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The Ionospheric Connection Explorer (ICON) is a planned satellite designed to investigate changes in the Earth's ionosphere. ICON will study the interaction between Earth's weather systems and space weather driven by the Sun, and how this interaction drives turbulence in the upper atmosphere. It is hoped that a better understanding of this dynamic will mitigate its effects on communications, GPS signals, and technology in general. It is part of NASA's Explorers program and will be operated by UC Berkeley's Space Sciences Laboratory.
On 12 April 2013, NASA announced that ICON, along with Global-scale Observations of the Limb and Disk (GOLD), had been selected for development with the cost capped at US$200 million, excluding launch costs. The principal investigator of ICON is Thomas Immel at the University of California, Berkeley.
ICON was originally scheduled to launch in December 2017 and has been repeatedly delayed because of problems with its Pegasus XL rocket. Most recently, it was due to launch on 26 October 2018 but the launch was postponed to 7 November 2018.
Once launched, ICON will perform a two-year mission to observe conditions in both the thermosphere and ionosphere. ICON will be equipped with four instruments: a Michelson interferometer, built by the United States Naval Research Laboratory, will measure the winds and temperatures in the thermosphere; an ion drift meter, built by UT Dallas, will measure the motion of charged particles in the ionosphere; and two ultraviolet imagers built at UC Berkeley will observe the airglow layers in the upper atmosphere in order to determine both ionospheric and thermospheric density and composition.
Many low-Earth orbiting satellites, including the International Space Station, fly through the ionosphere and can be affected by its changing electric and magnetic fields. The ionosphere also acts as a conduit for many communications signals, such as radio waves and the signals that make GPS systems work. The ionosphere is where space weather manifests, creating unpredicted conditions such as electric currents that can cause electrical charging of satellites, changing density that can affect satellite orbits, and shifting magnetic fields that can induce current in power systems, causing strain, disrupt communications and navigation or even blackouts. Improved understanding of this environment can help predict such events and improve satellite design.
Source (copy/paste due to lack of time):
- https://en.wikipedia.org/wiki/Ionospheric_Connection_Explorer
On 12 April 2013, NASA announced that ICON, along with Global-scale Observations of the Limb and Disk (GOLD), had been selected for development with the cost capped at US$200 million, excluding launch costs. The principal investigator of ICON is Thomas Immel at the University of California, Berkeley.
ICON was originally scheduled to launch in December 2017 and has been repeatedly delayed because of problems with its Pegasus XL rocket. Most recently, it was due to launch on 26 October 2018 but the launch was postponed to 7 November 2018.
Once launched, ICON will perform a two-year mission to observe conditions in both the thermosphere and ionosphere. ICON will be equipped with four instruments: a Michelson interferometer, built by the United States Naval Research Laboratory, will measure the winds and temperatures in the thermosphere; an ion drift meter, built by UT Dallas, will measure the motion of charged particles in the ionosphere; and two ultraviolet imagers built at UC Berkeley will observe the airglow layers in the upper atmosphere in order to determine both ionospheric and thermospheric density and composition.
Many low-Earth orbiting satellites, including the International Space Station, fly through the ionosphere and can be affected by its changing electric and magnetic fields. The ionosphere also acts as a conduit for many communications signals, such as radio waves and the signals that make GPS systems work. The ionosphere is where space weather manifests, creating unpredicted conditions such as electric currents that can cause electrical charging of satellites, changing density that can affect satellite orbits, and shifting magnetic fields that can induce current in power systems, causing strain, disrupt communications and navigation or even blackouts. Improved understanding of this environment can help predict such events and improve satellite design.
Source (copy/paste due to lack of time):
- https://en.wikipedia.org/wiki/Ionospheric_Connection_Explorer