Predicting Global Auroral Power: A Merging Term Plus a Viscous Term Works Best P. T. Newell, T. Sotirelis, K. Liou, and C.-I. Meng The Johns Hopkins University.

Slides:



Advertisements
Similar presentations
The Bimodal Solar Wind-Magnetosphere- Ionosphere System George Siscoe Center for Space Physics Boston University ●Vasyliunas Dichotomization Momentum transfer.
Advertisements

Generation of the transpolar potential Ramon E. Lopez Dept. of Physics UT Arlington.
Anti-Parallel Merging and Component Reconnection: Role in Magnetospheric Dynamics M.M Kuznetsova, M. Hesse, L. Rastaetter NASA/GSFC T. I. Gombosi University.
THE ROLE OF MAGNETOSPHERIC LOBES IN SOLAR WIND – MAGNETOSPHERE - IONOSPHERE RELATIONS Koleva R. 1, Grigorenko E. 2 (1) Solar-Terrestrial Influences Laboratory,
SuperDARN Workshop, 2011 Upstream Pc3 ULF wave signatures observed near the Earth's cusp Tim Yeoman Darren Wright (Leicester) Mark Engebretson, Fei Lu,
E. Amata M. Candidi (1), M.F. Marcucci (1), S. Massetti (1), P. Francia (3), U. Villante (3) (1) Istituto di Fisica dello Spazio Interplanetario (IFSI),
The role of solar wind energy flux for transpolar arc luminosity A.Kullen 1, J. A. Cumnock 2,3, and T. Karlsson 2 1 Swedish Institute of Space Physics,
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.
Occurrence and properties of substorms associated with pseudobreakups Anita Kullen Space & Plasma Physics, EES.
Identification and Analysis of Magnetic Substorms Patricia Gavin 1, Sandra Brogl 1, Ramon Lopez 2, Hamid Rassoul 1 1. Florida Institute of Technology,
Solar wind-magnetosphere coupling, substorms, and ramifications for ionospheric convection Steve Milan Adrian Grocott (Leics,
Figure 4: Overview of the geometry of the Rankin Inlet and Inuvik radar in MLT coordinates on Aug 08 th Merged vectors are shown in black. AMPERE.
1 SPACE WEATHER EFFECTS ON SATELLITE DRAG 6 January 2006 Cheryl Huang, Frank A. Marcos and William Burke Space Vehicles Directorate Air Force Research.
Ionospheric Convection and Field-Aligned Currents During Strong Magnetospheric Driving: A SuperDARN/AMPERE Case Study L. B. N. Clausen (1), J. B. H. Baker.
Adrian Grocott *, Steve Milan, Mark Lester, Tim Yeoman University of Leicester, U.K. *currently visiting NIPR, Japan Mervyn Freeman British Antarctic Survey,
Solar wind-magnetosphere coupling Magnetic reconnection In most solar system environments magnetic fields are “frozen” to the plasma - different plasmas.
2011 SuperDARN Workshop, Hanover, NH 1 Quantitative comparison of cross polar cap potential as derived from AMIE, DMSP, SuperDARN Elsayed R. Talaat 1,
State Key Laboratory of Space Weather An inter-hemisphere asymmetry of the cusp region against the geomagnetic dipole tilt Jiankui Shi Center for Space.
Periodicities of the Solar Wind, Global Electron Power, and Other Indices in 2005 in HSS Barbara A. Emery (NCAR), Ian G. Richardson (GSFC), David S. Evans.
1 Geomagnetic/Ionospheric Models NASA/GSFC, Code 692 During the early part of April 6, 2000 a large coronal “ejecta” event compressed and interacted with.
Radio and Space Plasma Physics Group The formation of transpolar arcs R. C. Fear and S. E. Milan University of Leicester.
M. Menvielle and A. Marchaudon ESWW2 M. Menvielle (1) and A. Marchaudon (2) (1) Centre d’études des Environnements Terrestre et Planétaires UMR 8615 IPL/CNRS/UVSQ.
Solar wind-magnetosphere- atmosphere coupling: effects of magnetic storms and substorms in atmospheric electric field variations Kleimenova N., Kozyreva.
Mervyn Freeman British Antarctic Survey
1 Saturn Aurora: The ionospheric and magnetospheric fingerprint, and a manifestation of interactions beyond. Saturn Aurora: The ionospheric and magnetospheric.
Space Weather Models running in real-time or forecasting mode Yihua Zheng SW REDI 2014.
Magnetospheric ULF wave activity monitoring based on the ULF-index OLGA KOZYREVA and N. Kleimenova Institute of the Earth Physics, RAS.
