Search engine for discovering works of Art, research articles, and books related to Art and Culture
ShareThis
Javascript must be enabled to continue!

The ESA M7 Plasma Observatory mission

View through CrossRef
The Magnetospheric System is the highly dynamic plasma environment where the strongest energization and energy transport occurs in near-Earth space.  Previous multi-point observations from missions such as ESA/Cluster and NASA/MMS have evidenced the fundamental role for these processes of cross-scales coupling . In the Magnetospheric System, the electromagnetic energy is converted into energized particles and energy is transported mainly at the ion and fluid scales. Simultaneous measurements at both large, fluid and small, kinetic scales are required to resolve scale coupling and ultimately fully understand plasma energization and energy transport processes. Here, we present the Plasma Observatory (PO) multi-scale mission concept tailored to study plasma energization and energy transport in the Earth's Magnetospheric System through with the first simultaneous in situ measurements at both fluid and ion scales. PO baseline mission includes one mothercraft (MSC) and six identical smallsat daughtercraft (DSC) in a two tetrahedra formation with MSC at the common vertex for both tetrahedra. PO baseline orbit is an HEO 8x17 RE orbit, covering all the key regions of the Magnetospheric System including the foreshock, the bow shock, the magnetosheath, the magnetopause, the transition region and the current sheet. Spacecraft separation ranges from fluid (5000 km) to ion (30 km) scales. The MSC payload provides a complete characterization of electromagnetic fields and particles in a single point with time resolution sufficient to resolve kinetic physics at sub-ion scales and fully characterize wave-particle interactions. The DSCs have identical payload, simpler than the MSC payload, yet giving a full characterization of the plasma at the ion and fluid scales and providing the context where energization and transport occurs. PO is the next logical step after Cluster and MMS and will allow us to resolve for the first time scale coupling in  the Earth's Magnetospheric System, leading to transformative advances in the field of space plasma physics. Plasma Observatory  is one of the three ESA M7 candidates, which have been selected in November 2023 for a competitive Phase A with a mission selection planned in 2026 and launch in 2037.  
Title: The ESA M7 Plasma Observatory mission
Description:
The Magnetospheric System is the highly dynamic plasma environment where the strongest energization and energy transport occurs in near-Earth space.
  Previous multi-point observations from missions such as ESA/Cluster and NASA/MMS have evidenced the fundamental role for these processes of cross-scales coupling .
In the Magnetospheric System, the electromagnetic energy is converted into energized particles and energy is transported mainly at the ion and fluid scales.
Simultaneous measurements at both large, fluid and small, kinetic scales are required to resolve scale coupling and ultimately fully understand plasma energization and energy transport processes.
Here, we present the Plasma Observatory (PO) multi-scale mission concept tailored to study plasma energization and energy transport in the Earth's Magnetospheric System through with the first simultaneous in situ measurements at both fluid and ion scales.
PO baseline mission includes one mothercraft (MSC) and six identical smallsat daughtercraft (DSC) in a two tetrahedra formation with MSC at the common vertex for both tetrahedra.
PO baseline orbit is an HEO 8x17 RE orbit, covering all the key regions of the Magnetospheric System including the foreshock, the bow shock, the magnetosheath, the magnetopause, the transition region and the current sheet.
Spacecraft separation ranges from fluid (5000 km) to ion (30 km) scales.
The MSC payload provides a complete characterization of electromagnetic fields and particles in a single point with time resolution sufficient to resolve kinetic physics at sub-ion scales and fully characterize wave-particle interactions.
The DSCs have identical payload, simpler than the MSC payload, yet giving a full characterization of the plasma at the ion and fluid scales and providing the context where energization and transport occurs.
PO is the next logical step after Cluster and MMS and will allow us to resolve for the first time scale coupling in  the Earth's Magnetospheric System, leading to transformative advances in the field of space plasma physics.
Plasma Observatory  is one of the three ESA M7 candidates, which have been selected in November 2023 for a competitive Phase A with a mission selection planned in 2026 and launch in 2037.
  .

Related Results

Magnetohydrodynamics enhanced radio blackout mitigation system for spacecraft during planetary entries
Magnetohydrodynamics enhanced radio blackout mitigation system for spacecraft during planetary entries
(English) Spacecraft entering planetary atmospheres are enveloped by a plasma layer with high levels of ionization, caused by the extreme temperatures in the shock layer. The charg...
Concepts for a German Small Sat Mission to (99942) Apophis
Concepts for a German Small Sat Mission to (99942) Apophis
Due to the increased performance of small satellites, their use in the exploration of asteroids is becoming increasingly more important. The DART mission with the CubeSat LICIACube...
The ESA M7 candidate mission Plasma Observatory.
The ESA M7 candidate mission Plasma Observatory.
Particle energization and transport of energy are key open problems of space plasma physics. Their comprehension has implications on research fields that span from space weather to...
Astronomical research in Kharkiv at the end of the 19th century – the first half of the 20th century
Astronomical research in Kharkiv at the end of the 19th century – the first half of the 20th century
The main milestones of the formation and development of astronomical science in Kharkiv during 1883–1945 are reconstructed on the example of the activities of the astronomical obse...
Fieldwork teaching on Mars using a Large-Scale Visualisation System
Fieldwork teaching on Mars using a Large-Scale Visualisation System
Recent orbital and rover images of the surface of Mars provide exceptional high-resolution views of the martian landscapes and its surface geology. These extensive datasets provide...
ExoMars/Rosalind Franklin Mission Update
ExoMars/Rosalind Franklin Mission Update
Finding signs of life elsewhere is one of the most important scientific objectives of our time.From the very beginning in 2002, ExoMars was conceived to answer one question:&#1...
Keyhole-Based Site Selection for Kinetic Impact Deflection of Near-Earth Asteroids
Keyhole-Based Site Selection for Kinetic Impact Deflection of Near-Earth Asteroids
Given present-day asteroid discovery capabilities, near-Earth asteroids (NEAs) are routinely discovered. 3,123 NEAs were discovered in 2024 alone1. Furthermore, new telescopes such...
A study of plasma treatments effects on dental biofilms
A study of plasma treatments effects on dental biofilms
[ACCESS RESTRICTED TO THE UNIVERSITY OF MISSOURI AT REQUEST OF AUTHOR.] Dental plaque is a biofilm that grows on surfaces within the mouth and contains millions of bacteria. The ba...

Back to Top