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  2. Solar rotation - Wikipedia

    en.wikipedia.org/wiki/Solar_rotation

    The "Carrington longitude" of the same feature refers to an arbitrary fixed reference point of an imagined rigid rotation, as defined originally by Richard Christopher Carrington. Carrington determined the solar rotation rate from low latitude sunspots in the 1850s and arrived at 25.38 days for the sidereal rotation period.

  3. Solar coordinate systems - Wikipedia

    en.wikipedia.org/wiki/Solar_coordinate_systems

    The Carrington heliographic coordinate system, established by Richard C. Carrington in 1863, rotates with the Sun at a fixed rate based on the observed rotation of low-latitude sunspots. It rotates with a sidereal period of exactly 25.38 days, which corresponds to a mean synodic period of 27.2753 days.

  4. Richard Christopher Carrington - Wikipedia

    en.wikipedia.org/wiki/Richard_Christopher_Carrington

    Richard Christopher Carrington (26 May 1826 – 27 November 1875) [2] was an English amateur astronomer whose 1859 astronomical observations demonstrated the existence of solar flares as well as suggesting their electrical influence upon the Earth and its aurorae; and whose 1863 records of sunspot observations revealed the differential rotation of the Sun.

  5. Carrington Event - Wikipedia

    en.wikipedia.org/wiki/Carrington_Event

    The Carrington Event was the most intense geomagnetic storm in recorded history, peaking on 1–2 September 1859 during solar cycle 10. It created strong auroral displays that were reported globally and caused sparking and even fires in telegraph stations. [ 1 ]

  6. Rotation period (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Rotation_period_(astronomy)

    Rotation period with respect to distant stars, the sidereal rotation period (compared to Earth's mean Solar days) Synodic rotation period (mean Solar day) Apparent rotational period viewed from Earth Sun [i] 25.379995 days (Carrington rotation) 35 days (high latitude) 25 d 9 h 7 m 11.6 s 35 d ~28 days (equatorial) [2] Mercury: 58.6462 days [3 ...

  7. Ionospheric storm - Wikipedia

    en.wikipedia.org/wiki/Ionospheric_storm

    The most intense ionospheric storm occurred in 1859, commonly named the “solar storm of 1859” or the “Carrington Event.” The Carrington Event was named after Richard Carrington , an English astronomer who observed the irregular sun activity [ 5 ] that occurred during the Carrington Event.

  8. Asteroid Samples Contain Building Blocks of Life - AOL

    www.aol.com/news/asteroid-samples-contain...

    Like all of the millions of other objects in the asteroid belt, it formed 4.5 billion years ago when our solar system was just accreting. But its loose, rubble-rich structure suggests that it was ...

  9. Timeline of solar astronomy - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_solar_astronomy

    1863 — Richard Carrington discovers the differential nature of solar rotation; 1868 — Pierre Janssen and Norman Lockyer discover an unidentified yellow line in solar prominence spectra and suggest it comes from a new element which they name "helium" 1893 — Edward Maunder discovers the 1645-1715 Maunder sunspot minimum