THEMIS GBO/ASI Minor intensification GBAY 01:48:42 KUUJ 01:48:51

Slides:



Advertisements
Similar presentations
Occurrence and properties of substorms associated with pseudobreakups Anita Kullen Space & Plasma Physics, EES.
Advertisements

The Upgraded and Expanded CARISMA Magnetometer Array: New Pi1 Substorm Science Capabilities I.J. Rae, Ian R. Mann (PI), K. Murphy, David K. Milling (PM),
Observations of the ballooning and interchange instabilities in the near-Earth magnetotail at substorm expansion onsets Yukinaga Miyashita (STEL, Nagoya.
Substorm Parameters: A Progress Report Christine Gabrielse Sergey Apatenkov, Nathaniel Frissell, Stefan Kiehas, Jiang Liu, Kyle Murphy,
Onsets and Flapping Studied using a Dynamic Harris Sheet Model M. Connors 1, R. Lerner 1, G. Jaugey 2, B. Lavraud 3, M. Volwerk 4, R. L. McPherron 5 1.
THEMIS first results 1 THEMIS JGR, Due: 4/15/2008 Major conjunction Mar 01 –1:52 substorm 2:15 intensification 2:30 intensification –3:35 substorm 3:55.
Observation and Theory of Substorm Onset C. Z. (Frank) Cheng (1,2), T. F. Chang (2), Sorin Zaharia (3), N. N. Gorelenkov (4) (1)Plasma and Space Science.
CASCADES-2: A View from THEMIS John Bonnell Space Sciences Laboratory UC Berkeley What can THEMIS provide? Multi-point magnetospheric observations of particles.
Magnetometer Tutorial PowerPoint March, 2007 THEMIS: The Science Behind Magnetometer Signatures Laura Peticolas GEONS workshop.
Magnetoseismology: Pi 2 Travel Time Peter Chi (IGPP/UCLA) 2008 GEM Summer Workshop, Miday, Utah 1998-Jul-22 ▲Maximum deviation in  H-  D plane Pi 2 arrival.
Finite Gyroradius Effect in Space and Laboratory 1. Radiation belt (Ring current) 2. Auroral phenomena (Substorm current) 3. Shock acceleration and upstream.
Thursday, May 14, 2009Cluster Workshop – UppsalaR. J. Strangeway – 1 The Auroral Acceleration Region: Lessons from FAST, Questions for Cluster Robert J.
1 Cambridge 2004 Wolfgang Baumjohann IWF/ÖAW Graz, Austria With help from: R. Nakamura, A. Runov, Y. Asano & V.A. Sergeev Magnetotail Transport and Substorms.
THEMIS and ARTEMIS David G. Sibeck THEMIS Project Scientist NASA/GSFC 2/17/2007 Cape Canaveral.
Aurora, Substorms, and THEMIS D. G. Sibeck NASA/GSFC THEMIS Project Scientist.
Magnetosphere-Ionosphere coupling processes reflected in
EISCAT-Cluster observations of quiet-time near-Earth magnetotail fast flows and their signatures in the ionosphere Nordic Cluster Meeting, Uppsala, Sweden,
Constraining Substorm Onset from Space- and Ground-Based Observations Department of Space & Climate Physics Mullard Space Science Laboratory A. P. Walsh.
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.
A T Y Lui, V Angelopoulos, S B Mende, O LeContel, H Frey, E Donovan, D G Sibeck, W Liu, H U Auster, X Li, M Nose, and M O Fillingim Outline  Conjunction.
MAGNETOSPHERIC RESPONSE TO COMPLEX INTERPLANETARY DRIVING DURING SOLAR MINIMUM: MULTI-POINT INVESTIGATION R. Koleva, A. Bochev Space and Solar Terrestrial.
Magnetic Flux Transport and Pressure Variations at Magnetotail Plasma Flow Bursts during Geomagnetically Quiet Times Motoharu Nowada ( 野和田 基晴 :
GEM 2008 Summer Workshop, Zermatt, Utah, June 25, Institute of Geophysics and Planetary Physics University of California, Los Angeles THEMIS observations.
THEMIS SWT, SSL Berkeley, Dec 20, THEMIS First Tail Season: What Did We Learn? In-situ data analyst view.
Recent THEMIS and coordinated GBO measurements of substorm expansion onset: Do we finally have an answer? Larry Kepko NASA/Goddard Space Flight Center.
Cluster observations of a reconnection site at high- latitude magnetopause Y. Khotyaintsev (1), A. Vaivads (1), Y. Ogawa (1,2), M. André(1), S. Buchert(1),
GEOSYNCHRONOUS SIGNATURES OF AURORAL SUBSTORMS PRECEDED BY PSEUDOBREAKUPS A. Kullen (1), S. Ohtani (2), and H. Singer (3) A. Kullen (1), S. Ohtani (2),
ESS 7 Lecture 13 October 29, 2008 Substorms. Time Series of Images of the Auroral Substorm This set of images in the ultra-violet from the Polar satellite.
