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The First Space-Weather Numerical Forecasting Model & Reconstruction of Halo CMEs

The First Space-Weather Numerical Forecasting Model & Reconstruction of Halo CMEs

The First Space-Weather Numerical Forecasting Model & Reconstruction of Halo CMEs. Xuepu Zhao http://sun.stanford.edu/~xuepu xpzhao98@yahoo.com NAOC Oct. 20, 2011. 1. The first space-weather numerical forecasting model. NSF Press Release, 26 Jan 2011 :

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411 views • 28 slides
Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau

Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau

CME Mythology: Do Global CMEs or Sympathetic CMEs Exist?. International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado. Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau. Halo CMEs: a new quality from SOHO.

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488 views • 27 slides
Solar Sources of Large Geomagnetic Storms During Solar Cycle 23

Solar Sources of Large Geomagnetic Storms During Solar Cycle 23

Solar Sources of Large Geomagnetic Storms During Solar Cycle 23. Gopalswamy (NASA/GSFC) Michalek, H. Xie, S. Yashiro (CUA) R. A. Howard (NRL). Objective.

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416 views • 27 slides
B. CME in In-situ data sets at Earth

B. CME in In-situ data sets at Earth

B. CME in In-situ data sets at Earth. Yuko Hada Chi- Ju Wu 2012/01/24. We select 4 events from CME catalog. ? All events are Halo CMEs. Today, I show you only March event. (Because I cannot study deeply. ). 2012/03/04. Left: SOHO/LASCO C2 Right: SOHO/LASCOC3.

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280 views • 18 slides
Validating One-point Inversion Solution of the Elliptic Cone Model for Full-Halo CMEs

Validating One-point Inversion Solution of the Elliptic Cone Model for Full-Halo CMEs

Validating One-point Inversion Solution of the Elliptic Cone Model for Full-Halo CMEs. X. P. Zhao Stanford University H. Cremades, UTN-FRM / CONICET SSH31A -0227 AGU Fall Meeting, December 12, 2007. Abstract

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297 views • 18 slides
X. P. Zhao, H. Cremades, J. T. Hoeksema, Y. Liu CISM All-hand Meeting, Boston September 17, 2007

X. P. Zhao, H. Cremades, J. T. Hoeksema, Y. Liu CISM All-hand Meeting, Boston September 17, 2007

Determination of Geometrical and Kinematical Properties of Disk Halo CMEs Using the Elliptic Cone Model. X. P. Zhao, H. Cremades, J. T. Hoeksema, Y. Liu CISM All-hand Meeting, Boston September 17, 2007. 1. Introduction.

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281 views • 18 slides
Inverting Geometrical Properties of 3-D Rope-like CMEs From 2-D Frontside Halo CMEs

Inverting Geometrical Properties of 3-D Rope-like CMEs From 2-D Frontside Halo CMEs

Inverting Geometrical Properties of 3-D Rope-like CMEs From 2-D Frontside Halo CMEs. Xuepu Zhao Stanford University SH23B-1635-- Dec. 16, 2008-- MC Hall D. Abstract. By using an elliptic cone model to mimic the 3-D rope-like CME structure, we have developed inversion

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295 views • 18 slides
Anemone Structure of AR NOAA 10798 and Related Geo-Effective Flares and CMEs

Anemone Structure of AR NOAA 10798 and Related Geo-Effective Flares and CMEs

Anemone Structure of AR NOAA 10798 and Related Geo-Effective Flares and CMEs. A. Asai 1 ( ?? ? ), T.T. Ishii 2 , K. Shibata 2 , N. Gopalswamy 3 1: Nobeyama Solar Radio Observatory, NAOJ 2: Kyoto University 3: NASA/GSFC. COSPAR2006-A-02406; D2.1-0023-06

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246 views • 17 slides
ZEC Model parameters of 20100801 Halo CMEs

ZEC Model parameters of 20100801 Halo CMEs

ZEC Model parameters of 20100801 Halo CMEs. Xuepu Zhao Jan. 18, 2011. 1. Observation.

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243 views • 17 slides
Anemone Structure and Geo-Effective Flares/CMEs

Anemone Structure and Geo-Effective Flares/CMEs

Anemone Structure and Geo-Effective Flares/CMEs. A. Asai 1 , T.T. Ishii 2 , K. Shibata 2 , N. Gopalswamy 3 , R. Kataoka 4 , M. Oka 2 1: Nobeyama Solar Radio Observatory, NAOJ 2: Kyoto University 3: NASA/GSFC 4: STE-Lab., Nagoya University. CSWM Workshop @Yokohama 2006 November 13 - 17.

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269 views • 15 slides

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