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Canadian Geospace Monitoring (CGSM) is a Canadian space science program that was initiated in 2005. CGSM is funded primarily by the Canadian Space Agency , and consists of networks of imagers, meridian scanning photometers , riometers, magnetometers , digital ionosondes , and High Frequency SuperDARN radars.
Presently, GPS TEC is monitored and distributed in real time from more than 360 stations maintained by agencies in many countries. Geoeffectiveness is a measure of how strongly space weather magnetic fields, such as coronal mass ejections, couple with the Earth's magnetic field.
Tip and cue systems utilize a network of satellites equipped with complementary sensor technologies to track moving objects in real-time. The method involves detecting a target with a primary sensor, such as an infrared or photographic sensor, which then cues secondary sensors on the same or other satellites for more detailed monitoring.
This orbit enables observations of the magnetosphere’s response to varying solar wind conditions from the full range of vantage points over time scales encompassing all space weather phenomena. Furthermore, this orbit allows scientific return 100% of the time from at least a single instrument and up to 83% of the time from all instruments ...
Animation of Advanced Composition Explorer's orbit viewed from the Sun Earth · Advanced Composition Explorer ACE in orbit around the Sun–Earth L 1 point. Advanced Composition Explorer (ACE or Explorer 71) is a NASA Explorer program satellite and space exploration mission to study matter comprising energetic particles from the solar wind, the interplanetary medium, and other sources.
Magnetic pulsations are extremely low frequency disturbances in the Earth's magnetosphere driven by its interactions with the solar wind. [1] These variations in the planet's magnetic field can oscillate for multiple hours when a solar wind driving force strikes a resonance. [2] This is a form of Kelvin–Helmholtz instability. [1]
A new SDK version has been developed in Java with JOGL referred to as WorldWind Java. The latest version (2.2.0) was released in August 2020. The latest version (2.2.0) was released in August 2020. This new version has an API -centric architecture with functionalities 'off-loaded' to modular components, leaving the API at the core.
Wind/ KONUS data was used to show, for the first time, that fast radio bursts may originate from magnetars, highlighted by NASA at Fast Radio Bursts on 4 November 2020. Wind / KONUS data helped provide evidence of the first giant flare in the nearby Sculptor Galaxy , highlighted by NASA at Giant Flare in Nearby Galaxy on 13 January 2021.