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  2. Ionospheric storm - Wikipedia

    en.wikipedia.org/wiki/Ionospheric_storm

    Ionospheric storms are storms which contain varying densities [1] of energised electrons in the ionosphere as produced from the Sun. Ionospheric storms are caused by geomagnetic storms. [2] They are categorised into positive and negative storms, where positive storms have a high density of electrons and negative storms contain a lower density ...

  3. List of Solar System objects by size - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System...

    Parts-per-million chart of the relative mass distribution of the Solar System, each cubelet denoting 2 × 10 24 kg. This article includes a list of the most massive known objects of the Solar System and partial lists of smaller objects by observed mean radius. These lists can be sorted according to an object's radius and mass and, for the most ...

  4. List of solar storms - Wikipedia

    en.wikipedia.org/wiki/List_of_solar_storms

    Comparable in size to the May 2024 storms. [46] Oct 1903 Solar storm of Oct-Nov 1903 An extreme storm, estimated at Dst −531 nT arose from a fast CME (mean ≈1500 km/s), occurred during the ascending phase of the minimum of the relatively weak solar cycle 14, which is the most significant storm on record in a solar minimum period. Aurora was ...

  5. The largest storm in our solar system is moving unexpectedly ...

    www.aol.com/news/hubble-images-show-jupiter...

    The insights gathered through the program’s observations of the largest storms in our solar system can help scientists understand what weather may be like on exoplanets orbiting other stars.

  6. Solar System model - Wikipedia

    en.wikipedia.org/wiki/Solar_System_model

    The properly-scaled, basket-ball-sized model is 1.3 miles (2.14 km) from the model Sun which is located at the museum, graphically illustrating the immense empty space in the Solar System. The objects in such large models do not move.

  7. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    The Solar System remains in a relatively stable, slowly evolving state by following isolated, gravitationally bound orbits around the Sun. [28] Although the Solar System has been fairly stable for billions of years, it is technically chaotic, and may eventually be disrupted. There is a small chance that another star will pass through the Solar ...

  8. Ionosphere - Wikipedia

    en.wikipedia.org/wiki/Ionosphere

    The worldwide solar-driven wind results in the so-called Sq (solar quiet) current system in the E region of the Earth's ionosphere (ionospheric dynamo region) (100–130 km (60–80 mi) altitude). [citation needed] Resulting from this current is an electrostatic field directed west–east (dawn–dusk) in the equatorial day side of the ionosphere.

  9. Sagan Planet Walk - Wikipedia

    en.wikipedia.org/wiki/Sagan_Planet_Walk

    The Sagan Planet Walk has inspired the creation of other scale-model Solar Systems in the United States. The Delmar Loop Planet Walk in St. Louis, Missouri: "In 2006, I became aware of the Sagan Planet Walk in Ithaca, NY, and as an amateur astronomy buff, I found the idea of a scale model solar system to be a fascinating concept.