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    Default Scientists Predict Rare 'Hibernation' Of Sunspots

    Scientists Predict Rare 'Hibernation' Of Sunspots
    June 15, 2011

    US scientists say the familiar sunspot cycle seems to be entering a hibernation period unseen since the 17th century, a pattern that could have a slight cooling effect on global temperatures.

    For years, scientists have been predicting the Sun would by around 2012 move into solar maximum, a period of intense flares and sunspot activity, but lately a curious calm has suggested quite the opposite.

    The signs include a missing jet stream, fading spots and slower activity near the poles, said a trio of studies presented Tuesday at the annual meeting of the American Astronomical Society's Solar Physics Division in Las Cruces, New Mexico.

    "This is highly unusual and unexpected," said Frank Hill, associate director of the National Solar Observatory's Solar Synoptic Network.

    "But the fact that three completely different views of the Sun point in the same direction is a powerful indicator that the sunspot cycle may be going into hibernation."

    Solar activity tends to rise and fall every 11 years or so. The solar maximum and solar minimum each mark about half the interval of the magnetic pole reversal on the Sun, which happens every 22 years.

    Experts are now probing whether this period of inactivity could be a second Maunder Minimum, a 70-year period when hardly any sunspots were observed between 1645-1715 known as the "Little Ice Age."

    "If we are right, this could be the last solar maximum we'll see for a few decades. That would affect everything from space exploration to Earth's climate," said Hill.

    Solar flares and eruptions can send highly charged particles hurtling toward Earth and interfere with satellite communications, GPS systems and even airline controls.

    Geomagnetic forces have been known to occasionally garble the world's modern gadgetry, and warnings were issued as recently as last week when a moderate solar flare sent a fiery coronal mass ejection in the Earth's direction.

    However, the temperature change associated with any reduction in sunspot activity would likely be minimal and not enough to offset the impact of greenhouse gases on global warming, according to scientists.

    "Recent solar 11-year cycles are associated empirically with changes in global surface temperature of 0.1 Celsius," said Judith Lean, a solar physicist with the US Naval Research Laboratory.

    If the cycle were to stop or slow down, the small fluctuation in temperature would do the same, eliminating the slightly cooler effect of a solar minimum compared to the warmer solar maximum. The phenomenon was witnessed during the descending phase of the last solar cycle.

    This "cancelled part of the greenhouse gas warming of the period 2000-2008, causing the net global surface temperature to remain approximately flat -- and leading to the big debate of why the Earth hadn't (been) warming in the past decade," Lean, who was not involved in the three studies presented, told AFP.

    Less sunspot activity means the Sun will radiate lower levels of energy, ultraviolet rays, solar wind and a weaker magnetic field, explained climate scientist and author Rasmus Benestad of the Norwegian Meteorological Institute.

    "Historical data suggest that solar activity, however, only appears to have a weak effect on our climate," said Benestad.

    A study in the March 2010 issue of Geophysical Research Letters explored what effect an extended solar minimum might have, and found no more than a 0.3 Celsius dip by 2100 compared to normal solar fluctuations.

    "A new Maunder-type solar activity minimum cannot offset the global warming caused by human greenhouse gas emissions," wrote authors Georg Feulner and Stefan Rahmstorf, noting that forecasts by the Intergovernmental Panel on Climate Change forecast a maximum 4.5 degree Celsius rise by this century's end compared to the latter half of the 20th century.

    "Moreover, any offset of global warming due to a grand minimum of solar activity would be merely a temporary effect, since the distinct solar minima during the last millennium typically lasted for only several decades or a century at most."

    Other experts were skeptical about whether the latest data actually predict a long-term solar minimum.

    "There is no compelling reason to think that the Sun is about to go into hibernation," said Yi-Ming Wang of the Naval Research Laboratory.

    "On the other hand, we don't understand the solar dynamo well enough to make any reliable prediction about what cycle 25 will be like."