Kp Forecast Models S. Wing 1, Y. Zhang 1, and J. R. Johnson 2 1 Applied Physics Laboratory, The Johns Hopkins University 2 Princeton Plasma Physics Laboratory,
Magnetosphere-Ionosphere coupling processes reflected in
Space Science MO&DA Programs - September Page 1 SS It is known that the aurora is created by intense electron beams which impact the upper atmosphere.
MAGNETOSPHERIC RESPONSE TO COMPLEX INTERPLANETARY DRIVING DURING SOLAR MINIMUM: MULTI-POINT INVESTIGATION R. Koleva, A. Bochev Space and Solar Terrestrial.
Specifying Instantaneous Currents and Electric Fields in the High-Latitude Ionosphere FESD-ECCWES Meeting, 21 July 20141/15 Ellen Cousins 1, Tomoko Matsuo.
Intense Poynting flux at very high latitudes during magnetic storms: GITM simulation results Yue Deng 1 Cheng Sheng 1, Manqi Shi 1, Yanshi Huang 2, Cheryl.
Testing the Equipotential Magnetic Field Line Assumption Using SuperDARN Measurements and the Cluster Electron Drift Instrument (EDI) Joseph B. H. Baker.
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.
Relating the Equatorward Boundary of the Diffuse Redline Aurora to its Magnetospheric Counterpart Grant, Jeff 1 ; Donovan, Eric 1 ; Spanswick, Emma 1 ;
June 30, 2011 Plasma Pressure Constraints on Magnetic Field Structure in the Substorm Growth Phase Sorin G. Zaharia 1 and Chih-Ping Wang.
Guan Le NASA Goddard Space Flight Center Challenges in Measuring External Current Systems Driven by Solar Wind-Magnetosphere Interaction.
New Science Opportunities with a Mid-Latitude SuperDARN Radar Raymond A. Greenwald Johns Hopkins University Applied Physics Laboratory.
Study on the Impact of Combined Magnetic and Electric Field Analysis and of Ocean Circulation Effects on Swarm Mission Performance by S. Vennerstrom, E.
1 The Solar Wind - Magnetosphere Coupling Function and Nowcasting of Geomagnetic Activity Leif Svalgaard Stanford University AMS-93, Austin, Jan
© Research Section for Plasma and Space Physics UNIVERSITY OF OSLO Daytime Aurora Jøran Moen.
Substorms: Ionospheric Manifestation of Magnetospheric Disturbances P. Song, V. M. Vasyliūnas, and J. Tu University of Massachusetts Lowell Substorms:
Swedish Institute of Space Physics, Kiruna M. Yamauchi 1 Different Sun-Earth energy coupling between different solar cycles Acknowledgement:
ECLAT Cluster Footprint Mapping. ECLAT meeting March 2012 WP330 Cluster footprint mapping 1.Cluster footprint mapping using statistical magnetospheric.
SuperDARN Observations of ULF Pulsations During a Substorm Expansion Phase Onset N. A. Frissell, J. B. H. Baker, J. M. Ruohoniemi, L. B. N. Clausen, R.
TBD: Contributions of MIT Coupling to Important Features… Open-closed field line boundary Equatorward boundaries of particle precipitation Plasmapause.
Bob Weigel George Mason University.  “We are still in the process of identifying characteristic behavior that identifies various modes as separate phenomena.”
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
Dynamics of the auroral bifurcations at Saturn and their role in magnetopause reconnection LPAP - Université de Liège A. Radioti, J.-C. Gérard, D. Grodent,
Data-Model Comparisons
Paul Song Center for Atmospheric Research
Dynamics of the AMPERE R1 Oval during substorms and SMCs
The Ionosphere and Thermosphere GEM 2013 Student Tutorial
High-latitude Neutral Density Maxima
Disturbance Dynamo Effects in the Low Latitude Ionosphere
TIEGCM with AMIE RENU Rocket Cusp Density
Space Weather Activities in China
The Physics of Space Plasmas
Penetration Jet DMSP F April MLT
Yama's works Using geomagnetic data
Yuki Takagi1*, Kazuo Shiokawa1, Yuichi Otsuka1, and Martin Connors2  
J.F. Carbary1, D.G. Mitchell1, P. Kollmann1,
Swedish Institute of Space Physics, Kiruna
P. Stauning: The Polar Cap (PC) Index for Space Weather Forecasts
Dynamic Coupling between the Magnetosphere and the Ionosphere
by Andreas Keiling, Scott Thaller, John Wygant, and John Dombeck
Added-Value Users of ACE Real Time Solar Wind (RTSW) Data
Presentation transcript:

