Solar variation

Solar cycles are cyclic changes in behavior of the Sun. Many possible patterns have been noticed.

• 11 years: Most obvious is a gradual increase and decrease of the number of sunspots over a period of about 11 years, called the Schwabe cycle. The Babcock Model explains this as being due to a shedding of entangled magnetic fields. The Sun's surface is also the most active when there are more sunspots, although the luminosity does not change much due to an increase in bright spots (faculae).
• 22 years: Hale cycle. The magnetic field of the Sun reverses during each Schwabe cycle, so the magnetic poles return to the same state after two reversals.
• 88 years: Gleissberg cycle (70-100 years) is thought to be an amplitude modulation of the 11-year Schwabe Cycle (Sonnett and Finney, 1990).
• 200 years: Suess cycle.
• 2,300 years: Hallstatt cycle.
• Other patterns have been detected:
  • In carbon-14: 105, 131, 232, 385, 504, 805, 2,241 years (Damon and Sonnett, 1991).
  • During the Upper Permian 240 million years ago, mineral layers created in the Castile Formation show cycles of 2,500 years.

Predictions based on patterns

• A simple model based on emulating harmonics by multiplying the basic 11-year cycle by powers of 2 produced results similar to Holocene behavior. Extrapolation suggests a gradual cooling during the next few centuries with intermittent minor warmups and a return to near Little Ice Age conditions within the next 500 years. This cool period then may be followed approximately 1,500 years from now by a return to altithermal conditions similar to the previous Holocene Maximum. 2010 while the following cycle should have a maximum of about 70±30 in 2023. 1400 (cool) AD 2520 232 --?-- AD 1922 (cool) AD 2038 208 Suess AD 1898 (cool) AD 2002 88 Gleisberg AD 1986 (cool) AD 2030

  Solar irradiance of Earth and its surface

  Solar irradiance, or insolation, is the amount of sunlight which reaches the Earth. The equipment used might measure optical brightness, total radiation, or radiation in various frequencies. Historical estimates use various measurements and proxies.

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  MODIS_ATM_solar_irradiance.jpg

  Solar irradiance spectrum above atmosphere and at surface

  There are two common meanings:

  • the radiation reaching the upper atmosphere
  • the radiation reaching some point within the atmosphere, including the surface.

  Various gases within the atmosphere absorb some solar radiation at different wavelengths, and clouds and dust also affect it. Hence measurements above the atmosphere are needed to observe variations in solar output, within the confounding effects of changes to the atmosphere. Indeed, there is some evidence that sunshine at the Earth's surface has been decreasing in the last 50 years (see global dimming) possibly caused by increased atmospheric pollution, whilst over roughly the same timespan solar output has been nearly constant.

  Milankovitch cycle variations

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  Some variations in insolation are not due to solar changes but rather due to the Earth moving closer or further from the Sun, or changes in the relative amount of radiation reaching regions of the Earth. These have caused variations of as much as 25% (locally; global average changes are much smaller) in solar insolation over long periods. The most recent significant event was an axial tilt of 24° during boreal summer at near the time of the Holocene climatic optimum.

  For details see the main article: Milankovitch cycles

  
  

  Solar interactions with Earth

  There are several ways that solar variations may affect Earth. Some variations, such as changes in the size of the Sun, are presently only of interest in the field of astronomy.

  Changes in total irradiance

  • Overall brightness may change.
  • The variation during recent cycles has been about 0.1%.
  • Changes corresponding to solar changes with periods of 9-13, 18-25, and >100 years been measured in sea-surface temperatures.
  • Since the Maunder Minimum, over the past 300 years there probably has been an increase of 0.1 to 0.6%, with climate models often using a 0.25% increase.

  Changes in ultraviolet irradiance

  • Ultraviolet irradiance (EUV) ranges widely through factors of 2 to 10 during a solar cycle.
  • Energy changes in the UV wavelengths involved in production and loss of ozone have atmospheric effects.
    • The 30 hPa pressure level has changed height in phase with solar activity during the last 4 solar cycles.
    • UV irradiance increase causes higher ozone production, leading to stratospheric heating and to poleward displacements in the stratospheric and tropospheric wind systems.
  • A proxy study estimates that UV increased by 3% since the Maunder Minimum.

  Changes in the solar wind and the Sun's magnetic flux

  • A more active solar wind and stronger magnetic field reduces the cosmic rays striking the Earth's atmosphere.
  • Variations in the solar wind affect the size and intensity of the heliosphere, the volume larger than the Solar System filled with solar wind particles.
  • Levels of ¹⁴C and ¹⁰Be show changes tied to solar activity.
  • Cosmic ray ionization in the upper atmosphere does change, but significant effects are not obvious.
  • As the solar coronal-source magnetic flux doubled during the past century, the cosmic-ray flux has decreased by about 15%.
  • The Sun's total magnetic flux rose by a factor of 1.41 from 1964-1996 and by a factor of 2.3 since 1901.

