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.

Slides:



Advertisements
Similar presentations
Recap and Space Weather In the Magnetosphere (II) Yihua Zheng June 5, 2013 SW REDI.
Advertisements

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.
1 FIREBIRD Science Overview Marcello Ruffolo Nathan Hyatt Jordan Maxwell 2 August 2013FIREBIRD Science.
First panel is the EFW spin fit (10.5 s) electric field in ~ dawn-dusk direction. This measurement is dominated by waves with amplitudes >32 mV/m ptp during.
Radiation Belt Electron Pitch Angle Measurements from the GOES Satellites T. G. Onsager, J. C. Green, and H. J. Singer NOAA Geostationary Operational Environmental.
ESS 7 Lecture 14 October 31, 2008 Magnetic Storms
Spatial distribution of the auroral precipitation zones during storms connected with magnetic clouds O.I. Yagodkina 1, I.V. Despirak 1, V. Guineva 2 1.
Radiation Belt Loss at the Magnetopause T. G. Onsager, J. C. Green, H. J. Singer, G. D. Reeves, S. Bourdarie Suggest a pitch-angle dependence of magnetopause.
Anti-parallel versus Component Reconnection at the Magnetopause K.J. Trattner Lockheed Martin Advanced Technology Center Palo Alto, CA, USA and the Polar/TIMAS,
Identification and Analysis of Magnetic Substorms Patricia Gavin 1, Sandra Brogl 1, Ramon Lopez 2, Hamid Rassoul 1 1. Florida Institute of Technology,
Auxiliary slides. ISEE-1 ISEE-2 ISEE-1 B Locus of  = 90 degree pitch angles Will plot as a sinusoid on a latitude/longitude projection of the unit.
Solar wind-magnetosphere coupling Magnetic reconnection In most solar system environments magnetic fields are “frozen” to the plasma - different plasmas.
Earth’s Radiation Belt Xi Shao Department of Astronomy, University Of Maryland, College Park, MD
O. M. Shalabiea Department of Physics, Northern Borders University, KSA.
CISM Radiation Belt Models CMIT Mary Hudson CISM Seminar Nov 06.
Lecture 3 Introduction to Magnetic Storms. An isolated substorm is caused by a brief (30-60 min) pulse of southward IMF. Magnetospheric storms are large,
From Geo- to Heliophysical Year: Results of CORONAS-F Space Mission International Conference «50 Years of International Geophysical Year and Electronic.
Magnetospheric Morphology Prepared by Prajwal Kulkarni and Naoshin Haque Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global.
S. Elkington, June 11, 2009 An overview of Earth’s magnetosphere and its coupling with the solar wind Scot R. Elkington LASP, University of Colorado
Recap and Space Weather In the Magnetosphere (II) Yihua Zheng June 5, 2014 SW REDI.
Science Questions What is responsible for the "near" prompt onset of convection in the inner magnetosphere? Fast mode rarefraction wave?. How is the dayside.
Van Allen Probes, NOAA, and Ground Observations of a Pc 1 Wave Event Extending 12 Hours in MLT Mark Engebretson 1, Jennifer Posch 1, John Wygant 2, Craig.
Tuija I. Pulkkinen Finnish Meteorological Institute Helsinki, Finland
ESS 200C Lecture 18. An isolated substorm is caused by a brief (30-60 min) pulse of southward IMF. Magnetospheric storms are large, prolonged disturbances.
D. Sibeck, R. Millan, H. Spence
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.
The Role of ULF wave activity in solar wind-magnetosphere interactions and magnetospheric electron acceleration V. Pilipenko, N. Romanova, M. Engebretson,
Magnetospheric ULF wave activity monitoring based on the ULF-index OLGA KOZYREVA and N. Kleimenova Institute of the Earth Physics, RAS.
Does Fermi Acceleration of account for variations of the fluxes of radiation belt particles observations at low altitudes during geomagnetic storms? J.
1 Barry Mauk, Nicola Fox, David Sibeck, Shrikanth Kanekal, Joseph Grebowsky, Ramona Kessel RBSP Project Science Team This document has been reviewed for.
Living With a Star Radiation Belt Storm Probes and Associated Geospace Missions D. G. Sibeck Project Scientist NASA Goddard Space Flight Center.
Magnetosphere-Ionosphere coupling processes reflected in
Response of the Polar Cusp and the Magnetotail to CIRs Studied by a Multispacecraft Wavelet Analysis Axel Korth 1, Ezequiel Echer 2, Fernando L. Guarnieri.
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.
Global Simulation of Interaction of the Solar Wind with the Earth's Magnetosphere and Ionosphere Tatsuki Ogino Solar-Terrestrial Environment Laboratory.
Space Weather: Magnetic Storms 31 October 2011 William J. Burke Air Force Research Laboratory/Space Vehicles Directorate Boston College Institute for Scientific.
Dynamics of the Radiation Belts & the Ring Current Ioannis A. Daglis Institute for Space Applications Athens.
PAPER I. ENA DATA ANALYSIS RESULTS. The Imager for Magnetopause-to- Aurora Global Exploration (IMAGE) missionis the first NASA Mid-size Explorer (MIDEX)
Initial Measurements of O-ion and He-ion Decay Rates Observed from the Van Allen Probes RBSPICE Instrument Andrew Gerrard, Louis Lanzerotti et al. Center.
MAGNETOSPHERIC RESPONSE TO COMPLEX INTERPLANETARY DRIVING DURING SOLAR MINIMUM: MULTI-POINT INVESTIGATION R. Koleva, A. Bochev Space and Solar Terrestrial.
Kinetic-scale electric field structures at plasma boundaries in the inner magnetosphere (including injection fronts) David Malaspina 1, John Wygant 2,
Earth’s Magnetosphere NASA Goddard Space Flight Center
Introduction to Space Weather Jie Zhang CSI 662 / PHYS 660 Fall, 2009 Copyright © Magnetosphere: Geomagnetic Activties Nov. 5, 2009.
Scott Thaller Van Allen Probes EFW meeting University of Minnesota June 10-12, 2014.
Mass Transport: To the Plasma Sheet – and Beyond!
Radiation Storms in the Near Space Environment Mikhail Panasyuk, Skobeltsyn Institute of Nuclear Physics of Lomonosov Moscow State University.
WG2 Summary Broke into ring current/plasmasphere and radiation-belt subgroups RING CURRENT Identified events for addressing science questions What is the.
Space Weather in Earth’s magnetosphere MODELS  DATA  TOOLS  SYSTEMS  SERVICES  INNOVATIVE SOLUTIONS Space Weather Researc h Center Masha Kuznetsova.
NASA NAG Structure and Dynamics of the Near Earth Large-Scale Electric Field During Major Geomagnetic Storms P-I John R. Wygant Assoc. Professor.
Van Allen Probes Extended Mission Science Themes (1 of 3) 1.Spatial and temporal structures of injections and other transient phenomena and their effects.
Space Science MO&DA Programs - November Page 1 SS It is well known that intense auroral disturbances occur in association with substorms and are.
Multi-Spacecraft Observation of Compressional Mode ULF Waves Excitation and Relativistic Electron Acceleration X. Shao 1, L. C. Tan 1, A. S. Sharma 1,
What is a geomagnetic storm? A very efficient exchange of energy from the solar wind into the space environment surrounding Earth; These storms result.
The large scale convection electric field, ring current energization, and plasmasphere erosion in the June 1, 2013 storm Scott Thaller Van Allen Probes.
Storm-dependent Radiation Belt Dynamics Mei-Ching Fok NASA Goddard Space Flight Center, USA Richard Horne, Nigel Meredith, Sarah Glauert British Antarctic.
Earth’s Magnetosphere Space Weather Training Kennedy Space Center Space Weather Research Center.
On-Line Visualization Ring Current / Radiation Belt.
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.
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
GOES Data Status Mutual Benefits of NASA THEMIS and NOAA GOES
Plasma Wave Excitation Regions in the Earth’s Global Magnetosphere
VNC: Application of Physics and Systems Science methodologies to Forecasting of the Radiation Belt Electron Environment S. N. Walker1, M. A. Balikhin1,
ESS 200C Lecture 18.
Mission overview: two spacecraft that target key radiation belt regions with variable spacing
Subauroral heliosphere-geosphere coupling during November 2004 ionospheric storms: F2-region, North-East Asia Chelpanov M. A., Zolotukhina N.A. Institute.
N. Romanova, V Pilipenko, O. Kozyreva, and N. Yagova
Richard B. Horne British Antarctic Survey Cambridge UK
Added-Value Users of ACE Real Time Solar Wind (RTSW) Data
Magnetosphere: Structure and Properties
Presentation transcript:

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 Received 24 MAR 2015 Accepted 18 JUL 2015 Accepted article online 22 JUL 2015 Published online 9 SEP 2015 Journal of Geophysical Research: Space Physics

Contents Basic Key Point Basic Key Point Van Allen Probe Van Allen Probe Abstract Abstract Event Overview Event Overview Wave activity Wave activity Conclusion Conclusion Discussion Discussion

Basic key point Dst It gives information about the strength of the ring current around Earth caused by solar protons and electrons.(Kyoto) Dst It gives information about the strength of the ring current around Earth caused by solar protons and electrons.(Kyoto)ring currentring current Kp The K-index quantifies disturbances in the horizontal component of earth's magnetic field with an integer in the range 0–9 with 1 being calm and 5 or more indicating a geomagnetic storm 13 position estimated (Potsdam) Kp The K-index quantifies disturbances in the horizontal component of earth's magnetic field with an integer in the range 0–9 with 1 being calm and 5 or more indicating a geomagnetic storm 13 position estimated (Potsdam)earth's magnetic fieldintegergeomagnetic stormearth's magnetic fieldintegergeomagnetic storm AE index It was measure of global electrojet activity in the auroral zone. The AE index is now widely used for researches in geomagnetism, aeronomy, and solar-terrestrial physics AE index It was measure of global electrojet activity in the auroral zone. The AE index is now widely used for researches in geomagnetism, aeronomy, and solar-terrestrial physics. Magnetopause The magnetopause is the abrupt boundary between a magnetosphere and the surrounding plasma. For planetary science, the magnetopause is the boundary between the planet’s magnetic field and the solar wind Magnetopause The magnetopause is the abrupt boundary between a magnetosphere and the surrounding plasma. For planetary science, the magnetopause is the boundary between the planet’s magnetic field and the solar wind magnetosphereplasmaplanetary sciencesolar wind magnetosphereplasmaplanetary sciencesolar wind Bx By Bz

