Creative Data Display with the Parker Solar Probe

The high-definition television of solar cameras, SDO takes movies of the Sun in different wavelengths of light (colors) and continuously sends them to the ground.

Main science page for the NASA Science Mission Directorate Heliophysics Division, which studies the Sun and how it influences the very nature of space — and, in turn, the atmospheres of planets.

Parker Solar Probe animation and graphics created by the SVS, based at NASA's Goddard Space Flight Center, in coordination with the Parker Solar Probe science team.

The CCMC is a multi-agency partnership to enable, support, and perform the research and development for next-generation space science and space weather models. The CCMC provides the international research community with access to modern space science simulations.

Among CCMC resources is the iNTEGRATED SPACE WEATHER ANALYSIS SYSTEM (iSWA), a flexible, turnkey, web-based dissemination system for NASA-relevant space weather information that combines forecasts based on the most advanced space weather models with concurrent space environment information. iSWA is customer-configurable and adaptable for use as a powerful decision-making tool. The system offers an unprecedented ability to analyze the present and expected future space weather impacts on NASA's human and robotic missions.

Parker Solar Probe mission science team website; includes access to actual instrument data and images, as well as orbit and instrument plans, schedules, and visualizations.

Data from one of the oldest space weather stations; ACE still provides data that we receive within minutes of when it is collected in space.

Data from the Canadian solar flux archive could help you find regions and time ranges that have interesting solar effects.

The Canadian Astronomy Data Centre archive contains imagery and other data of the sun from several missions. You could use these data to complement the Parker Solar Probe data.

INPE, developed among other activities also, has been researching the spatial phenomena, from the Sun, interplanetary space, and magnetosphere to the ionosphere, the upper and middle atmosphere, and geomagnetism since its inception in 1964. In addition to the constant and essential scientific research activity of geospatial phenomena is growing need for information on the Space Weather from the technological and socio-economic communities.

A neutron monitor is a ground-based detector designed to measure the number of high-energy charged particles striking the Earth's atmosphere from outer space based at Hermanus.