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SUNSPOT NUMBER

  • Sunspot number
  • Measure of sunspot activity

    Wolf number (also known as the relative sunspot number or Zürich number) is a quantity that measures the number of sunspots and groups of sunspots present

    Sunspot number

    Sunspot number

    Sunspot_number

  • Sunspot
  • Temporary spots on the Sun's surface

    that inhibit convection. Sunspots appear within active regions, usually in pairs of opposite magnetic polarity. Their number varies according to the approximately

    Sunspot

    Sunspot

    Sunspot

  • Solar cycle
  • Periodic change in the Sun's activity

    activity cycle, sunspot cycle, or Schwabe cycle, is a periodic 11-year change in the Sun's activity measured in terms of variations in the number of observed

    Solar cycle

    Solar cycle

    Solar_cycle

  • Solar cycle 10
  • Solar activity from December 1855 to March 1867

    sunspot activity began. The solar cycle lasted 11.3 years, beginning in December 1855 and ending in March 1867. The maximum smoothed sunspot number observed

    Solar cycle 10

    Solar cycle 10

    Solar_cycle_10

  • Solar cycle 25
  • Solar activity from 2019 to about 2030

    when extensive recording of solar sunspot activity began. It began in December 2019 with a minimum smoothed sunspot number of 1.8. It is expected to continue

    Solar cycle 25

    Solar cycle 25

    Solar_cycle_25

  • Maunder Minimum
  • Period of low solar activity, 1645–1715

    Minimum, also known as the "prolonged sunspot minimum", was a period around 1645 to 1715 during which sunspots became exceedingly rare. During the 28-year

    Maunder Minimum

    Maunder Minimum

    Maunder_Minimum

  • Dalton Minimum
  • Period of low solar activity from 1790 to 1830

    is often compared with the Maunder Minimum, its sunspot number was slightly higher and reported sunspots distributed in both solar hemispheres unlike the

    Dalton Minimum

    Dalton Minimum

    Dalton_Minimum

  • Solar cycle 23
  • Solar activity from August 1996 to December 2008

    sunspot activity began. The solar cycle lasted 12.6 years, beginning in August 1996 and ending in December 2008. The maximum smoothed sunspot number observed

    Solar cycle 23

    Solar cycle 23

    Solar_cycle_23

  • Sun
  • Star at the centre of the Solar System

    field, and sunspots diminish in number and size. At solar-cycle minimum, the toroidal field is, correspondingly, at minimum strength, sunspots are relatively

    Sun

    Sun

    Sun

  • Solar cycle 15
  • Solar activity from July 1913 to August 1923

    solar sunspot activity began. The solar cycle lasted 10.1 years, beginning in July 1913 and ending in August 1923. The maximum smoothed sunspot number observed

    Solar cycle 15

    Solar cycle 15

    Solar_cycle_15

  • Solar maximum
  • Regular period of greatest solar activity

    the Sun's 11-year solar cycle. During solar maximum, large numbers of sunspots appear, and the solar irradiance output grows by about 0.07%. On average

    Solar maximum

    Solar maximum

    Solar_maximum

  • Solar cycle 8
  • Solar activity from November 1833 to July 1843

    solar sunspot activity began. The solar cycle lasted 9.7 years, beginning in November 1833 and ending in July 1843. The maximum smoothed sunspot number observed

    Solar cycle 8

    Solar_cycle_8

  • Solar cycle 24
  • Solar activity from December 2008 to December 2019

    when extensive recording of solar sunspot activity began. It began in December 2008 with a minimum smoothed sunspot number of 2.2,[failed verification] and

    Solar cycle 24

    Solar cycle 24

    Solar_cycle_24

  • Solar cycle 11
  • Solar activity from March 1867 to December 1878

    sunspot activity began. The solar cycle lasted 11.8 years, beginning in March 1867 and ending in December 1878. The maximum smoothed sunspot number observed

    Solar cycle 11

    Solar cycle 11

    Solar_cycle_11

  • Solar cycle 20
  • Solar activity from October 1964 to March 1976

    solar sunspot activity began. The solar cycle lasted 11.4 years, beginning in October 1964 and ending in March 1976. The maximum smoothed sunspot number observed