Predicting Global Auroral Power: A Merging Term Plus a Viscous Term Works Best P. T. Newell, T. Sotirelis, K. Liou, and C.-I. Meng The Johns Hopkins University Applied Physics Laboratory Laurel, Maryland, 20723

Motivation If thousands (or tens of thousands) of data points over multiple years are used, which, among the various coupling functions proposed, works best? If the exercise is repeated for multiple disparate data sets, does a pattern emerge?

Popular Coupling Functions (In ascending order of merit) B z  = vB 2 sin 4 (  c /2)  Akasofu-Perrault) Bs vBs(half-wave rectifier) E KL = vB T sin 2 (  c /2) (Kan-Lee electric field) E WAV = vB T sin 4 (  c /2) (Wygant’s “intermediate”) where  c = arctan(B y /B z )

Approach Ten characterizations of the magnetosphere were examined over multiyear periods at relatively high cadence (hourly) Scores of coupling functions were tested, searching for a pattern (performance of 32 functions documented) ab inito: No use of the time history of the target index

Data 5 Traditional (ground-based magnetometer) indices: AE, AU, AL, Kp, and Dst 5 Space-age indices: Auroral power (Polar UVI), cusp latitude (sin(  c )) and b2i (ion equatorward boundary of multi-keV ion precipitation), both from DMSP, magnetotail inclination angle (arctan(v/h)) from GOES-8, and polar cap flux (  PC ) from SuperDARN as calibrated to DMSP

Main Result A single coupling function correlates best with 9/10 indices (11 data runs, counting multiple solar cycles) d  MP /dt = v 4/3 B T 2/3 sin 8/3 (  c /2) The exception is Dst. Dst correlates best (r=0.87) with p 1/2 d  MP /dt

Meaning of d  MP /dt Dayside merging voltage is the product of three factors: · solar wind electric field, vB T ·length of merging line, ~(B MP /B T ) 1/3 · % of lines which merge, sin 8/3 (  c /2) · Note that B MP (~v) d  MP /dt = v 4/3 B T 2/3 sin 8/3 (  c /2)

What is the form for the best viscous term? If two terms are used, is it best to used two highly performing coupling functions (both of which would be merging related) or one merging term and one viscous term? We now know the optimized merging estimator. Here we pursue two follow up questions

Twenty Viscous Candidates n, v, nv, p (nv 2 /2), p 2, p 1/2, etc. The highest performing viscous function out of the 20 considered is: n 1/2 v 2

What is the optimal pair of terms? Is it best to use two highly performing terms (such as the Kan-Lee electric field and d  MP /dt)? Or is it best to combine a merging term and a viscous term? And if so, is the best combination the obvious choice (best merging term plus best viscous term)?

496 Possible Combinations With 20 viscous-related terms and 12 merging- related terms (32 in all) there are 496 possible distinct combinations We evaluated the ability of all 496 combinations to predict 10 different indices (such as Kp, cusp latitude, auroral power etc) over multi-year periods at hourly cadence

Summary The best performing viscous term is n 1/2 v 2 Out of the 496 unique pairs from 32 coupling functions, the optimal pair is d  MP /dt with n 1/2 v 2 Any reasonable merging term coupled with any reasonable viscous term does well d  MP /dt and n 1/2 v 2 together form a “tool kit” for model construction