  Effects on clouds

  • Cosmic rays may affect formation of clouds.
  • 1983-1994 data from the International Cloud Climate Project (ISCCP) showed that global low cloud formation was highly correlated with cosmic ray flux.
  • The Earth's albedo decreased by about 2.5% over 5 years during the recent solar cycle, as measured by lunar "Earthshine". Similar reduction was measured by satellites during the previous cycle.
  • Mediterranean core study of plankton detected a solar-related 11 year cycle, and an increase 3.7 times larger between 1760 and 1950. A considerable reduction in cloud cover is proposed.

  Other effects due to solar variation

  Interaction of solar particles, the solar magnetic field, and the Earth's magnetic field, cause variations in the particle and electromagnetic fields at the surface of the planet. Extreme solar events can affect electrical devices. Weakening of the Sun's magnetic field is believed to increase the number of interstellar cosmic rays which reach Earth's atmosphere, altering the types of particles reaching the surface. It has been speculated that a change in cosmic rays could cause an increase in certain types of clouds, affecting Earth's albedo.

  Geomagnetic effects

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  Magnetosphere_rendition.jpg

  Solar particles interact with Earth's magnetosphere

  The Earth's polar aurora are visual displays created by interactions between the solar wind, the solar magnetosphere, the Earth's magnetic field, and the Earth's atmosphere. Variations in any of these affect aurora displays.

  Sudden changes can cause the intense disturbances in the Earth's magnetic fields which are called geomagnetic storms.

  Solar proton events

  Energetic protons can reach Earth within 30 minutes of a major flare's peak. During such a solar proton event, Earth is showered energetic solar particles (primarily protons) released from the flare site. Some of these particles spiral down Earth's magnetic field lines, penetrating the upper layers of our atmosphere where they produce additional ionization and may produce a significant increase in the radiation environment.

  Galactic cosmic rays

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  Heliosphere_drawing.gif

  Solar wind and magnetic field create heliosphere around solar system.

  An increase in solar activity (more sunspots) is accompanied by an increase in the "solar wind," which is an outflow of ionized particles, mostly protons and electrons, from the sun. The Earth's geomagnetic field, the solar wind, and solar magnetic field deflects galactic cosmic rays (GCR). A decrease in solar activity increases the GCR penetration of the troposphere and stratosphere. GCR particles are the primary source of ionization in the troposphere above 1 km (below 1 km, radon is a dominant source of ionization in many areas).

  Levels of GCRs have been indirectly recorded by their influence on the production of carbon-14 and beryllium-10. The Hallstatt solar cycle length of approximately 2300 years is reflected by climatic Dansgaard-Oeschger events. The 80-90 year solar Gleissberg cycles appear to vary in length depending upon the lengths of the concurrent 11 year solar cycles, and there also appear to be similar climate patterns occurring on this time scale.

  Cloud effects

  Changes in ionization affect the abundance of aerosols that serve as the nuclei of condensation for cloud formation. As a result, ionization levels potentially affect levels of condensation, low clouds, relative humidity, and albedo due to clouds. Clouds formed from greater amounts of condensation nuclei are brighter, longer lived, and likely to produce less precipitation. Changes of 3-4% in cloudiness and concurrent changes in cloud top temperatures have been correlated to the 11 and 22 year solar (sunspot) cycles, with increased GCR levels during "antiparallel" cycles.^{Carbon-14: 14C) also is related to solar activity. Radiocarbon is produced in the upper atmosphere by bombardment of atmospheric nitrogen (14N) with neutrons from outer space (cosmic rays). Increased solar activity reduces cosmic rays and reduces 14C production. Therefore, the 14C concentration of the atmosphere is lower during sunspot maxima and higher during sunspot minima. By measuring the captured 14C in wood and counting tree rings, production of radiocarbon relative to recent wood can be measured and dated. A reconstruction of the past 10,000 years shows that the 14C production was much higher during the mid-Holocene 7,000 years ago and decreased until 1,000 years ago. In addition to variations in solar activity, the long term trends in Carbon-14 production are influenced by changes in the Earth's geomagnetic field and by changes in carbon cycling within the biosphere (particularly those associated with changes in the extent of vegetation since the last ice age)Earth's average temperature and climate - sometimes finding an effect, and sometimes not. When effects are found they have tended to be greater than can be explained by direct response to the change in radiative forcing from solar change, so feedback or amplification mechanisms are required.[12] For a discussion of attribution of causes of current global warming see: Attribution of recent climate change}

  Research by Willie Soon and Sallie Baliunas presents evidence that variations in solar radiation produced the warming that "put the green in Greenland" and led to a "Little Ice Age". The IPCC's estimate of solar forcing since 1750 is available [13]. More recently Lean et al 2002 say that total solar irradiance may also lack significant secular trends.

