar magnetic structures.
The photo montage to the left illustrates this variation for soft X-ray, as observed by the Japanese satellite Yohkoh from after August 30, 1991, at the peak of cycle 22, to September 6, 2001, at the peak of cycle 23. Similar cycle-related variations are observed in the flux of solar UV or EUV radiation, as observed, for example, by the SOHO or TRACE satellites.
Even though it only accounts for a minuscule fraction of total solar radiation, the impact of solar UV, EUV and X-ray radiation on the Earth's upper atmosphere is profound. Solar UV flux is a major driver of stratospheric chemistry, and increases in ionizing radiation significantly affect ionosphere-influenced temperature and electrical conductivity.
Sunspot activity has a major effect on long distance radio communications particularly on the shortwave bands although medium wave and low VHF frequencies are also affected. High levels of sunspot activity lead to improved signal propagation on higher frequency bands, although they also increase the levels of solar noise and ionospheric disturbances. These effects are caused by impact of the increased level of solar radiation on the ionosphere.
It has been proposed that 10.7 cm solar flux can interfere with point-to-point terrestrial communications.
The occurrence frequency of coronal mass ejections and flares is strongly modulated by the solar activity cycle. Flares of any given size are some 50 times more frequent at solar maximum than at minimum. Large coronal mass ejections occur on average a few times a day at solar maximum, down to one every few days at solar minimum. The size of these events themselves does not depend sensitively on the phase of the solar cycle. A good recent case in point are the three large X-class flares having occurred in December 2006, very near solar minimum; one of these (an X9.0 flare on Dec 5) stands as one of the brightest on record.
The impact of Solar cycle on living organisms has been investigated (see chronobiology). Some researchers claim to have found connections with human health.
The amount of UVB light at 300 nm reaching the Earth varies by as much as 400% over the solar cycle due to variations in the protective ozone layer. In the stratosphere, ozone is continuously regenerated by the splitting of O2 molecules by ultraviolet light. During a solar minimum, the decrease in ultraviolet light received from the Sun leads to a decrease in the concentration of ozone, allowing increased UVB to penetrate to the Earth's surface.
Observations have shown correlations between the length of the solar cycle and observed (or proxy-calculated) atmospheric temperature on the earth.
The most well-documented connection between solar activity and climate change is the Maunder Minimum, during which cold weather prevailed in Europe. Research suggests a new 90-year Maunder minimum would result in a reduction of global average temperatures of about 0.3°C, which would not be enough to offset the ongoing and forecasted average global temperature increase due to global warming.
Daniel J. Hancock and Douglas N. Yarger found "statistically significant relationships between the double [~21 year] sunspot cycle and the 'January thaw' phenomenon along the East Coast and between the double sunspot cycle and 'drought' (June temperature and precipitation) in the Midwest."
Category:Stellar phenomena Cycle
ca:Cicle solar cs:Sluneční cyklus de:Sonnenfleck#Zyklen eo:Suna ciklo fr:Cycle solaire hr:Sunčev ciklus it:Ciclo undecennale dell'attività solare nl:Zonnecyclus no:Solflekksyklusen pt:Ciclo solar ro:Ciclul solar ru:Солнечный цикл sr:Соларни циклус sv:Solfläckscykeln uk:Цикли сонячної активності zh:太陽週期This text is licensed under the Creative Commons CC-BY-SA License. This text was originally published on Wikipedia and was developed by the Wikipedia community.
| Coordinates | 28°36′50″N77°12′32″N |
|---|---|
| name | Alfred Lambremont Webre |
| birth date | May 24, 1942 |
| birth place | Pensacola, Florida |
| education | Yale UniversityYale Law SchoolUniversity of Texas at Brownsville |
| occupation | AuthorLawyerFuturistPeace ActivistEnvironmental ActivistSpace Activist |
| spouse | Geri DiStefano Webre |
| children | }} |
In 2000, he was a presenter at the Presidential Forum on Off-Planet Cultures Policy at the Santa Clara Convention Center in California. Since 2002, he is the host of "The Monday Brown Bagger", a public affairs radio talk show on Coop Radio CFRO 102.7 FM in Vancouver, British Columbia. He is a founding director of Canada's No Weapons in Space Campaign (NOWIS) established in 2002. In 2004, he created the Campaign for Cooperation in Space (CCIS), an international organization where he works with others to prevent the weaponization of space and promote the transformation of the war economy into a peaceful, cooperative space exploration industry. On March 8, 2004, Webre attended the Council of Canadians public forum at the Maritime Labour Centre in Vancouver. On March 14, 2005 Webre joined the editorial and advisory team for Peace Media. On February 16, 2007, Webre said that the 2007 Chinese anti-satellite missile test occurred in order to stop the United States from proliferating weapons in space.
