NASA has selected two groundbreaking space missions to advance towards flight design and launch, with one aimed at unlocking the mysteries of Earth's magnetosphere and the other focused on diagnosing the root causes of solar eruptions.
The CINEMA (Cross-scale Investigation of Earthβs Magnetotail and Aurora) mission concept has been chosen for Phase B development, a crucial step that involves planning, design, and mission operations. Led by principal investigator Robyn Millan from Dartmouth College, CINEMA seeks to investigate the complex flow of plasma energy into Earth's magnetosphere, which is characterized by unpredictable dynamics and drives phenomena such as fast plasma jets, global electrical current systems, and spectacular auroral displays.
By launching a constellation of nine small satellites in polar low Earth orbit, CINEMA aims to connect energetic activity in the large-scale magnetic structure to visible signatures like aurora in the ionosphere. The mission will utilize a combination of instruments, including an energetic particle detector, auroral imager, and magnetometer, to gather data that will improve our understanding of space weather events' impacts on humans and technology across the solar system.
The $28 million budget allocated for Phase B represents just a fraction of the total cost of the mission, which is expected to exceed $182.8 million. Launching as early as 2030, CINEMA aims to make critical breakthroughs in heliophysics research.
On the other hand, NASA has also selected the CMEx (Chromospheric Magnetism Explorer) mission for an extended Phase A study, which will assess and refine its design for potential future consideration. Led by principal investigator Holly Gilbert from the National Center for Atmospheric Research, CMEx seeks to diagnose lower layers of the Sun's chromosphere to understand the origin of solar eruptions and determine the magnetic sources of the solar wind.
Using proven UV spectropolarimetric instrumentation demonstrated during NASA's CLASP sub-orbital sounding rocket flight, CMEx aims to improve our understanding of the complex interplay between the Sun's atmosphere and its impact on space weather events. With an extended Phase A study costing $2 million for 12 months, CMEx is set to make significant contributions to the field of heliophysics research.
Both missions are poised to revolutionize our understanding of space weather events and their impacts on our planet and beyond. As NASA Acting Associate Flight Director Asal Naseri noted, "Space plays a role in just about everything we do," and these mission concepts have the potential to improve our ability to predict solar events that could harm satellites and astronauts near Earth, at the Moon, or Mars.
The CINEMA (Cross-scale Investigation of Earthβs Magnetotail and Aurora) mission concept has been chosen for Phase B development, a crucial step that involves planning, design, and mission operations. Led by principal investigator Robyn Millan from Dartmouth College, CINEMA seeks to investigate the complex flow of plasma energy into Earth's magnetosphere, which is characterized by unpredictable dynamics and drives phenomena such as fast plasma jets, global electrical current systems, and spectacular auroral displays.
By launching a constellation of nine small satellites in polar low Earth orbit, CINEMA aims to connect energetic activity in the large-scale magnetic structure to visible signatures like aurora in the ionosphere. The mission will utilize a combination of instruments, including an energetic particle detector, auroral imager, and magnetometer, to gather data that will improve our understanding of space weather events' impacts on humans and technology across the solar system.
The $28 million budget allocated for Phase B represents just a fraction of the total cost of the mission, which is expected to exceed $182.8 million. Launching as early as 2030, CINEMA aims to make critical breakthroughs in heliophysics research.
On the other hand, NASA has also selected the CMEx (Chromospheric Magnetism Explorer) mission for an extended Phase A study, which will assess and refine its design for potential future consideration. Led by principal investigator Holly Gilbert from the National Center for Atmospheric Research, CMEx seeks to diagnose lower layers of the Sun's chromosphere to understand the origin of solar eruptions and determine the magnetic sources of the solar wind.
Using proven UV spectropolarimetric instrumentation demonstrated during NASA's CLASP sub-orbital sounding rocket flight, CMEx aims to improve our understanding of the complex interplay between the Sun's atmosphere and its impact on space weather events. With an extended Phase A study costing $2 million for 12 months, CMEx is set to make significant contributions to the field of heliophysics research.
Both missions are poised to revolutionize our understanding of space weather events and their impacts on our planet and beyond. As NASA Acting Associate Flight Director Asal Naseri noted, "Space plays a role in just about everything we do," and these mission concepts have the potential to improve our ability to predict solar events that could harm satellites and astronauts near Earth, at the Moon, or Mars.