    Solar cycle 20

    Solar cycle 20

    Solar_cycle_20

  • Solar cycle 18
  • Solar activity from February 1944 to April 1954

    sunspot activity began. The solar cycle lasted 10.2 years, beginning in February 1944 and ending in April 1954. The maximum smoothed sunspot number observed

    Solar cycle 18

    Solar_cycle_18

  • Solar cycle 16
  • Solar activity from August 1923 to September 1933

    sunspot activity began. The solar cycle lasted 10.1 years, beginning in August 1923 and ending in September 1933. The maximum smoothed sunspot number

    Solar cycle 16

    Solar cycle 16

    Solar_cycle_16

  • Coronal mass ejection
  • Ejecta from the Sun's corona

    maximum. However, the peak CME occurrence rate is often 6–12 months after sunspot number reaches its maximum. Only a small fraction of CMEs are directed toward

    Coronal mass ejection

    Coronal mass ejection

    Coronal_mass_ejection

  • Solar cycle 19
  • Solar activity from April 1954 to October 1964

    Year occurred at the peak of this solar cycle. The maximum smoothed sunspot number observed during the solar cycle was 285.0, in March 1958 (the highest

    Solar cycle 19

    Solar cycle 19

    Solar_cycle_19

  • Solar cycle 1
  • Solar activity from February 1755 to June 1766

    solar sunspot activity took place. The solar cycle lasted 11.3 years, beginning in February 1755 and ending in June 1766. The maximum smoothed sunspot number

    Solar cycle 1

    Solar cycle 1

    Solar_cycle_1

  • Solar cycle 14
  • Solar activity from January 1902 to July 1913

    solar sunspot activity began. The solar cycle lasted 11.5 years, beginning in January 1902 and ending in July 1913. The maximum smoothed sunspot number observed

    Solar cycle 14

    Solar cycle 14

    Solar_cycle_14

  • Solar cycle 5
  • Solar activity from April 1798 to August 1810

    1810 (thus falling within the Dalton Minimum). The maximum smoothed sunspot number observed during the solar cycle was 82.0, in February 1805 (the third-lowest

    Solar cycle 5

    Solar cycle 5

    Solar_cycle_5

  • Solar cycle 6
  • Solar activity from August 1810 to May 1823

    1823 (thus falling within the Dalton Minimum). The maximum smoothed sunspot number observed during the solar cycle was 81.2, in May 1816 (the lowest of

    Solar cycle 6

    Solar cycle 6

    Solar_cycle_6

  • Solar cycle 12
  • Solar activity from December 1878 to March 1890

    sunspot activity began. The solar cycle lasted 11.3 years, beginning in December 1878 and ending in March 1890. The maximum smoothed sunspot number observed

    Solar cycle 12

    Solar cycle 12

    Solar_cycle_12

  • Solar cycle 21
  • Solar activity from March 1976 to September 1986

    sunspot activity began. The solar cycle lasted 10.5 years, beginning in March 1976 and ending in September 1986. The maximum smoothed sunspot number observed

    Solar cycle 21

    Solar cycle 21

    Solar_cycle_21

  • Heliosphere
  • Region of space dominated by the Sun

    a change in the direction of the magnetic field, and an increase in the number of galactic cosmic rays. In May 2012, Voyager 1 detected a rapid increase

    Heliosphere

    Heliosphere

    Heliosphere

  • Solar observation
  • Study of the Sun's behavior

    thicker sediment deposits) could have occurred during years with greater sunspot activity. This would presume annual layering; however, alternative explanations

    Solar observation

    Solar_observation

  • Solar cycle 22
  • Solar activity from September 1986 to August 1996

    sunspot activity began. The solar cycle lasted 9.9 years, beginning in September 1986 and ending in August 1996. The maximum smoothed sunspot number observed

