4,126 Cmes PPTs View free & download

Inverting Geometrical Properties of 3D Ropelike CMEs From 2D Frontside Halo CMEs PowerPoint PPT Presentation

Inverting Geometrical Properties of 3D Ropelike CMEs From 2D Frontside Halo CMEs - of 3-D rope-like CMEs can be more accurately inverted. for MOST ... 1. Three types of ... Note: the halo params for right three CME halos are exactly the ...

of 3-D rope-like CMEs can be more accurately inverted. for MOST ... 1. Three types of ... Note: the halo params for right three CME halos are exactly the ...

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Disentangling the Magnetic Flux Rope Topology from CMEs Do All Regular CMEs Contain Flux Ropes PowerPoint PPT Presentation

Disentangling the Magnetic Flux Rope Topology from CMEs Do All Regular CMEs Contain Flux Ropes - Disentangling the Magnetic Flux Rope Topology from CMEs. Do All Regular ... C. Jacobs1, N. Lugaz2, I. Roussev2 and S. Poedts1. 2. 1. submitted to ApJ Letters ...

Disentangling the Magnetic Flux Rope Topology from CMEs. Do All Regular ... C. Jacobs1, N. Lugaz2, I. Roussev2 and S. Poedts1. 2. 1. submitted to ApJ Letters ...

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CMES - CMES La sant par le sport * * * * * * * * * Notre engagement Convaincu que le sport doit jouer un r le dans la soci t , et que l activit physique am liore ...

CMES La sant par le sport * * * * * * * * * Notre engagement Convaincu que le sport doit jouer un r le dans la soci t , et que l activit physique am liore ...

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Estimating the CMEs propagation PowerPoint PPT Presentation

Estimating the CMEs propagation - Contents. The instrument and the Data. Description of the Method. Geometry. 3D ... Vb = 253 km/s. V = 548 km/s. Summary. Using HT diagrams on SECCHI-COR1 data: ...

Contents. The instrument and the Data. Description of the Method. Geometry. 3D ... Vb = 253 km/s. V = 548 km/s. Summary. Using HT diagrams on SECCHI-COR1 data: ...

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CMEs OBSERVED IN THE HELIOSPHERE BY PowerPoint PPT Presentation

CMEs OBSERVED IN THE HELIOSPHERE BY - CMEs OBSERVED IN THE HELIOSPHERE BY THE SOLAR MASS EJECTION IMAGER (SMEI) David Webb, D. Mizuno & T. Kuchar, Boston College J. Johnston & R. Radick, Air Force ...

CMEs OBSERVED IN THE HELIOSPHERE BY THE SOLAR MASS EJECTION IMAGER (SMEI) David Webb, D. Mizuno & T. Kuchar, Boston College J. Johnston & R. Radick, Air Force ...

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CMEs Associated With Impulsive Flares PowerPoint PPT Presentation

CMEs Associated With Impulsive Flares - Flare-Associated Motions and CMEs (diffuse motion (wave?) -- big CME) ... What is the origin of some of coronal waves and metric type II burst? ...

Flare-Associated Motions and CMEs (diffuse motion (wave?) -- big CME) ... What is the origin of some of coronal waves and metric type II burst? ...

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Tracking CMEs from Sun to Earth PowerPoint PPT Presentation

Tracking CMEs from Sun to Earth - Tracking CMEs from Sun to Earth M. Temmer1, C. M stl2, A. Veronig1, O. Flor1, T. Rollett1,2 1 Kanzelh he Observatory/IGAM, Institute of ...

Tracking CMEs from Sun to Earth M. Temmer1, C. M stl2, A. Veronig1, O. Flor1, T. Rollett1,2 1 Kanzelh he Observatory/IGAM, Institute of ...

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Multiscale Detection and Characterisation of CMEs PowerPoint PPT Presentation

Multiscale Detection and Characterisation of CMEs - Multiscale Detection and Characterisation of CMEs J. P. Byrne1, P. T. Gallagher1, C. A. Young2 and R. T. J. McAteer3 1 Astrophysics Research Group, School of Physics ...