Basic key point Radiation belt? Radiation belt? A radiation belt is a layer of energetic charged particles that is held in place around a magnetized planet A radiation belt is a layer of energetic charged particles that is held in place around a magnetized planetenergeticcharged particlesenergeticcharged particles Substorm injection? Substorm injection? CME(Coronal Mass Ejection)  Geomagnetic storm  ions into the outer radiation belt CME(Coronal Mass Ejection)  Geomagnetic storm  ions into the outer radiation belt Chorus wave? Chorus wave? 0.1fce~0.8fce frequency wave activity(seed acceleration) 0.1fce~0.8fce frequency wave activity(seed acceleration)

Van Allen Probes Van Allen Probes?Van Allen Probes?  Consist of two spacecraft  Orbit: 620 ~ 30,500 km  Inclination: 10°  Period: 9 hr  Observe radiation belt storms with excellent  Observe radiation belt storms with excellent spatial and time resolution spatial and time resolution  Life time: 2 years(Launch July 2012 ~ now)  5 Instruments(EMFISIS, ECT, EFW, RPS, RBSPICE)

Abstract

Electron Local ‘Heating’ Acceleration ~50% storms high-energy electron flux increase ~50% storms high-energy electron flux increase ~25% storms decrease electron flux ~25% storms decrease electron flux 25% storms remain stable 25% storms remain stable Relativistic electron-solar wind speed relationship is not a simple linear one. Relativistic electron-solar wind speed relationship is not a simple linear one. Seed electron L~4.2 Strong southward turning of the IMF Energy into the Earth’s magnetotail Strong southward turning of the IMF Energy into the Earth’s magnetotail Injected by substorm

Event Overview August-September 2014 August-September 2014 GOES-13 electrons GOES-13 electrons keV keV keV keV keV keV >0.8 MeV >0.8 MeV >2.0 MeV >2.0 MeV Solar energetic Particle event occurred Solar energetic Particle event occurred

Event Overview Predicted AE Predicted AE Predicted Dst Predicted Dst Solar wind pressure Solar wind pressure Solar wind velocity Solar wind velocity Velocity >700km/s~ remain >500km/s several days Velocity >700km/s~ remain >500km/s several days HILDCAA intervals (high-intensity, long-duration, continuous AE activity) HILDCAA intervals (high-intensity, long-duration, continuous AE activity) Absence of source population electrons(northward IMF) Absence of source population electrons(northward IMF)

Event Overview VAP data 25 Aug~04 Oct VAP data 25 Aug~04 Oct HOPE, MagEIS, REPT HOPE, MagEIS, REPT Apogee located 5.5 MLT, local time coverage L=4.0 covering ~ MLT Apogee located 5.5 MLT, local time coverage L=4.0 covering ~ MLT Intense occur

Event Overview Pitch angle distribution(12 Sep) Pitch angle distribution(12 Sep) REPT REPT MagEIS MagEIS Quickly build up to prestorm levels Quickly build up to prestorm levels Expect relativistic electron flux increase but strongly depleted Expect relativistic electron flux increase but strongly depleted Magnetopause ‘shadowing’  dropout Magnetopause ‘shadowing’  dropout Particle loss through dayside magnetospheric boundary Particle loss through dayside magnetospheric boundary

Wave activity storm 12 Sep by Chorus wave storm 12 Sep by Chorus wave Recovery 21 Sep by Hiss wave Recovery 21 Sep by Hiss wave

Wave activity POES(850km, 14.1 orbits per day) data over keV to infer chorus wave intensity POES(850km, 14.1 orbits per day) data over keV to infer chorus wave intensity Southward substorm electron injection(02:00 UT on 22) Southward substorm electron injection(02:00 UT on 22)

Wave activity Pc5 power enhanced during main phase of the 12 Sep storm Pc5 power enhanced during main phase of the 12 Sep storm ULF waves played a direct role in the disappearance of the outer belt 13 Sep ULF waves played a direct role in the disappearance of the outer belt 13 Sep

Discussion and Conclusion High solar wind speed leas strong substorm activity High solar wind speed leas strong substorm activity IMF northward during solar wind stream, electron flux level can be quiet low IMF northward during solar wind stream, electron flux level can be quiet low IMF southward most case solar wind stream, produce substorm injection of source and seed electrons IMF southward most case solar wind stream, produce substorm injection of source and seed electrons Without source particle, lower band chorus wave are not produced Without source particle, lower band chorus wave are not produced