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    Default Re: Scientists Predict Rare 'Hibernation' Of Sunspots

    BREAKING – Major AAS Solar Announcement: Sun’s Fading Spots Signal Big Drop in Solar Activity
    June 14, 2011

    “If we are right, this could be the last solar maximum we’ll see for a few decades,” Hill said. “That would affect everything from space exploration to Earth’s climate.”

    Update: see the official press release here – “All three of these lines of research to point to the familiar sunspot cycle shutting down for a while.

    It looks like Livingston and Penn are getting some long deserved recognition. See their graph below:



    Graph above from the WUWT solar reference page. Note: when the B gauss reading of sunspots hits 1500, they will no longer have enough contrast to be visible. That may occur at or near the years 2015-2017. WUWT carried a story in 2008 warning of this.

    The American Astronomical Society meeting in Los Cruces, NM has just made a major announcement on the state of the sun. Sunspots may be on the way out and an extended solar minimum may be on the horizon.

    From Space.com reporting from the conference:

    Some unusual solar readings, including fading sunspots and weakening magnetic activity near the poles, could be indications that our sun is preparing to be less active in the coming years.

    The results of three separate studies seem to show that even as the current sunspot cycle swells toward the solar maximum, the sun could be heading into a more-dormant period, with activity during the next 11-year sunspot cycle greatly reduced or even eliminated.

    The results of the new studies were announced today (June 14) at the annual meeting of the solar physics division of the American Astronomical Society, which is being held this week at New Mexico State University in Las Cruces.



    Currently, the sun is in the midst of the period designated as Cycle 24 and is ramping up toward the cycle’s period of maximum activity. However, the recent findings indicate that the activity in the next 11-year solar cycle, Cycle 25, could be greatly reduced. In fact, some scientists are questioning whether this drop in activity could lead to a second Maunder Minimum, which was a 70-year period from 1645 to 1715 when the sun showed virtually no sunspots.



    “We expected to see the start of the zonal flow for Cycle 25 by now, but we see no sign of it,” Hill said. “This indicates that the start of Cycle 25 may be delayed to 2021 or 2022, or may not happen at all.”



    If the models prove accurate and the trends continue, the implications could be far-reaching.

    “If we are right, this could be the last solar maximum we’ll see for a few decades,” Hill said. “That would affect everything from space exploration to Earth’s climate.”
    More on this as it unfolds. This article will be updated as new information becomes available.

    See also these previous WUWT posts leading up to this:

    Solar activity still driving in the slow lane

    Sun’s magnetics remain in a funk: sunspots may be on their way out

    The sun is still in a slump – still not conforming to NOAA “consensus” forecasts

    Livingston and Penn in EOS: Are Sunspots Different During This Solar Minimum?

    Livingston and Penn paper: “Sunspots may vanish by 2015″.

    Sunspots Today: A Cheshire Cat – New Essay from Livingston and Penn

    ================================================== =====================

    As I have been saying for some time:

    The long term Ap (the solar geomagnetic index) has been on a downtrend, ever since there was a step change in October 2005.



    Thanks to Leif Svalgaard, we have a more extensive and “official” Ap dataset (NOAA’s SWPC shown above has some small issues) that I’ve plotted below. The step change in October 2005 is still visible and the value of 3.9 that occurred in April of 2009 is the lowest for the entire dataset. The Ap Index was the lowest in 75 years then.