    Solar cycle 22

    Solar cycle 22

    Solar_cycle_22

  • Solar cycle 9
  • Solar activity from July 1843 to December 1855

    solar sunspot activity began. The solar cycle lasted 12.4 years, beginning in July 1843 and ending in December 1855. The maximum smoothed sunspot number observed

    Solar cycle 9

    Solar cycle 9

    Solar_cycle_9

  • Solar cycle 13
  • Solar activity from March 1890 to January 1902

    solar sunspot activity began. The solar cycle lasted 11.8 years, beginning in March 1890 and ending in January 1902. The maximum smoothed sunspot number observed

    Solar cycle 13

    Solar cycle 13

    Solar_cycle_13

  • Solar cycle 17
  • Solar activity from September 1933 to February 1944

    solar sunspot activity began. The solar cycle lasted 10.4 years, beginning in September 1933 and ending in February 1944. The maximum smoothed sunspot number

    Solar cycle 17

    Solar_cycle_17

  • Solar cycle 7
  • Solar activity from May 1823 to November 1833

    November 1833 (thus overlapping the Dalton Minimum). The maximum smoothed sunspot number observed during the solar cycle was 119.2 (November 1829), and the starting

    Solar cycle 7

    Solar cycle 7

    Solar_cycle_7

  • Solar phenomena
  • Natural phenomena within the Sun's atmosphere

    radio wave flux, solar flares, coronal mass ejections, coronal heating and sunspots. These phenomena are believed to be generated by a helical dynamo, located

    Solar phenomena

    Solar phenomena

    Solar_phenomena

  • Letters on Sunspots
  • 1613 pamphlet by Galileo Galilei

    Letters on Sunspots (Istoria e Dimostrazioni intorno alle Macchie Solari) was a pamphlet written by Galileo Galilei in 1612 and published in Rome by the

    Letters on Sunspots

    Letters on Sunspots

    Letters_on_Sunspots

  • Solar cycle 2
  • Solar activity from June 1766 to June 1775

    recording of sunspot activity began. The solar cycle lasted 9 years, beginning in June 1766 and ending in June 1775. The maximum smoothed sunspot number observed

    Solar cycle 2

    Solar cycle 2

    Solar_cycle_2

  • Modern Maximum
  • Period of high solar activity beginning in 1914

    PMID 15510145. S2CID 4373732. Retrieved 17 April 2007., "11,000 Year Sunspot Number Reconstruction". Global Change Master Directory. Retrieved 2005-03-11

    Modern Maximum

    Modern Maximum

    Modern_Maximum

  • Little Ice Age
  • Climatic cooling after the Medieval Warm Period (16th–19th centuries)

    emissions. Solar activity includes any disturbances on the Sun such as sunspots and solar flares associated with the variable magnetic field of the solar

    Little Ice Age

    Little Ice Age

    Little_Ice_Age

  • Solar activity and climate
  • Field of scientific study

    1970s is estimated using proxy variables, such as tree rings, the number of sunspots, and the abundances of cosmogenic isotopes such as 10Be, all of which

    Solar activity and climate

    Solar activity and climate

    Solar_activity_and_climate

  • Solar cycle 3
  • Solar activity from June 1775 to September 1784

    solar sunspot activity began. The solar cycle lasted 9.3 years, beginning in June 1775 and ending in September 1784. The maximum smoothed sunspot number observed

    Solar cycle 3

    Solar cycle 3

    Solar_cycle_3

  • Crangon crangon
  • Species of shrimp

    closely correlated with the mean annual Zürich sunspot number for the period 1965-1975. Given that sunspot numbers are predictable, this provides another

    Crangon crangon

    Crangon crangon

    Crangon_crangon

  • Sunspot drawing
  • Sunspot drawing or sunspot sketching is the act of drawing sunspots. Sunspots are darker spots on the Sun's photosphere. Their prediction is very important

    Sunspot drawing

    Sunspot drawing

    Sunspot_drawing

  • Sunspots (economics)
  • Extrinsic random variable not affecting economic fundamentals

    In economics, the term sunspots (or sometimes "a sunspot") refers to an extrinsic random variable, that is, a random variable that does not affect economic

