A statistical study of the Field-Aligned Electron Events (status report) Solène Lejosne, Forrest Mozer and Oleksiy Agapitov SSL, University of California,

Slides:



Advertisements
Similar presentations
Solar flare hard X-ray spikes observed by RHESSI: a statistical study Jianxia Cheng Jiong Qiu, Mingde Ding, and Haimin Wang.
Advertisements

U N C L A S S I F I E D Operated by the Los Alamos National Security, LLC for the DOE/NNSA Direct measurements of chorus wave effects on electrons in the.
Electron Acceleration in the Van Allen Radiation Belts by Fast Magnetosonic Waves Richard B. Horne 1 R. M. Thorne 2, S. A. Glauert 1, N. P. Meredith 1.
Influence of EMIC Waves on Radiation Belt Dynamics T. Kersten, R. B. Horne, N. P. Meredith, S. A. Glauert ESWW11 Liège, 17-21/11/2014 British Antarctic.
1 FIREBIRD Science Overview Marcello Ruffolo Nathan Hyatt Jordan Maxwell 2 August 2013FIREBIRD Science.
MHD Simulations of the January 10-11, 1997 Magnetic Storm Scientific visualizations provide both scientist and the general public with unprecedented view.
U N C L A S S I F I E D Operated by the Los Alamos National Security, LLC for the DOE/NNSA Pitch angle evolution of energetic electrons at geosynchronous.
The Importance of Wave Acceleration and Loss for Dynamic Radiation Belt Models Richard B. Horne M. M. Lam, N. P. Meredith and S. A. Glauert, British Antarctic.
Electron Acceleration inside Jupiter’s Radiation Belt and the Origin of Synchrotron Radiation Richard B. Horne 1 R. M. Thorne 2, S. A. Glauert 1, J. D.
Pitch-Angle Scattering of Relativistic Electrons at Earth’s Inner Radiation Belt with EMIC Waves Xi Shao and K. Papadopoulos Department of Astronomy University.
Jasper S. Halekas Space Sciences Laboratory
Cusp Radiation Source: A Challenge for Theory and Simulation Jiasheng Chen, Theodore A. Fritz, Katherine E. Whitaker, Forrest S. Mozer, and Robert B. Sheldon.
1 TOWARD PREDICTING VLF TRIGGERING MURI Workshop 3 March 2008 E. Mishin and A. Gibby Boston College ISR Stanford University STAR Lab.
Seasonal dependence of LEP observed on DEMETER Erin S. Gemelos 1, Umran S. Inan 1, Martin Walt 1, Jean-Andre Sauvaud 2, Michel Parrot 3 February 18, 2009.
ROPA/REIMEI show ~300eV inverted-V type spatial structures Collocated with region of patches but not correlated with individual patches Low energy precipitation.
SSL UC Berkeley 2010 June ACE/SOHO/STEREO/Wind Workshop Interplanetary Propagation of Solar Impulsive Energetic Electrons Linghua Wang, Bob Lin and S ä.
Finite Temperature Effects on VLF-Induced Precipitation Praj Kulkarni, U.S. Inan and T. F. Bell MURI Review February 18, 2009.
RBSP-ECT Suite Status: Instrument Status and Instrument Operations Flexibility Harlan E. Spence on behalf of RBSP-ECT Team University of New Hampshire.
RBSP observations: Poloidal ULF waves and drift-resonance wave particle interaction Lei Dai, Kazue Takahashi, John Wygant, EFW team. EMFISIS and ECT(MagEIS)
Auroral Boundaries Model Validation – What has been done.
ELECTRON ACCELERATION BY TIME DOMAIN STRUCTURES (TDS) by Mozer, F.S., O.V. Agapitov, A.V. Artemyev, V. Krasnoselskikh, and I. Vasko OUTLINE 1.Experimental.
Nonlinear VLF Wave Physics in the Radiation Belts Chris Crabtree Guru Ganguli Erik Tejero Naval Research Laboratory Leonid Rudakov Icarus Research Inc.
EFW Data Products/Processing Van Allen Probe SWG San Antonio September 2104 J.R. Wygant, J. Bonnell, Aaron Breneman, S. Thaller and the EFW Team.
Comparisons of Inner Radiation Belt Formation in Planetary Magnetospheres Richard B Horne British Antarctic Survey Cambridge Invited.
Morphology of Inner Magnetospheric low-energy ions M. Yamauchi, et al. Swedish Institute of Space Physics (IRF), Kiruna.
RBSP SWG Meeting 1 3/5/2009 BARREL Update (Balloon Array for RBSP Relativistic Electron Losses) R. M. Millan and the BARREL Team.
Magnetosphere-Ionosphere coupling processes reflected in
Hot He + events in the inner magnetosphere observed by Cluster M. Yamauchi 1, I. Dandouras 2, H. Reme 2, H. Nilsson 1 (1) Swedish Institute of Space Physics.
Outline > does the presence of NL waves affect the conclusion that QL acceleration suffices? > it depends... Outline Large amplitude whistler waves Limitations.