Simultaneous in-situ observations of the feature of a typical FTE by Cluster and TC1 Zhang Qinghe Liu Ruiyuan Polar Research Institute of China
Substorm-origin sub-keV ring current ions: wedge-like structure ICS-9, Graz, ~7 Substorm : production of plasma Sub-keV ring current : fossil of.
Sani 1 June 15, 2009 Introduction on bursty flows Particle distributions and ion acceleration Electron acceleration and effects Linear and non-linear waves:
Cluster 911 Plasmoid Substorm Sept 11, 2002 DOY 254 Onset at 1600 UT Shock at Cluster 16:23 Plasmoid 16: :40 UT.
Magnetic reconnection in the magnetotail: Geotail observations T. Nagai Tokyo Institute of Technology World Space Environment Forum 2005 May 4, 2005 Wednesday.
Emma Spanswick & Eric Donovan SS Injection Region Ionospheric Observations Magnetospheric Observations Physical boundaries magnetospheric models Correlation.
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.
Joint Cluster-THEMIS SWT 1 Sep 23-26, 2008 Vassilis Angelopoulos, James P. McFadden, Davin Larson, Charles W. Carlson, Stephen B. Mende, Harald Frey, Tai.
Substorm Parameters: A Progress Report Christine Gabrielse Sergey Apatenkov, Nathaniel Frissell, Stefan Kiehas, Jiang Liu, Kyle Murphy,
 Morphology and Dynamics of Auroral Arcs By Sarah Bender Mentor: Kyle Murphy 8/7/2014.
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.
Cluster observation of electron acceleration by ULF Alfvén waves
The Magnetospheric Source Location of the Proton Aurora
THEMIS Science Progress NASA/GSFC, Oct 26, 2007
Recent KTH Cluster research
Definitive Mapping in the Late Growth Phase
E. Spanswick, E. Donovan, J. Liang, J. McFadden, T. -S. Hsu, C. -P
Substorm current wedge, Alfven waves, ion injections, Pi2 pulsations, and ion outflows: A THEMIS look The THEMIS team.
Evidence for Dayside Interhemispheric Field-Aligned Currents During Strong IMF By Conditions Seen by SuperDARN Radars Joseph B.H. Baker, Bharat Kunduri.
Sources of < 10 keV ring current ions: supply mechanism?
The Physics of Space Plasmas
THEMIS observations at a substorm onset on March 1, 2008
Magnetospheric solitary structure maintained by 3000 km/s ions as a cause of westward moving auroral bulge at 19 MLT M. Yamauchi1, I. Dandouras2, P.W.
Substorm current wedge, Alfven waves, ion injections, Pi2 pulsations, and ion outflows: A THEMIS look The THEMIS team.
THEMIS SWG, Annapolis, Sept. 14, 2011 Supported by NSF grant #
Yama's works Using geomagnetic data
First 10 months (Feb 2007-Dec 2007)
On Feb 12, a minor THEMIS conjunction, TH-C at 18RE in the tail, observed the first indication of reconnection Earthward of it. Substorm ~03:00-04:30UT.
March 23 J. McFadden UC Berkeley SSL.
Analysis of Substorms during the Second THEMIS Tail Season
Magnetospheric solitary structure maintained by 3000 km/s ions as a cause of westward moving auroral bulge at 19 MLT M. Yamauchi1, I. Dandouras2, P.W.
High-Speed Plasma Flows Observed in the Magnetotail during Geomagemtically Quiet Times: Relationship between Magnetic Reconnection, Substorm and High-Speed.
THEMIS Summary Data Plots
1IGPP/UCLA, 2SSL/UCB, 3LASP, 4Univ. Calgary, 5TUB, 6UNH
Magnetic reconnection X-line crossing by THEMIS-B on February 7, 2009
A statistical study of Cluster and ground-based observations of Pi1B pulsations at substorm onset Marc Lessard1, Eric Lund1, Christopher Mouikis1, Yasong.
Determination of the Substorm Initiation Region From a Major Conjunction Interval of THEMIS Satellites A T Y Lui, V Angelopoulos, S B Mende, O LeContel,
Determination of the Substorm Initiation Region From a Major Conjunction Interval of THEMIS Satellites A T Y Lui, V Angelopoulos, S B Mende, O LeContel,
Dynamics of reconnection and multiple activation of substorms
Determination of the Substorm Initiation Region From a Major Conjunction Interval of THEMIS Satellites A T Y Lui, V Angelopoulos, S B Mende, O LeContel,
Three Regions of Auroral Acceleration
PBI by definition Optical data THEMIS data Rocket data
Presentation transcript:

THEMIS GBO/ASI Minor intensification GBAY 01:48:42 KUUJ 01:48:51 CHBG 01:49:39 SNKQ 01:50:54 GILL 01:51:18 TPAS 01:51:21 Major intensification (substorm) GBAY 01:55:36 KUUJ 01:55:21 CHBG 01:56:33 SNKQ 01:52:27 GILL 01:54:21 TPAS 01:54:30

THEMIS SC, GBO and GOES observations 08-03-01/0100 – 0210 UT P1 KUUJ P2 P3 P4 G12 G10 GBAY 01:48:50 UT 0148:42 0154:21

P1 and P2: X=-22.7, -17.4 RE

P1 P2

Timing of HE particles (P1 and P2 SST) First tailward burst 0148:42 UT 0148:42 UT 134 keV

P3 and P4: X=-9.5, -8.0 RE

Magnetic field variations at P3, P4, GOES 10, GOES 12 P3 and P4 FGM measurements: Total field (Bt) at P3 and P4 continuously increases until ~0955 UT Variations of the components, (baseline subtracted): δBy and δBz started at 0148:20 – 0148:40 UT, indicating outward FAC underneath the SC, while Bx and Bt were increasing (the total current built up) until ~0154:30UT (current reduction/disruption). CR/CD P4  P3: Tailward at a velocity of 150 km/s GOES 10: Positive δBn (eastward!) at 0148- 0155 UT G10 was under the FAC GOES10, 12: Dipolarization started at ~0155 UT

2008-03-01/0140 – 0205 UT First activation 0148:20: HE electron flux increase at P2 0148:20: ~150 keV ion flux increase at P2 0148:30: minor δBy at P3 & P4 0148:42: Auroral onset at GBAY 0148:45: PI2 onset at GBAY 0148:50: δBy and δBz at P2/THC 0148:50: Tailward flow at P2/THC 0149:30: δBy and δBz at P1/THB 0149:30: Tailward flow at P1/THB 0149:30: major δBy δBz at P3 & P4 Second activation (substorm) 0154:21: Auroral onset at KUUJ 0154:30: Tailward flow at P1 0154:30: δBy, δBz at P2 0155:00: Tailward flow at P2 0155:00: Drop of Bt at P4 0155:00: Dipolarization at P4 0155:00: δVy, δVz at P4 0155:50: Drop of Bt at P3 0155:50: Dipolarization at P3 0155:50: δVy znd δVz at P3 Signatures in space and in the ionosphere are seen within 20 s! Current reduction /CD at X~-8 RE and plasma acceleration at X~-17 RE acted almost simultaneously (independently?)

3 variants of mapping: TIPSOD (T96?), T96 SW, Event Oriented (EO) THEMIS ASI P1 T96 SW TIPSOD P2 EO P3 P4 G12 G10 GBAY 3 variants of mapping: TIPSOD (T96?), T96 SW, Event Oriented (EO)