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Untangling complex processes within Earth s radiation belts with the Radiation Belt Storm Probes (RBSP) mission. Barry Mauk, Nicola Fox, David Sibeck, – PowerPoint PPT presentation

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Title: Barry Mauk,


1
Untangling complex processes within Earths
radiation belts with the Radiation Belt Storm
Probes (RBSP) mission.
  • Barry Mauk,
  • Nicola Fox, David Sibeck,
  • Shrikanth Kanekal, Joseph Grebowsky, Ramona
    Kessel
  • RBSP Project Science Team

This document has been reviewed for ITAR
restrictions and is cleared for public release
2
The RBSP Mission is designed to
  • Objective
  • Provide understanding, ideally to the point of
    predictability, of how populations of
    relativistic electrons and penetrating ions in
    space form or change in response to variable
    inputs of energy from the Sun.
  • Impacts
  • Understand fundamental radiation processes
    operating throughout the universe.
  • Understand Earths radiation belts and related
    regions that pose hazards to human and robotic
    explorers.

Intensities of Earths dynamic radiation belts
3
We have learned much about radiation belt
physics but substantial important mysteries
remain
4
Two types of RBSP Goals
  • Better understand individual transport and
    energization mechanisms
  • Understand the extent to which non-linearities
    modify the role that whistler mode waves play in
    exchanging energy with and scattering radiation
    belt electrons.
  • Untangling complex processes Better understand
    how these mechanisms act together to yield the
    complex behaviors that are observed.
  • What is the relationship between processes that
    supply electron source populations and those that
    generate the Ultra Low Frequency waves that can
    help transport those particles? 
  • What is the role of substorm injections in
    creating or modifying the global electric fields
    that transport and redistribute the injected
    plasma populations?
  • How dependent is the wave activity that energizes
    radiation belt electrons on the global electric
    field that creates the conditions for wave
    generation?

5
Example What is the importance of EMIC waves in
the control (loss) of radiation belt particles?
Courtesy A. (Sasha) Ukhorskiy
Mauk McPherron, Phys. Fluids,1980
6
It has been proposed that increases in helium
concentrations stimulates EMIC wave generation
Young et al., 1981 Roux et al., Rauch et al.,
1982
7
Wave modifications are so profound that mass
composition cannot be confidently determined
Mauk McPherron, Phys. Fluids,1980
Mauk and McIlwain, JGR, 1993
8
Global magnetosheric structure and transport
generate the conditions for EMIC wave generation
Global convection likely plays a key role
9
But, we remain profoundly ignorant of the
configuration and dynamic of convective fields
Rowland Wygant, 1998
Hori et al. 2005
10
Dynamic injections appear required to explain the
transport needed to population the regions of
EMIC generation
Mauk and Meng, 1983a
Kivelson et al. 1979
10
11
Understanding the importance of EMIC wave control
or radiation belts requires
  • Improved understanding of the microphysics of
    wave generate.
  • Improved understanding of the global
    electromagnetic transport processes to understand
    how the conditions for wave generation are
    created.
  • Untangling complex processes within Earths
    radiation belts

12
What is required to untangle complex processes?
  • Simultaneous, multipoint sampling at various
    spatial scales reveals source and evolution of
    critical features.
  • High quality, integrated measurements are needed
    to target key processes.

13
Multiple spacecraft must target key radiation
belt regions with variable spacing
  • 2 identically-instrumented spacecraft for
    space/time separation.
  • Lapping rates (4-5 laps/year) for simultaneous
    observations over a range of s/c separations.
  • 600 km perigee to 5.8 RE geocentric apogee for
    full radiation belts sampling.
  • Orbital cadences faster than relevant magnetic
    storm time scales.
  • 2-year mission for precession to all local time
    positions and interaction regions.
  • Low inclination (10?) to access all magnetically
    trapped particles
  • Sunward spin axis for full particle pitch angle
    and dawn-dusk electric field sampling.
  • Space weather broadcast

14
RBSP has unusually comprehensive particle and
fields instrument measurement capabilities
Particle Sensors PSBR/RPS ECT/REPT ECT/MagEIS RBSP
ICE ECT/HOPE
MagEIS
electrons
REPT
HOPE
protons
RPS
ion composition
RBSPICE
Energy
1eV
1keV
1MeV
1GeV
EMFISIS FGM
DC Magnetic
Fields Waves Sensors EMFISIS/MAG EMFISIS/Waves E
FW
AC Magnetic
EFW Perp 2D
DC Electric
EFW Par 1D
EMFISIS Waves
AC Electric
EFW E-field Spectra
DC 10Hz
1kHz
1MHz
Frequency
15
Coordinating RBSP with other missions helps
greatly to untangle processes Example Themis
Courtesy of Sibeck Ukhorskiy
16
RBSP resolves important universal science
questions that have practical consequences
  • RBSP advances NASAs Strategic Plan and
    Heliospheric Science Objectives
  • Fundamental science.
  • Determining effects of solar variability on
    technological systems.
  • Developing ability to predict extreme dynamic
    space conditions.
  • Much has been learned about radiation belt
    physics but our ignorance is profound in some
    areas
  • Text book predictions about key observations are
    wrong.
  • Radiation belt dynamics is not understood.
  • Untangling the interaction of complex processes
    is needed.
  • RBSP provides the needed multi-point sampling and
    integrated measurements to make transformational
    advances in understanding.

17
  • Backup
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