Title: Pitch angle evolution of energetic electrons at geosynchronous orbit during disturbed times
1Pitch angle evolution of energetic electrons at
geosynchronous orbit during disturbed times
- R. Friedel, Y. Chen, G. Reeves, T. Cayton
- ISR-1, Los Alamos National Laboratory, USA
- Yuri Shprits
- University of California, Los Angeles, USA
2Contents
- Rationale
- Geosynchronous pitch angle distributions
- Instrumentation and Data
- Drift shell splitting example and explanation
- Mapping to constant L 6.5
- Assumptions
- Demonstration of method
- Quiet time test of method (10-13 December 2002)
- Application to small relativistic electron event
- August 2-5, 2002
- Theoretical predictions
- Summary/Conclusion
3Rationale
- Energetic electron pitch angle distributions show
clear local time variations due to the asymmetry
of the Earths field Drift shell splitting
L f (pitch angle) - These geometric effects may mask the changes
that may be due to in-situ acceleration or pitch
angle scattering processes. - We remove here the geometric effects by mapping
the observed pitch angle distributions to a fixed
3rd (L,F) adiabatic invariant preserving the 1st
(µ) and 2nd (K,J) adiabatic invariants.
4Geosynchronous Instrumentation and Data
- Data is presented from the relativistic electron
channels of the LANL SOPA instrument 50 keV
1.5 MeV. - As there is no magnetometer on the LANL GEO
spacecraft, the magnetic field direction is
inferred using the MPA plasma measurements by
deducing the symmetry axis of the pressure tensor
(Thomsen et al, 1996). - GEO spacecraft have a 10 sec spin period. SOPA
data sampling is at 0.16 seconds. Data is
collected in 32 azimuthal bins averaged over 10
minutes. - Pitch angle resolved GEO data is available for
LANL-97a, 1991-080 and 1990-095 for most of Jul
2002 Dec 2003.
5Geosynchronous Orbit Drift shell splitting
example and explanation
6Mapping to L6.5Assumptions
Drift shell splitting at geo orbit leads to
observations over L 6 7. We map observations
to a fixed L 6.5 at constant µ (1st) and K
(2nd) invariant using the following assumptions
- Phase space density gradients near GEO are flat
or small (SCATHA Fennell and GEO/Polar Chen
observations). - Over this small range of L we can approximate
our µ mapping using a dipolar
approximation. - The change in the mapping of K to pitch angle is
over this range of L is negligible.
7Mapping to L6.5Demonstration of method near
midnight
8Mapping to L6.5Map at constant K or pitch
angle?
- We tested the change in the 2nd invariant K to
pitch angle mapping at a variety of local times
for L6 and L7, the maximum mapping needed in
this study. - Changes in pitch angle at constant K are lt 3 Deg,
which below our 10 deg pitch angle resolution.
Near geosynchronous orbit we thus are safe to
map at constant pitch angle.
9Pitch Angle MappingQuiet time test of Method -
Olson Pfitzer Model
10Pitch angle MappingSmall rel. electron Event
August 2-5, 2002
11Evolution of Pitch Angle Distributions
Modeling effects of Waves - UCLA
- Addition of EMIC waves leads to rapid loss of
electrons at energies down to 0.5 MeV - Higher pitch angles are affected for higher
energies - lt 60o 1 MeV
- lt 30o 400 keV
12LANL GEO Pitch Angle observations at all
energies 50 keV 1.5 MeV
- Losses to lt60o for 1MeV
- Losses become less severe as energy decreases
- Observations are roughly consistent with EMIC
theory and modeling
13Summary / Conclusion
- Pitch angle mapping seems to work and can reveal
the real PA distribution dynamics - We show that method works in principle however
many assumptions probably violated during very
active periods - For the week relativistic electron event of
August 2-5, 2002 - the pitch angle distribution seems to show
evidence of acceleration processes (-gt peaked at
90o) - The loss period at the end of the event is
clearly associated with cold dense plasma and
losses are due to precipitation -gt field aligned
electrons vanish - Association with EMIC waves Detailed evolution
modeling of PA distributions shows roughly
consistent behavior with data.