  Douglass and Clader, Geophysical Research Letters, 2002 indicate that the climate response to forcings due to solar variations has been about twice that of simple radiation balancing, in agreement with the standard idea that some feedback mechanism is required to explain the influence of solar forcing found in ocean measurements and paleo data.

  In 2003, Shaviv and Veizer compared a temperature reconstruction of the last 500 million years to expected changes in cosmic ray flux as the solar system moves around the galaxy. They concluded that, at least over very long time scales, cosmic ray variations had a much larger impact on climate than other processes (such as greenhouse gas changes) [14]. Since, as described above, cosmic rays are also affected solar variations, their work may imply a larger role for solar variability in recent climate change than has previously been appreciated. Also, by looking at the temperature changes not ascribed to cosmic rays, they estimated that the climate response to doubling CO₂ is only about 0.75 °C as compared to the 1.5-4.5 °C reported by the IPCC [15]. However, long-term processes occurring over millions of years may make it impossible to interpret of Shaviv & Veizer's results over the short time scales relevant to recent warming. [16].

  Solar variation in climate models

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  Solar_Forcing_GISS_model.gif

  Solar forcing 1850-2050 used in a NASA GISS climate model. Recent variation pattern used after 2000.

  Climate models are computer simulations which are used to examine understanding of climate behavior. Some models use constant values for solar irradiance, while some include the heating effects of a variable Sun. A good simulation by GCMs of global mean temperature over the last 100 years requires both natural (solar; volcanic) and human (greenhouse gas) factors.

  There is currently no clear agreement as to the likely magnitude of long-term (last hundred or more years) solar variation. The IPCC discuss this in section 6.11 of the TAR [17] and show various results including Lean et al. (1995) [18]. However the Lean 1995 value may well be too high: more recently Lean et al (GRL 2002, [19]) say:

  Our simulation suggests that secular changes in terrestrial proxies of solar activity (such as the 14C and 10Be cosmogenic isotopes and the aa geomagnetic index) can occur in the absence of long-term (i.e., secular) solar irradiance changes. ...this suggests that total solar irradiance may also lack significant secular trends. ...Solar radiative forcing of climate is reduced by a factor of 5 when the background component is omitted from historical reconstructions of total solar irradiance ...This suggest that general circulation model (GCM) simulations of twentieth century warming may overestimate the role of solar irradiance variability. ...There is, however, growing empirical evidence for the Sun's role in climate change on multiple time scales including the 11-year cycle ...Climate response to solar variability may involve amplification of climate modes which the GCMs do not typically include. ...In this way, long-term climate change may appear to track the amplitude of the solar activity cycles because the stochastic response increases with the cycle amplitude, not because there is an actual secular irradiance change.

  In 2003, Stott et al found that "current climate models underestimate the observed climate response to solar forcing over the twentieth century as a whole, indicating that the climate system has a greater sensitivity to solar forcing than do models." [20]

  History of study of solar variations

  The longest recorded aspect of solar variations are changes in sunspots. Shortly after astronomers began using the telescope in 1609, sunspots and their motions were observed. Initial study was focused on their nature and behavior. Although the physical aspects of sunspots was not identified until the 1900s, observations continued. Study was hampered during the 1600s and 1700s due to the low number of sunspots during what is now recognized as an extended period of low solar activity, this event named the Maunder Minimum. By the 1800s records of their numbers began to show variations in their numbers. For details about sunspots see the main article: Sunspot

  Around 1900 connections between solar variations and weather on Earth began to be explored. Challenges are shown in the efforts of Charles Greeley Abbot, assigned by the Smithsonian Astrophysical Observatory to detect changes in the radiation of the Sun. His team had to begin by inventing instruments to measure solar radiation. Later, when he was head of the SAO, it established a solar station at Calama, Chile to complement its data from Mount Wilson Observatory. He detected 27 harmonic periods within the 273-month Hale cycles, including 7, 13, and 39 month patterns. He looked for connections to weather by means such as matching opposing solar trends during a month to opposing temperature and precipitation trends in cities.

  Statistical studies of solar activity with weather and climate were particularly popular until the 1980s, when publications blossomed with studies of weather fronts and global meteorological patterns. Photos from space and weather satellites emphasized the importance of clouds and weather fronts. Climate studies and weather forecasting have been enhanced by increasing use of climate models, beginning with simple computer simulations and replacing "solar constant" values with more detailed solar variation as computing power increased and understanding of weather processes improves.