    Sunspots (economics)

    Sunspots_(economics)

  • Superflare
  • Strong explosion observed on stars

    Both measures agree reasonably with each other and with the Zurich sunspot number of the last two centuries. As an additional check, it is possible to

    Superflare

    Superflare

    Superflare

  • Solar minimum
  • Regular period of least solar activity

    solar activity in the Sun's 11-year solar cycle. During solar minimum, sunspot and solar flare activity diminishes, and often does not occur for days

    Solar minimum

    Solar minimum

    Solar_minimum

  • Skywave
  • Propagation of radio waves beyond the radio horizon

    usable frequency for skywave propagation is strongly influenced by sunspot number. Skywave propagation is usually degraded – sometimes seriously – during

    Skywave

    Skywave

    Skywave

  • Solar cycle 4
  • Solar activity from September 1784 to April 1798

    April 1798 (thus overlapping the Dalton Minimum). The maximum smoothed sunspot number observed during the solar cycle was 235.3 (in February 1788), and the

    Solar cycle 4

    Solar_cycle_4

  • Convection zone
  • Region of a star

    cycle List of solar cycles Active region Solar maximum Solar minimum Sunspot number Solar wind Solar wind turbulence Magnetic switchback Flare Helioseismology

    Convection zone

    Convection zone

    Convection_zone

  • Space weather
  • Branch of space physics and aeronomy

    occurrence of geomagnetic storms on Earth was correlated with the number of sunspots, demonstrating a novel solar-terrestrial interaction. The solar storm

    Space weather

    Space weather

    Space_weather

  • Beryllium
  • Chemical element with atomic number 4 (Be)

    Beryllium is a chemical element; it has symbol Be and atomic number 4. It is a steel-gray, hard, strong, lightweight and brittle alkaline earth metal.

    Beryllium

    Beryllium

    Beryllium

  • Solar core
  • Central region of the Sun

    able to escape the Sun immediately. For many years measurements of the number of neutrinos produced in the Sun were much lower than theories predicted

    Solar core

    Solar core

    Solar_core

  • Radiative zone
  • Region of a star

    cycle List of solar cycles Active region Solar maximum Solar minimum Sunspot number Solar wind Solar wind turbulence Magnetic switchback Flare Helioseismology

    Radiative zone

    Radiative_zone

  • Solar prominence
  • Structure extending off of the Sun's surface

    prominence is primarily used to refer to larger and cooler features. There are a number of different prominence classification schemes in use today. One of the

    Solar prominence

    Solar prominence

    Solar_prominence

  • Louis Miles Muggleton
  • British physicist and electrical engineer

    E-region peak electron density, N m ( E ) {\displaystyle N_{m}(E)} , and sunspot number, R {\displaystyle R} , depend on the particular solar cycle investigated

    Louis Miles Muggleton

    Louis Miles Muggleton

    Louis_Miles_Muggleton

  • Numbers station
  • Shortwave radio stations broadcasting only numbers

    all reception conditions (such as sunspot cycles and seasonal static). However, in the field low-tech spoken number transmissions continue to have advantages

    Numbers station

    Numbers_station

  • Solar rotation
  • Differential rotation of the Sun

    face is called West. Therefore, sunspots are said to move across the Sun's face from east to west. Bartels' rotation number is a serial count that numbers

    Solar rotation

    Solar rotation

    Solar_rotation

  • Joan Feynman
  • American astrophysicist (1927–2020)

    predicts the number of high-energy particles likely to hit a spacecraft over its lifetime, and uncovered a method for predicting sunspot cycles. She was

    Joan Feynman

    Joan Feynman

    Joan_Feynman

  • Crackling noise
  • N=10^{a-bM}} Gutenberg–Richter law shows an inverse power relation between the number of earthquakes occurring N and its magnitude M with a proportionality constant

    Crackling noise

    Crackling noise

    Crackling_noise

  • Jean Maud Bullen
  • New Zealand-born geophysicist

    modifying influence on linear trend of F-region electron density with sunspot number. Nature, 192(4802), 542-543. "Junior Scholarships". paperspast.natlib

