cross-scale and scope:

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CROSS-SCALE and SCOPE: The future in Space Plasma Physics Matt Taylor on behalf of Steve Schwartz, Masaki Fujimoto and the Cross-Scale and SCOPE Teams The Influence of Solar Variability on Geophysical and Heliospheric Phenomena 2009 ILWS Workshop, Itamambuca Eco Resort, Ubatuba beach, Brazil http://sci.esa.in t/crossscale http://www.cross- scale.org

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CROSS-SCALE and SCOPE:. The future in Space Plasma Physics. Matt Taylor on behalf of Steve Schwartz, Masaki Fujimoto and the Cross-Scale and SCOPE Teams. http://sci.esa.int/crossscale http://www.cross-scale.org. The Influence of Solar Variability on Geophysical and Heliospheric Phenomena - PowerPoint PPT Presentation

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Page 1: CROSS-SCALE and SCOPE:

CROSS-SCALE and SCOPE:The future in Space Plasma

PhysicsMatt Taylor

on behalf of Steve Schwartz, Masaki Fujimoto

and the Cross-Scale and SCOPE Teams

The Influence of Solar Variability on Geophysical and Heliospheric Phenomena 2009 ILWS Workshop, Itamambuca Eco Resort, Ubatuba beach, Brazil

http://sci.esa.int/crossscalehttp://www.cross-scale.org

Page 2: CROSS-SCALE and SCOPE:

AOGS 2009 ST06-A006

• Motivation• Science Questions• Science Overview

Shocks ReconnectionTurbulenceCoupling

• Cross-Scale• SCOPE• Next Steps

Outline

Page 3: CROSS-SCALE and SCOPE:

Plasma Universe

Page 4: CROSS-SCALE and SCOPE:

AOGS 2009 ST06-A006

Motivation

3 universal phenomena control plasmas

-Shocks-Reconnection-Turbulence

Responsible for-Particle Acceleration-Energy and momentum exchange-Transport

in astrophysical and laboratory plasmas

Page 5: CROSS-SCALE and SCOPE:

AOGS 2009 ST06-A006

Top-level Science Questions‣How do shocks accelerate and heat particles?

- Acceleration mechanisms?- Energy Partition?- Variability?

‣How does reconnection convert magnetic energy?

- Initiation? - Magnetic topology?- Particle acceleration?

‣How does turbulence control transport in plasmas?

- Energy cascade?- Anisotropies?- Coherent structures?

Page 6: CROSS-SCALE and SCOPE:

AOGS 2009 ST06-A006

‣How do shocks accelerate and heat particles?

- Acceleration mechanisms?- Energy Partition?- Variability?

‣How does reconnection convert magnetic energy?

- Initiation? - Magnetic topology?- Particle acceleration?

‣How does turbulence control transport in plasmas?

- Energy cascade?- Anisotropies?- Coherent structures?

Top-level Science Questions

Page 7: CROSS-SCALE and SCOPE:

‣How do shocks accelerate and heat particles?

- Acceleration mechanisms?- Energy Partition?- Variability?

‣How does reconnection convert magnetic energy?

- Initiation? - Magnetic topology?- Particle acceleration?

‣How does turbulence control transport in plasmas?

- Energy cascade?- Anisotropies?- Coherent structures?

Top-level Science Questions

Page 8: CROSS-SCALE and SCOPE:

AOGS 2009 ST06-A006

Cross-Scale Coupling at Shocks

Page 9: CROSS-SCALE and SCOPE:

Cross-Scale Coupling at Shocks

Page 10: CROSS-SCALE and SCOPE:

Cross-Scale Coupling at Shocks

Page 11: CROSS-SCALE and SCOPE:

Cross-Scale Coupling and Reconnection

Page 12: CROSS-SCALE and SCOPE:

Cross-Scale Coupling and Reconnection

Page 13: CROSS-SCALE and SCOPE:

Cross-Scale Coupling and Reconnection

Page 14: CROSS-SCALE and SCOPE:

Cross-Scale Coupling and Turbulence

Page 15: CROSS-SCALE and SCOPE:

Cross-Scale Coupling and Turbulence

Page 16: CROSS-SCALE and SCOPE:

Cross-Scale Coupling and Turbulence

Page 17: CROSS-SCALE and SCOPE:

Observational Challenges

‣Time-varying‣Fundamentally 3D‣3 spatial & temporal scales

- electron- ion- fluid

‣Nonlinearly coupled‣Collisionless ⇒ Kinetic‣Plasma ⇔EM fields‣Can’t sample distant astro-plasmas

‣Near Earth space provides an excellent laboratory

A collisionless Shock

Page 18: CROSS-SCALE and SCOPE:

Length and Time Scale in Geospace

Example of the various scale lengths and time scales present in the near-Earth environment.

The smallest lengths and shortest timescales correspond to electron dynamics, followed by ion scales to eventually the fluid scales that set the context and driving conditions for the phenomena of interest.

The coupling between the various scales requires measurements at least two scales simultaneously.

Page 19: CROSS-SCALE and SCOPE:

State of the ArtCluster

‣First 3D plasma measurements

‣One scale at a time

‣Results highlighted need for multi-scale

‣Success of mission extension also confirming need for multiple scales in 3D

MMS

‣Access to electron scales in 3D‣Only one scale at a time

THEMIS

‣Global Sun-Earth Magnetosphere

‣Not universal cross-scale physics

Page 20: CROSS-SCALE and SCOPE:

State of the ArtCluster

‣First 3D plasma measurements

‣One scale at a time

‣Results highlighted need for multi-scale

‣Success of mission extension also confirming need for multiple scales in 3D

MMS

‣Access to electron scales in 3D‣Only one scale at a time

THEMIS

‣Global Sun-Earth Magnetosphere

‣Not universal cross-scale physics

Page 21: CROSS-SCALE and SCOPE:

Cluster

‣First 3D plasma measurements

‣One scale at a time

‣Results highlighted need for multi-scale

‣Success of mission extension also confirming need for multiple scales in 3D

MMS

‣Access to electron scales in 3D‣Only one scale at a time

THEMIS

‣Global Sun-Earth Magnetosphere

‣Not universal cross-scale physics

State of the Art

Page 22: CROSS-SCALE and SCOPE:

RequirementsKey Concepts

• <Behaviour> ≠ Behaviour of <>

• Simultaneous multi-scale

• Fields & particles

• Near-Earth: unique in-situ plasma laboratoryMission Design• Electron Scale: Comprehensive payload• Ion Scale: Targeted payload• Fluid Scale Context payload• Focus: coupling between scales

The Cross-Scale mission is dedicated to the study of the cross-scale coupling of Reconnection, Shocks and Turbulence

Page 23: CROSS-SCALE and SCOPE:

Requirements

10 km; 10 ms500 km; 1-5 s5000 km; 30 s

Key Concepts

• <Behaviour> ≠ Behaviour of <>

• Simultaneous multi-scale

• Fields & particles

• Near-Earth: unique in-situ plasma laboratoryFull Cross-Scale Mission Concept• Electron Scale: Comprehensive payload• Ion Scale: Targeted payload• Fluid Scale Context payload• Focus: coupling between scales

The Cross-Scale mission is dedicated to the study of the cross-scale coupling of Reconnection, Shocks and Turbulence

Page 24: CROSS-SCALE and SCOPE:

Requirements

10 km; 10 ms500 km; 1-5 s5000 km; 30 s

Key Concepts

• <Behaviour> ≠ Behaviour of <>

• Simultaneous multi-scale

• Fields & particles

• Near-Earth: unique in-situ plasma laboratoryFull Cross-Scale Mission Concept• Electron Scale: Comprehensive payload• Ion Scale: Targeted payload• Fluid Scale Context payload• Focus: coupling between scales

The Cross-Scale mission is dedicated to the study of the cross-scale coupling of Reconnection, Shocks and Turbulence

Page 25: CROSS-SCALE and SCOPE:

Requirements

10 km; 10 ms500 km; 1-5 s5000 km; 30 s

Key Concepts

• <Behaviour> ≠ Behaviour of <>

• Simultaneous multi-scale

• Fields & particles

• Near-Earth: unique in-situ plasma laboratoryFull Cross-Scale Mission Concept• Electron Scale: Comprehensive payload• Ion Scale: Targeted payload• Fluid Scale Context payload• Focus: coupling between scales

The Cross-Scale mission is dedicated to the study of the cross-scale coupling of Reconnection, Shocks and Turbulence

Page 26: CROSS-SCALE and SCOPE:

Missions

Focus: coupling between scales

ESA - Cross-Scale JAXA/CSA - SCOPE

10 km; 10 ms500 km; 1-5 s5000 km; 30 s

Page 27: CROSS-SCALE and SCOPE:

Cross-Scale Mission Study•The Cross-Scale mission has been the subject of an assessment study as part of ESA’s Cosmic Vision Plan for the ESA Science Programme•Cross-Scale is an M-Class mission candidate, due for launch in 2017. •The assessment study consisted of two parallel, recently concluded, industrial studies from 2007-2009.•Science input was via a Science Study Team, comprising of a group of international scientists (Europe, Japan, US, Canada) led by Professor Steven J. Schwartz•In parallel to the industrial activities, a number of instrument teams or consortia have been working on the scientific payload elements of the mission

Page 28: CROSS-SCALE and SCOPE:

Cross-Scale Mission Study Baseline

• Roughly equatorial (14∘) 10 x 25 RE orbit will enable numerous opportunity to investigate:

• Shocks• Reconnection• Turbulence

• 7 ESA spacecraft, launched on Soyuz-Fregat• Spacecraft will form 2 nested tetrahedra with shared corner to sample 2 scale simultaneously:

• First year of mission•Ion-Electron scales• Second year of mission•Ion-Fluid scales

Page 29: CROSS-SCALE and SCOPE:

Cross-Scale Mission Study Baseline

Page 30: CROSS-SCALE and SCOPE:

Cross-Scale Mission Study

Two different designs

Page 31: CROSS-SCALE and SCOPE:

Cross-Scale Mission Study

Option 1: the spacecraft are built around a 1666 mm cylinder. Spacecraft diameter is ~2.5 m, height 50 cm

Page 32: CROSS-SCALE and SCOPE:

Cross-Scale Mission Study

Option 2: the spacecraft are octagonal prism structures,1.59 m in diameter and 0.98 in height

Page 33: CROSS-SCALE and SCOPE:

Electron-scale physics

with the M-ND pair

Larger scale context

Daughter(far) : 5km 〜5000km

Daughter (far)

Daughter (far)

Daughter (far)

SCOPE

Ultra high-speed

electron measurement

s

Daughter(near) : 5km 〜 100km

Page 34: CROSS-SCALE and SCOPE:

Current Status

Passed Mission Design Review in January 2009

System Requirements Review at the end of Phase A will be joint with CSA (in less than 2 years time).

LoI between CSA and JAXA for the joint Phase A and SRR being drafted.

SCOPE

Page 35: CROSS-SCALE and SCOPE:

JAXA: Mother, NearDaughter + DispenserCSA: Far Daughter x 3

Dual launch partner?Over 1 tonne spare capacity2~3 s/c of 150kg classOther international partners?US, Russia, China,Taiwan

Launch configuration requires only half of by H-2A capacity

Mother Satelliteφ3.0m×h1.2m , 6

00kg

SCOPE

Dispenser Module

Daughter Satellite

×4φ1.5m×h0.6m , 150kg

Page 36: CROSS-SCALE and SCOPE:

AOGS 2009 ST06-A006

Cross-Scale – SCOPE

Next Steps-

Page 37: CROSS-SCALE and SCOPE:

AOGS 2009 ST06-A006

Location Cross-Scale + SCOPE

Page 38: CROSS-SCALE and SCOPE:

AOGS 2009 ST06-A006

Cross-Scale – SCOPE

Thank you for your attention