Large-Amplitude Electric Fields Associated with Bursty Bulk Flow Braking in the Earth’s Plasma Sheet R. E. Ergun et al., JGR (2014) Speaker: Zhao Duo.
Large electric fields near the nightside plasmapause observed by the Polar spacecraft K.-H. Kim 1, F. Mozer 2, and D.-H. Lee 1 1 Department of Astronomy.
Kinetic-scale electric field structures at plasma boundaries in the inner magnetosphere (including injection fronts) David Malaspina 1, John Wygant 2,
In Situ Measurements of Auroral Acceleration Regions Wu Tong
Nonlinear Electric Field Structures and Magnetic Dipolarizations in the Inner Magnetosphere David Malaspina 1, Laila Andersson 1, Robert Ergun 1, John.
EUV Observations of the Structure and Dynamics of the Plasmasphere Bill R. Sandel, Jerry Goldstein, Dennis Gallagher, & Don Carpenter.
Proposed project on lightning-induced electron precipitation (LEP) Lightning produces VLF waves that propagate globally in the Earth- ionosphere waveguide.
Multi-point observations of dispersionless injection fronts inside geostationary orbit: propagation and structure Authors (preliminary) David Malaspina.
NASA NAG Structure and Dynamics of the Near Earth Large-Scale Electric Field During Major Geomagnetic Storms P-I John R. Wygant Assoc. Professor.
EFW SOC DATA John Wygant SWG June Redondo Beach.
Cluster 911 Plasmoid Substorm Sept 11, 2002 DOY 254 Onset at 1600 UT Shock at Cluster 16:23 Plasmoid 16: :40 UT.
Hot He + events in the inner magnetosphere observed by Cluster 1 Yamauchi, et al. (2014), JGR, doi: /2013JA Inner magnetosphere: Majority.
Microwave emission from the trapped and precipitated electrons in solar bursts J. E. R. Costa and A. C. Rosal1 2005, A&A, 436, 347.
Electric field, electric potential, and ‘density’ measurements at quasi-perpendicular collisionless shocks: Cluster/EFW measurements Stuart D. Bale, Ryan.
Multi-Spacecraft Observation of Compressional Mode ULF Waves Excitation and Relativistic Electron Acceleration X. Shao 1, L. C. Tan 1, A. S. Sharma 1,
Nonlinear electric field structures in the inner magnetosphere D. M. Malaspina 1, L. Andersson 1, R. E. Ergun 1, J. R. Wygant 2, J. W. Bonnell 3, C. Kletzing.
The large scale convection electric field, ring current energization, and plasmasphere erosion in the June 1, 2013 storm Scott Thaller Van Allen Probes.
MULTI-INSTRUMENT STUDY OF THE ENERGY STEP STRUCTURES OF O + AND H + IONS IN THE CUSP AND POLAR CAP REGIONS Yulia V. Bogdanova, Berndt Klecker and CIS TEAM.
Storm-dependent Radiation Belt Dynamics Mei-Ching Fok NASA Goddard Space Flight Center, USA Richard Horne, Nigel Meredith, Sarah Glauert British Antarctic.
HISAKI mission – ひさき – Chihiro Tao 1,2, Nicolas Andre 1, Hisaki/EXCEED team 1. IRAP, Univ. de Toulouse/UPS-OMP/CNRS 2. now at NICT
© Research Section for Plasma and Space Physics UNIVERSITY OF OSLO Daytime Aurora Jøran Moen.
SEPT/STEREO Observations of Upstream Particle Events: Almost Monoenergetic Ion Beams A. Klassen, R. Gomez-Herrero, R. Mueller-Mellin and SEPT Team, G.
Field-aligned currents associated with interchange injections at Saturn Anna DeJong, James Burch and Roberto Livi Southwest Research Institute.
The Role of VLF Transmitters in Limiting the Earthward Penetration of Ultra-Relativistic Electrons in the Radiation Belts J. C. Foster, D. N. Baker, P.J.
Source and seed populations for relativistic electrons: Their roles in radiation belt changes A. N. Jaynes1, D. N. Baker1, H. J. Singer2, J. V. Rodriguez3,4.
Modulation of chorus wave intensity by ULF waves from Van Allen Probes Observation Lunjin Chen 1, Zhiyang Xia 1, Lei Dai 2 1 Physics Dept., The University.
Cluster observation of electron acceleration by ULF Alfvén waves
AGILE as particle monitor: an update
Alexandra Teste, G. K. Parks, M. Wilber, N. Lin
Olga Khabarova 1, valentina zharkova 2 & vladimir kuznetsov 1
Recent KTH Cluster research
Definitive Mapping in the Late Growth Phase
M. Yamauchi1, I. Dandouras2, H. Reme2,
Sub-keV Phenomena of Dayside Ring Current
Magnetospheric waves Lauren Blum.
R. Bucˇık , K. Kudela and S. N. Kuznetsov
Jupiter’s Polar Auroral Emisssions
Yue Chen (Los Alamos National Laboratory)
Particle energization by substorm dipolarizations
K. A. Goodrich, R. E. Ergun, S. J. Schwartz, L. B
Relative Intensity (Ratio)
Presentation transcript:

A statistical study of the Field-Aligned Electron Events (status report) Solène Lejosne, Forrest Mozer and Oleksiy Agapitov SSL, University of California, Berkeley Special thanks to the HOPE team SWG Meeting, July 2015, APL

Field-Aligned Electron Events? 5 panels of electron pitch angle distributions measured by HOPE (<50 keV) -Bursts of usually <10min duration of field-aligned electrons (mostly in both directions) -Indications of possible precipitation Motivation (1/2) Energy (eV)

-[Mozer et al., 2015] + [Lejosne et al., … under review, JGR]: relation between TDS, field-aligned electrons, and auroras -“field-aligned electron distributions are indeed quite interesting, and determining when they occur would be important” -[Abel et al., 2002a, 2002b]: statistical study of field-aligned events using CRRES data (15 months) no statistical link between the observed events and the wave power of the whistler mode and ECH waves Motivation (2/2)

Approach (1/3) (Pitch Angle) Ratio = Flux near loss cone Flux 90 o particles Energy (eV) Playing with HOPE data (Pitch Angle) Ratio > 1 => precipitation?

Approach (2/3) An example of chorus waves in the presence of field aligned electrons An example of broadband noise (TDS) in the presence of field aligned electrons

Approach (3/3) -Designed an algorithm to detect Field-aligned Electron Events from daily pitch angle ratio matrixes -For each event: time_start duration average ratio by energy ch“max” EFW (BFW) by freq ch - Statistical analysis from November 2012 to June 2015

First results: where can I see field-aligned electron events? (1/3) Probability to see field-aligned electrons as a function of the radial distance

First results: where can I see field-aligned electron events? (2/3) Max(EFW) >0.5mV/m Probability to see active field-aligned electron events as a function of MLT

First results: where can I see field-aligned electron events? (3/3) Probability to see active field-aligned electron events as a function of energy and MLT Max(EFW) >0.5mV/m

First results: what about the wave content? (1/2) Max(EFW) >0.5mV/m

First results: what about the wave content? (2/2) Max(EFW) >0.5mV/m

Conclusion The occurrence frequency of the field aligned electron events increases with the radial distance. There are more ~300eV field aligned electron events than ~10keV field-aligned electron events 300 eV field-aligned electron events are : -Observed predominantly on the premidnight sector (~22MLT) -Associated with broadband electrostatic noise in the filterbank => TDS cause field-alignment of electrons of ~300 eV in the premidnight sector ~10 keV field-aligned electron events are: -Observed predominantly on the morning side (~6MLT) -Associated with a signal of high frequency in the filterbank => Chorus cause field-alignment of electrons of ~10 keV in the morning sector