    Jean Maud Bullen

    Jean_Maud_Bullen

  • Hisako Koyama
  • Japanese solar observer

    whose multidecade collection of detailed sunspot sketches played a role in reconstructing a continuous sunspot record dating back to 1610. Koyama worked

    Hisako Koyama

    Hisako_Koyama

  • Index of radio propagation articles
  • stratosphere - substorm - sudden ionospheric disturbance (SID) - sunspot - sunspot cycle - sunspot number - super high frequency (SHF) - supergranulation - surface

    Index of radio propagation articles

    Index_of_radio_propagation_articles

  • Heinrich Schwabe
  • German astronomer (1789–1875)

    on sunspots. He observed sunspots and made drawings of them from 1825 to 1867 and suggested in 1838 that there may be a ten-year cycle of sunspot activity

    Heinrich Schwabe

    Heinrich Schwabe

    Heinrich_Schwabe

  • Mathew Owens
  • British physicist

    10 November 2017. Retrieved 14 October 2019. "Recalibration of the Sunspot Number Series | ISSI Team led by Mathew Owens & Frederic Clette (UK)". Retrieved

    Mathew Owens

    Mathew Owens

    Mathew_Owens

  • Ilya G. Usoskin
  • Finnish Astrophysicist

    Manfred; Mursula, Kalevi; Alanko, Katja (2003), "A Millennium Scale Sunspot Number Reconstruction: Evidence For an Unusually Active Sun Since the 1940s"

    Ilya G. Usoskin

    Ilya G. Usoskin

    Ilya_G._Usoskin

  • Timeline of solar astronomy
  • his discovery of the sunspot cycle and estimates its period to be about a decade 1852 — Edward Sabine shows that sunspot number is correlated with geomagnetic

    Timeline of solar astronomy

    Timeline_of_solar_astronomy

  • Common sunflower
  • Species of flowering plant

    Arnika Autumn Beauty Aztec Sun Black Oil Chianti Hybrid Claret agm Dwarf Sunspot Evening Sun Florenza Giant Primrose Gullick's Variety agm Incredible Indian

    Common sunflower

    Common sunflower

    Common_sunflower

  • Night Moves (album)
  • 1976 studio album by Bob Seger & the Silver Bullet Band

    Rhythm Section at Muscle Shoals Sound Studios in Sheffield, Alabama. Track numbering below refers to CD and digital releases of the album. Erlewine, Stephen

    Night Moves (album)

    Night_Moves_(album)

  • Active region
  • Temporary region on the Sun

    associated with sunspots and are commonly the source of violent eruptions such as coronal mass ejections and solar flares. The number and location of

    Active region

    Active_region

  • Alfvén surface
  • Boundary between solar corona and wind

    Charles W. (January 2014). "An analysis of Alfvén radius based on sunspot number from 1749 to today". Journal of Geophysical Research: Space Physics

    Alfvén surface

    Alfvén surface

    Alfvén_surface

  • Sami Solanki
  • Astronomer

    Manfred; Mursula, Kalevi; Alanko, Katja (2003), "A Millennium Scale Sunspot Number Reconstruction: Evidence For an Unusually Active Sun Since the 1940s"

    Sami Solanki

    Sami Solanki

    Sami_Solanki

  • Hale's law
  • Empirical law for solar active regions

    active regions have the opposite leading polarity; and that, from one sunspot cycle to the next, these polarities reverse. It is named after George Ellery

    Hale's law

    Hale's law

    Hale's_law

  • List of solar cycles
  • periodic 11-year changes in the Sun's activity that are based on the number of sunspots present on the Sun's surface. The first solar cycle conventionally

    List of solar cycles

    List_of_solar_cycles

  • Solar flare
  • Eruption of electromagnetic radiation

    radio waves to gamma rays. Flares occur in active regions, often around sunspots, where intense magnetic fields penetrate the photosphere to link the corona

    Solar flare

    Solar flare

    Solar_flare

  • William Stanley Jevons
  • English economist and logician (1835–1882)

    presented a statistical study relating business cycles with sunspots. His reasoning was that sunspots affected the weather, which, in turn, affected crops.