  See Also

  • Global dimming

  References

  1. ^  "Solar Forcing of Climate." Climate Change 2001: Working Group I: The Scientific Basis. Accessed on March 10, 2005.
  2. ^  "Changing Sun, Changing Climate?." The Discovery of Global Warming. Accessed on February 21, 2005.
  3. ^  Solanki, S.K., I.G. Usoskin, B. Kromer, M. Schussler and J. Beer (2004). "Unusual activity of the Sun during recent decades compared to the previous 11,000 years". Nature 431 (7012): 1084-1087. DOI:10.1038/nature02995 "11,000 Year Sunspot Number Reconstruction." Global Change Master Directory. Accessed on March 11, 2005.
  4. ^  Charles A. Perry and Kenneth J. Hsudagger (2000). "Geophysical, archaeological, and historical evidence support a solar-output model for climate change". PNAS 97 (23): 12433-12438. DOI:10.1073/pnas.230423297
  5. ^  "What the Sunspot Record Tells Us about Space Climate." Submitted to Solar Physics 2004/08/31. Accessed on March 11, 2005.
  6. ^  "SOLAR VARIABILITY: climatic change resulting from changes in the amount of solar energy reaching the upper atmosphere.." INTRODUCTION TO QUATERNARY ECOLOGY. Accessed on March 11, 2005.
  7. ^  Henrik Svensmark (1998). "Influence of Cosmic Rays on Earth's Climate". Physical Review Letters 81 (22): 5027-5030.
  8. ^  "Atmospheric Ionization and Clouds as Links Between Solar Activity and Climate." Tinsley, Brian A. and Fangqun Yu, in: Solar Variability and Its Effects on the Earth's Atmospheric and Climate System. Accessed on March 10, 2005. Judit M. Pap and Peter Fox (2004). Solar Variability and Its Effects on the Earth's Atmospheric and Climate System. American Geophysical Union. ISBN 0-87590-406-8.
  9. ^  E. Pallé, C.J. Butler, K. O'Brien (2004). "The possible connection between ionization in the atmosphere by cosmic rays and low level clouds". Journal of Atmospheric and Solar-Terrestrial Physics 66 (18): 1779-1720. DOI:10.1016/j.jastp.2004.07.041
  10. ^  Pallé, E. (2005). "Possible satellite perspective effects on the reported correlations between solar activity and clouds". Geophys. Res. Lett. 32 (3): L03802. DOI:10.1029/2004GL021167
  11. ^  "Variations in CO2 Growth Rate Associated with Solar Activity." Still Waiting for Greenhouse. Accessed on March 10, 2005.
  • C. G. Abbot (1966). "SOLAR VARIATION, A WEATHER ELEMENT". Proc Natl Acad Sci U S A. 56 (6): 1627-1634.
  • "The Sun and Climate." U.S. Geological Survey Fact Sheet 0095-00. Accessed on February 21, 2005.
  • "The Sun's role in Climate Changes." Proc. of The International Conference on Global Warming and The Next Ice Age, 19-24 August, 2001, Halifax, Nova Scotia.. Accessed on February 21, 2005.
  • Warren B. White, Judith Lean, Daniel R. Cayan and Michael D. Dettinger (1997). "Response of global upper ocean temperature to changing solar irradiance". J. Geophys. Res. 102 (C2): 3255-3266.

  External links

  • Gerrit Lohmann, Norel Rimbu, Mihai Dima (2004). Climate signature of solar irradiance variations: analysis of long-term instrumental, historical, and proxy data. International Journal of Climatology 24(8), 1045-1056 - Abstract: http://www.palmod.uni-bremen.de/~gerrit/abstractSolar.html
  • Solar Climatic Effects (Recent Influence) — Summary. Center for the Study of Carbon Dioxide and Global Change. 19 March 2003. http://www.co2science.org/subject/s/summaries/solarrecin.htm
  • NOAA / NESDIS / NGDC (2002) Solar Variability Affecting Earth NOAA CD-ROM NGDC-05/01. This CD-ROM contains over 100 solar-terrestrial and related global data bases covering the period through April 1990. http://www.ngdc.noaa.gov/stp/CDROM/solar_variability.html
  • S.K Solanski, M. Fligge (2001) Long-term changes in solar irradiance ESA SP-463, ESA Publications Division. http://www.astro.phys.ethz.ch/papers/fligge/solspa_2.pdf
  • S.K. Solanki, M. Fligge (2000) Reconstruction of past solar irradiance Space Science Review 94, 127-138 http://www.astro.phys.ethz.ch/papers/fligge/solfli_rev.pdf
  • George C. Reid (1995) The sun-climate question: Is there a real connection? Aeronomy Laboratory, NOAA/ERL, Boulder, Colorado. U.S. National Report to IUGG, 1991-1994 Rev. Geophys. Vol. 33 Suppl. http://www.agu.org/revgeophys/reid00/reid00.html

  In a barotropic atmosphere the geostrophic wind is independent of height.

  See also: Solar variation, 1040, 1080