The ICIS board is made up of various prominent individuals such as former astronauts Edgar Mitchell and Dr. Brian O'Leary, and formerly the late Arthur C. Clarke, General Council Daniel Sheehan and John McConnell who is the founder of International Earth Day.. Alfred Webre resigned from the Board of Directors of ICIS on January 1, 2011 to focus on a treaty to ban HAARP, which he alleges to be a weapon.
Webre believes that as exopolitics posits, the truest conception of our human circumstance may be that we are on an isolated planet in the midst of a populated, evolving, highly organized inter-planetary, inter-galactic, multi-dimensional Universe society. He believes that we live on a planet that has been quarantined (the Zoo Hypothesis) and that we are now being given an opportunity to join the rest of the spiritually evolved Universe Society in peace, thus an opportunity to avoid environmental global self-destruction or global self-destruction through war.
On March 10, 2007, Webre launched the Exopolitics Radio program, hosted by 1480 KPHX (which at the time was the Air America Radio affiliate, and Nova M Radio flagship station, in Phoenix) until the fall of 2008; the program remains in production and is distributed via podcast on its own website . Guests on the program have been generally advocates of views similar to that of Webre, and many are well known within the UFO research/enthusiast (and to a lesser extent the New Age) community.
Category:1942 births Category:Living people Category:People from Pensacola, Florida Category:American environmentalists Category:American anti-war activists Category:American UFO writers Category:Washington, D.C. lawyers Category:Futurologists Category:SRI International people Category:Ufologists Category:UFO conspiracy theorists Category:Yale Law School alumni Category:Yale University faculty Category:Fulbright Scholars Category:Writers from Florida
This text is licensed under the Creative Commons CC-BY-SA License. This text was originally published on Wikipedia and was developed by the Wikipedia community.
The World News (WN) Network, has created this privacy statement in order to demonstrate our firm commitment to user privacy. The following discloses our information gathering and dissemination practices for wn.com, as well as e-mail newsletters.
We do not collect personally identifiable information about you, except when you provide it to us. For example, if you submit an inquiry to us or sign up for our newsletter, you may be asked to provide certain information such as your contact details (name, e-mail address, mailing address, etc.).
When you submit your personally identifiable information through wn.com, you are giving your consent to the collection, use and disclosure of your personal information as set forth in this Privacy Policy. If you would prefer that we not collect any personally identifiable information from you, please do not provide us with any such information. We will not sell or rent your personally identifiable information to third parties without your consent, except as otherwise disclosed in this Privacy Policy.
Except as otherwise disclosed in this Privacy Policy, we will use the information you provide us only for the purpose of responding to your inquiry or in connection with the service for which you provided such information. We may forward your contact information and inquiry to our affiliates and other divisions of our company that we feel can best address your inquiry or provide you with the requested service. We may also use the information you provide in aggregate form for internal business purposes, such as generating statistics and developing marketing plans. We may share or transfer such non-personally identifiable information with or to our affiliates, licensees, agents and partners.
We may retain other companies and individuals to perform functions on our behalf. Such third parties may be provided with access to personally identifiable information needed to perform their functions, but may not use such information for any other purpose.
In addition, we may disclose any information, including personally identifiable information, we deem necessary, in our sole discretion, to comply with any applicable law, regulation, legal proceeding or governmental request.
We do not want you to receive unwanted e-mail from us. We try to make it easy to opt-out of any service you have asked to receive. If you sign-up to our e-mail newsletters we do not sell, exchange or give your e-mail address to a third party.
E-mail addresses are collected via the wn.com web site. Users have to physically opt-in to receive the wn.com newsletter and a verification e-mail is sent. wn.com is clearly and conspicuously named at the point of
collection.If you no longer wish to receive our newsletter and promotional communications, you may opt-out of receiving them by following the instructions included in each newsletter or communication or by e-mailing us at michaelw(at)wn.com
The security of your personal information is important to us. We follow generally accepted industry standards to protect the personal information submitted to us, both during registration and once we receive it. No method of transmission over the Internet, or method of electronic storage, is 100 percent secure, however. Therefore, though we strive to use commercially acceptable means to protect your personal information, we cannot guarantee its absolute security.
If we decide to change our e-mail practices, we will post those changes to this privacy statement, the homepage, and other places we think appropriate so that you are aware of what information we collect, how we use it, and under what circumstances, if any, we disclose it.
If we make material changes to our e-mail practices, we will notify you here, by e-mail, and by means of a notice on our home page.
The advertising banners and other forms of advertising appearing on this Web site are sometimes delivered to you, on our behalf, by a third party. In the course of serving advertisements to this site, the third party may place or recognize a unique cookie on your browser. For more information on cookies, you can visit www.cookiecentral.com.
As we continue to develop our business, we might sell certain aspects of our entities or assets. In such transactions, user information, including personally identifiable information, generally is one of the transferred business assets, and by submitting your personal information on Wn.com you agree that your data may be transferred to such parties in these circumstances.