    William Stanley Jevons

    William Stanley Jevons

    William_Stanley_Jevons

  • Rudolf Wolf
  • Swiss astronomer and mathematician (1816–1893)

    cycle of 11.1 years. In 1848 he devised a way of quantifying sunspot activity. The Wolf number, as it is now called, remains in use. In 1852 Wolf was one

    Rudolf Wolf

    Rudolf Wolf

    Rudolf_Wolf

  • Galileo Galilei
  • Italian physicist and astronomer (1564–1642)

    four largest satellites of Jupiter, Saturn's rings, lunar craters, and sunspots. He also built an early microscope. Galileo's championing of Copernican

    Galileo Galilei

    Galileo Galilei

    Galileo_Galilei

  • Speckled wood (butterfly)
  • Species of butterfly in the family Nymphalidae

    through the canopy. The males often remain in the same sunspot until the evening, following the sunspot as it moves across the forest floor. The males often

    Speckled wood (butterfly)

    Speckled wood (butterfly)

    Speckled_wood_(butterfly)

  • Sebastian Shaw (character)
  • Marvel Comics supervillain

    and is replaced by Sunspot, who becomes Lord Imperial of the Hellfire Club. Shaw attends a Hellfire Club dinner hosted by Sunspot and is alerted to a

    Sebastian Shaw (character)

    Sebastian_Shaw_(character)

  • Airglow
  • Faint emission of light by a planetary atmosphere

    self-illuminated gases and has no relationship with Earth's magnetism or sunspot activity, causing aurorae. Airglow occurs in two forms, as a result of

    Airglow

    Airglow

    Airglow

  • Alexander Chizhevsky
  • Russian interdisciplinary scientist (1897–1964)

    Chizhevsky proposed that not only did geomagnetic storms resulting from sunspot-related solar flares affect electrical usage, plane crashes, epidemics

    Alexander Chizhevsky

    Alexander Chizhevsky

    Alexander_Chizhevsky

  • Hellfire Club (comics)
  • Fictional society in the Marvel Comics universe

    gravely injured, and Sunspot takes over as Lord Imperial, which was Tessa's plan all along. Tessa left the Club, still under Sunspot's rule, and joined New

    Hellfire Club (comics)

    Hellfire_Club_(comics)

  • Solar dynamo
  • Physical process that generates a star's magnetic field

    solar cycle, characterized by an increasing and decreasing number and size of sunspots. Sunspots are visible as dark patches on the Sun's photosphere and

    Solar dynamo

    Solar_dynamo

  • William Herschel
  • German-British astronomer and composer (1738–1822)

    low number of sunspots and lower yields explaining recurring booms and slumps in the economy. Herschel's speculation on a connection between sunspots and

    William Herschel

    William Herschel

    William_Herschel

  • Sun in fiction
  • harbingers of social upheaval. Sunspots, and their 11-year cycle of frequency in occurrence, appear in a small number of works. The Sun poses a danger

    Sun in fiction

    Sun in fiction

    Sun_in_fiction

  • X-Men '97
  • Marvel Studios animated series

    Johnston voices young Nathan Summers. Gui Agustini as Roberto da Costa / Sunspot: A young mutant rescued by the X-Men who can channel solar energy. Naoko

    X-Men '97

    X-Men '97

    X-Men_'97

  • Richard Christopher Carrington
  • English astronomer (1826–1875)

    electrical influence upon the Earth and its aurorae; and whose 1863 records of sunspot observations revealed the differential rotation of the Sun. Carrington

    Richard Christopher Carrington

    Richard Christopher Carrington

    Richard_Christopher_Carrington

  • List of cycles
  • Orbital period – Saros cycle – Sothic cycle – Secularity – Sidereal year – Sunspot – Tide – Tropical year – Year Animal migration – Avalanche – Carbon cycle

