The science targets of the SCOPE mission Masaki Fujimoto ISAS, JAXA.
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Transcript of The science targets of the SCOPE mission Masaki Fujimoto ISAS, JAXA.
The science targets of the SCOPE mission
Masaki FujimotoISAS, JAXA
The solar system, the natural laboratory for space plasma
• Formation of planetary magnetospheres via interaction between the solar wind and the planet’s intrinsic magnetic field
• Dynamics behavior of plasma in the magnetospheres
The same is true for the earth’s magnetosphere
• Aurora. Its attractive behavior reflects the dynamism of the plasma in the earth’s magnetosphere
Earth and planetary magnetospheres:The point of view
• Interest in itself.
Earth and planetary magnetospheres:The point of view
• Interest in itself.
• The laboratory of space plasma dynamics
• The only field where in-situ measurements of particles and fields can be made.
Magnetospheric physics: The new stage
• “The Plasma Universe”
• “The Magnetic Universe”
The question
What makes the cosmic gas to behave so dynamically?
#Looking through the earth’s magnetosphere at the Plasma Universe
Plasmas throughout the Universe
What SCOPE can do to establish the Plasma Universe concept
• Perform unprecedented in-situ observations targeted at
shocks, reconnection, and turbulence. • The target physical processes are of
fundamental importance in the universal context, and are operative in the earth’s magnetosphere.
• Construct hands-on-data basis towards the fundamental understanding of the processes.
• Critical knowledge that can come only through in-situ observations.
The MHD way of looking at space plasmas
• MHD Approximation
- Gas motion under the influence of magnetic field and electric currents
- The gas motion twists the field lines.
- A new spatial distribution of electric currents are set up.
- Gas motion is altered.
- (refrain)
Electric currents in space
• J = rot B in MHD
• J is determined by the spatial structure of B. No problem in producing whatever current density required.
• J = rot B in MHD• J is determined by the spatial structure of B. No
problem in producing whatever current density required.
??!
Electric currents in space
• J = rot B in MHD• J is determined by the spatial structure of B. No
problem in producing whatever current density required.
• In reality, J reflects differential motion between ions and electrons, namely, J=en(Vi-Ve).
• A mechanism (non-MHD physics) is needed when extremely large current density (thin current sheet) is required.
• Onset of non-MHD effects in a thin current sheet embedded in the MHD-scale dynamics that pinches the current sheet: This is where most of the wonders in space plasmas originate!
Beyond MHD
• MHD is useful but misses the most attractive part of space plasma physics
• We are determined to step forward and to construct a new framework that truly captures the attraction
• SCOPE will generate hands-on-data basis for the new framework.
The only field where detailed in-situ measurements
of the complicated physical system is possible
The target physical processes
Shocks, reconnection,
and turbulence:
Shocks
• Shocks themselves are fluid-dynamical entities
• In space physics, shocks are said to be particle accelerators
• Fluid versus particle?!
The energy spectrum of cosmic ray
Particle acceleration at shocks
SN R1006
Shocks: ordinary fluid-dynamics versus space plasma physics
UpstreamFast and cold, Maxwell distribution
Very thin transition layer, where viscosity is effecttive
DownstreamSlow and hot, Maxwell distribution
Explosive magnetic reconnection
In the night-side magnetosphere,
Large scale current sheetpinching motion
Thin current sheet foramtion,onset of electron scale dynamicsWithin it.
Maturing of the reconnection engine(diffusion region)
Creation of reconnection jet
Jet interacting with the surrounding plasma
Set-up of auroral current system
Production ofenergetic particles
Theory “predicts” very curious behavior of collisionless plasma. Is it truly happening in the real space plasma? We won’t identify ourselves understanding it until we “see” it in the data.
Turbulence
• Turbulence is something you cannot get away from if you are interedted in non-linear fluid/gas dynamics
• The addition of the magnetic effects adds even more complication in space plasmas
• One of the fundamental problem in space plasma physics, particle acceleration, is closely related with turbulence.
Magnetic field, collisionless system, dynamical coupling among different scales
• Cascade power at short wavelength viscous dissipation: Ordinary picture
• Cascade power at short wavelength New terms start to dominate giving rise to new effects: Space plasmas
Space plasma turbulence
k
Power
Energy cascase
MHD-scale
Ion-scale
Electron-scale
Non-MHD effects arise as cascade proceeds
Magnetic field, collisionless system, dynamical coupling among different scales
• Cascade power at short wavelength viscous dissipation: Ordinary picture
• Cascade power at short wavelength New terms start to dominate giving rise to new effects: Space plasmas
• Background (zero-th order) inhomogeneity supported by magnetic field is ubiquitous
Dipole-tail current sheet transition region
Shocks, reconnection, and turbulence
MHD phenomenon as a whole.
MHD does not let you truly understand what you are attracted to in space plasma physics
It is the coupling between MHD-scale dynamics and non-MHD (ion and electron scale physics)that is crucial for the fundamental understanding of space plasma dynamics
What SCOPE can do to establish the Plasma Universe concept
• Perform unprecedented in-situ observations targeted at
shocks, reconnection, and turbulence.