    And I’ve also plotted the 1991 to 2009 from BGS/Svalgaard to compare against the NOAA SWPC data:



    ================================================== ==========

    Dr. Leif Svalgaard writes:

    Here are the abstracts of the three studies referred to in the announcement:

    P16.10
    Large-scale Zonal Flows During the Solar Minimum — Where Is Cycle 25?13
    Frank Hill, R. Howe, R. Komm, J. Christensen-Dalsgaard, T. P. Larson, J. Schou, M. J. Thompson
    The so-called torsional oscillation is a pattern of migrating zonal flow bands that move from midlatitudes towards the equator and poles as the magnetic cycle progresses. Helioseismology allows us to probe these flows below the solar surface. The prolonged solar minimum following Cycle 23 was accompanied by a delay of 1.5 to 2 years in the migration of bands of faster rotation towards the equator. During the rising phase of Cycle 24, while the lower-level bands match those seen in the rising phase of Cycle 23, the rotation rate at middle and higher latitudes remains slower than it was at the corresponding phase in earlier cycles, perhaps reflecting the weakness of the polar fields. In addition, there is no evidence of the poleward flow associated with Cycle 25. We will present the latest results based on nearly sixteen years of global helioseismic observations from GONG and MDI, with recent results from HMI, and discuss the implications for the development of Cycle 25.

    P17.21
    A Decade of Diminishing Sunspot Vigor
    W. C. Livingston, M. Penn, L. Svalgaard
    s Convention Center
    Sunspots are small dark areas on the solar disk where internal magnetism, 1500 to 3500 Gauss, has been
    buoyed to the surface. (Spot life times are the order of one day to a couple of weeks or more. They are thought to be dark because convection inhibits the outward transport of energy there). Their “vigor” can be described by spot area, spot brightness intensity, and magnetic field. From 2001 to 2011 we have measured field strength and brightness at the darkest position in umbrae of 1750 spots using the Zeeman splitting of the Fe 1564.8 nm line. Only one observation per spot per day is carried out during our monthly telescope time of 3-4 days average. Over this interval the temporal mean magnetic field has declined about 500 Gauss and mean spot intensity has risen about 20%. We do not understand the physical mechanism behind these changes or the effect, if any, it will have on the Earth environment.

    P18.04
    Whither goes Cycle 24? A View from the Fe XIV Corona
    Richard C. Altrock
    Solar Cycle 24 had a historically prolonged and weak start. Observations of the Fe XIV corona from the Sacramento Peak site of the National Solar Observatory showed an abnormal pattern of emission compared to observations of Cycles 21, 22, and 23 from the same instrument. The previous three cycles had a strong, rapid “Rush to the Poles” in Fe XIV. Cycle 24 displays a delayed, weak, intermittent, and slow “Rush” that is mainly apparent in the northern hemisphere. If this Rush persists at its current rate, evidence from previous cycles indicates that solar maximum will occur in approximately early 2013. At lower latitudes, solar maximum previously occurred when the greatest number of Fe XIV emission regions* first reached approximately 20° latitude. Currently, the value of this parameter at 20° is approximately 0.15. Previous behavior of this parameter indicates that solar maximum should occur in approximately two years, or 2013. Thus, both techniques yield an expected time of solar maximum in early 2013.
    *annual average number of Fe XIV emission features per day greater than 0.19

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    Default Re: Scientists Predict Rare 'Hibernation' Of Sunspots

    If things keep going the way those charts are looking, we could be seeing some much colder weather.

    Think food prices are bad now?

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    Default Re: Scientists Predict Rare 'Hibernation' Of Sunspots

    It's only rare if you can't comprehend that a millennium is but eye-blink to an object that will burn for over 10 billion years.
    "Far better it is to dare mighty things, to win glorious triumphs even though checkered by failure, than to rank with those poor spirits who neither enjoy nor suffer much because they live in the gray twilight that knows neither victory nor defeat."
    -- Theodore Roosevelt


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    Default Re: Scientists Predict Rare 'Hibernation' Of Sunspots

    We'll get through it like humans have always gotten through it.

    We'll kill off most of the other humans.

    /chuckles
    Libertatem Prius!


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    Default Re: Scientists Predict Rare 'Hibernation' Of Sunspots

    Wait, I thought we were entering a Solar Maximum cycle?

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    Default Re: Scientists Predict Rare 'Hibernation' Of Sunspots

    Well... we should have been entering it a few years BACK....
    Libertatem Prius!


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