    List of cycles

    List_of_cycles

  • George Ellery Hale
  • American solar astronomer (1868–1938)

    American astrophysicist best known for his discovery of magnetic fields in sunspots. He was also a key figure in the planning and construction of several world-leading

    George Ellery Hale

    George Ellery Hale

    George_Ellery_Hale

  • Babcock model
  • Mechanism explaining sunspot patterns

    explain magnetic and sunspot patterns observed on the Sun. It is named after Horace W. Babcock. The modern understanding of sunspots starts with George

    Babcock model

    Babcock_model

  • X-Men (film series)
  • American superhero film series

    N'Duka, Amanda (June 1, 2017). "'New Mutants': Henry Zaga Set To Play Sunspot In 'X-Men' Spinoff". Deadline Hollywood. Archived from the original on

    X-Men (film series)

    X-Men_(film_series)

  • Richard B. Dunn Solar Telescope
  • Optical telescope dedicated to observing the Sun

    spectroscopy. It is located at Sacramento Peak in Sunspot, New Mexico. It was the main telescope at the Sunspot Solar Observatory, operated by New Mexico State

    Richard B. Dunn Solar Telescope

    Richard B. Dunn Solar Telescope

    Richard_B._Dunn_Solar_Telescope

  • El Niño–Southern Oscillation
  • Global climate phenomenon

    PMID 11577233. Muñoz, Arsenio; Ojeda, Jorge; Sánchez-Valverde, Belén (2002). "Sunspot-like and ENSO/NAO-like periodicities in lacustrinelaminated sediments of

    El Niño–Southern Oscillation

    El Niño–Southern Oscillation

    El_Niño–Southern_Oscillation

  • Jean Tarde
  • French vicar general and scientist

    astronomy, physics, and geography. He is most famous for his work with sunspots which he concluded were small satellites of the sun. Jean Tarde belonged

    Jean Tarde

    Jean_Tarde

  • New Mexico State Road 6563
  • Highway in New Mexico

    State Road 6563 (NM 6563), also known as the Sunspot Scenic Byway, is a 15.530-mile-long (24.993 km) two-lane state highway in Otero County, New Mexico

    New Mexico State Road 6563

    New Mexico State Road 6563

    New_Mexico_State_Road_6563

  • May 2024 solar storms
  • Series of intense solar storms in 2024

    com. Archived from the original on 11 May 2024. Retrieved 11 May 2024. "Sunspot region 3664, major flares and CMEs!". SpaceWeatherLive. 8 May 2024. Archived

    May 2024 solar storms

    May 2024 solar storms

    May_2024_solar_storms

  • 145452 Ritona
  • Classical Kuiper belt object

    Becker, Andrew Puckett and Jeremy Kubica at Apache Point Observatory in Sunspot, New Mexico. Ritona has a measured diameter of 679+55 −73 km, which is

    145452 Ritona

    145452 Ritona

    145452_Ritona

  • Aurora
  • Atmospheric effect caused by the solar wind

    Large geomagnetic storms are most common during the peak of the 11-year sunspot cycle or during the three years after the peak. An electron spirals (gyrates)

    Aurora

    Aurora

    Aurora

  • 145451 Rumina
  • Scattered disc object

    Becker, Andrew Puckett and Jeremy Kubica at the Apache Point Observatory in Sunspot, New Mexico. It measures approximately 600 kilometers in diameter, and

    145451 Rumina

    145451 Rumina

    145451_Rumina

  • The Stranglers
  • English rock band

    was widely considered an artistic and commercial failure. The track "Two Sunspots" had been recorded during the Black And White sessions in 1978, but was

    The Stranglers

    The Stranglers

    The_Stranglers

  • List of X-Force members
  • the decades, X-Force have featured a rotating line up composed of large number of mutant characters. Notations: A slash (/) between names, indicates the

    List of X-Force members

    List_of_X-Force_members

  • List of Avengers members
  • List of all members of the avengers

    the decades, the Avengers are featured as a rotating line up of a large number of characters. According to various handbooks, members of the main team

    List of Avengers members

    List_of_Avengers_members

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