What exactly is this?
• Perform unprecedented in-situ observations targeted at
shocks, reconnection, and turbulence.
Simultaneousmulti-scale observations
Cross Scale CouplingMHD-scale dynamics
Key process in key region
In most cases, ion/electron scale physics
Non-linear effects
Non-MHD processes add interestingeffects unreachable by MHD dynamics
Boundary condition
Addition of curious effects Large-scale Dynamic
phenomenon develops only when the system works
as a whole
Simultaneous multi-scale measurements
• Zoom-in to the electron-scale and monitoring ion/MHD-scale dynamics at the same time
# Large FOV and high-resolution pixels at the same time, in the case of imaging.
SCOPE
Shock wave
Magnetic Reconnection
Boundary Layer TurbulenceProcesses of fundamental importance in the Plasma Universe
Turbulence atdipole-current sheet transition region
The science questions of SCOPE
• Shocks
• Reconnection
• Turbulence
Shocks
• How does a shock dissipate and distribute the upstream kinetic energy?
• What is the role of the extended turbulent region upstream of a shock front due to the collision-less nature of the plasma?
• How does a shock accelerate particles to high energies?
Reconnection
• How is reconnection triggered?
• How does the energy conversion in reconnection progress?
• How does reconnection produce non-thermal particles?
Turbulence
• How does turbulence transport energy over multiple scales?
• How does turbulence lead to anomalous transport of plasma?
• How does turbulence interact with the background non-uniformity to produce anomalous transport?
The worst question you can ever think of:
“Will SCOPE just confirm what theorists predict?”
• The key issue: How does the system act locally in response to the requirement J = rot B given by MHD-scale dynamics
• Collisionless plasma: Almost infinite degrees of freedom in the distr. fn. shape that satisfies
J=en(Vi – Ve)
• How Nature makes the choice is the question.
• You just cannot convince yourself until you “see the data in your hand”.
Simulation studies and SCOPE
• Due to computational resource limitations, one should think that simulation results are suggesting possibilities but nothing more.
• At the same time, one should be excited to see in the simulation results how curious space plasmas can possibly behave.
• Then one should be motivated to dig into the data to discover that is very exciting, or plan a mission that will produce very exciting data.
• Likewise simulation studies are occasionally directed by data analysis studies.
• In any case, most simulationists (at least in JP) will invest their efforts in multi-scale simulations for the next ~10 years.
SCOPE: The mission
Daughter(far) : 5km 〜 5000km
Daughter(far)
Daughter(far)
Mother
Daughter(near) : 5km 〜 100 km
Daughter(far)
MHD Scale
Ultra high-speed electron measurements
Electron Scale
SCOPE-Original
Mother-NearDaughter pair
• As good as/bettter than the MMS s/c• FESA: 10 msec ele detection in the magnetotail
(100 times higher sensitivity than MMS)• MEP: Covers 10~100 keV energy range continu
ously• Wave-particle correlator• Sun-pointing spin axis of ND: Precise measurem
ents of north-south DC E-field component • Inter-s/c distance <100km: Electron-scale pair
FarDaughters
• More or less a standard spacecraft (~150kg)• 3-component E&B wave measurements on all s/
c enabling quantitative analysis of the wave energy flow
• Inter-s/c distance <100km ~ 5000km
Electron~ion~MHD scales
M-ND pair@electron scale + FD@ion/MHD
simultaneous multi-scale obs.
Obs. supporting systems
• Inter-s/c comm. for localization, time-synchronization, commanding, and data link for intelligent coordination
• Large volume data storage
• Spin axis antenna
Right size budget?
• M-ND by JAXA
• FD by CSA
• SIs onboard SCOPE by JAXA-CSA led consortium
• Launcher = H2A: More capability than ISAS science program can afford to fill
NASA as the dual-launch partner
The toughest question
• Is the number of the s/c outside the mother-daughter pair, three, good enough?
• Two-scales at the same time, at most.• More straightly, more is not only better but is differ
ent.
International collaboration helps.
The whole picture of SCOPE/Cross-Scale:
Full-scale coverage via international collaboration with clear interfaces
ESA’s component Cross-Scale
China’s component Russia’s component
To be launched by JAXA’s H2-ASCOPE mother and near/far-daughter (JAXA) Far-daughters (CSA)
Dual launch partner THEMIS-like s/c (NASA)
The status of SCOPE
• Passed MDR in Jan 09
• Ready to move on to Phase A (another review expected in May 09)
• Intense collaboration with CSA started
• Need to accelerate the study on the NASA component
• SCOPE/Cross-Scale MUST happen with the full-scale international collaboration scheme.
The whole picture of SCOPE/Cross-Scale:
Full-scale coverage via international collaboration with clear interfaces
ESA’s component Cross-Scale
China’s component Russia’s component
To be launched by JAXA’s H2-ASCOPE mother and near/far-daughter (JAXA) Far-daughters (CSA)
Dual launch partner THEMIS-like s/c (NASA)
Hey, how about Taiwan?!