Multiscale Detection and Characterisation of CMEs J. P. Byrne1, P. T. Gallagher1, C. A. Young2 and R. T. J. McAteer3 1 Astrophysics Research Group, School of Physics ...

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To Get your CMEs PowerPoint PPT Presentation

To Get your CMEs - You may type your question here during the 'live' presentation or call our ... Post-herpetic neuralgia. Diarrhea. Assessment. Onset, frequency, consistency, color ...

You may type your question here during the 'live' presentation or call our ... Post-herpetic neuralgia. Diarrhea. Assessment. Onset, frequency, consistency, color ...

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To Get your CMEs - Sign in, look for the title of this seminar. Follow directions to register ... 2 reactivation activated CD4 cells infiltrate mucosa ready targets for HIV ...

Sign in, look for the title of this seminar. Follow directions to register ... 2 reactivation activated CD4 cells infiltrate mucosa ready targets for HIV ...

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2003 October-November CMEs PowerPoint PPT Presentation

2003 October-November CMEs - Structure and energy of potential field for AR484, 486, and 488 ... backside. 53 -44.5. 1206 -59.5. 1523. 17:30. 11/06/03. AR0486. 34 -385.5. 2996. 434.8. 2657 ...

Structure and energy of potential field for AR484, 486, and 488 ... backside. 53 -44.5. 1206 -59.5. 1523. 17:30. 11/06/03. AR0486. 34 -385.5. 2996. 434.8. 2657 ...

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Radio bursts and CMEs PowerPoint PPT Presentation

Radio bursts and CMEs - Cadence 1s 600 km/s. Continuum. 17 March 2002 Event B. 17 March 2002 Event A ... AR 9871 inside old remnant region. Inclusion of small interacting loops ...

Cadence 1s 600 km/s. Continuum. 17 March 2002 Event B. 17 March 2002 Event A ... AR 9871 inside old remnant region. Inclusion of small interacting loops ...

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An Emerging Flux Trigger Model for CMEs - An Emerging Flux Trigger Model for CMEs

An Emerging Flux Trigger Model for CMEs

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Hard Xrays associated with CMEs PowerPoint PPT Presentation

Hard Xrays associated with CMEs - Direct coronal observations of Type II bursts (Shibata presentation) ... Limb occultation allows us to see hard X-rays from the middle corona ...

Direct coronal observations of Type II bursts (Shibata presentation) ... Limb occultation allows us to see hard X-rays from the middle corona ...

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CMEs, CIRs, and Space Weather PowerPoint PPT Presentation

CMEs, CIRs, and Space Weather - none

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Future Improvements in European CMECPD: PowerPoint PPT Presentation

Future Improvements in European CMECPD: - UK. IR. IT. GR. CR. AT. CH. DE. BL. DK. NL. RO. FI. CZ. HG. SL. European ... Continuing medical education (CME) systems are already in ... insurance ...

UK. IR. IT. GR. CR. AT. CH. DE. BL. DK. NL. RO. FI. CZ. HG. SL. European ... Continuing medical education (CME) systems are already in ... insurance ...

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Lecture 4 The Formation and Evolution of CMEs PowerPoint PPT Presentation

Lecture 4 The Formation and Evolution of CMEs - Lecture 4 The Formation and Evolution of CMEs Coronal Mass Ejections (CMEs) Appear as loop like features that breakup helmet streamers in the corona.

Lecture 4 The Formation and Evolution of CMEs Coronal Mass Ejections (CMEs) Appear as loop like features that breakup helmet streamers in the corona.

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A new view: flares and CMEs PowerPoint PPT Presentation

A new view: flares and CMEs - A new view: flares and CMEs. Louise K Harra ... Gemma Attrill's talk tomorrow: Physical properties of coronal waves and associated dimmings ...

A new view: flares and CMEs. Louise K Harra ... Gemma Attrill's talk tomorrow: Physical properties of coronal waves and associated dimmings ...

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Coronal Mass Ejections 4: Modeling CMEs PowerPoint PPT Presentation

Coronal Mass Ejections 4: Modeling CMEs - Flare energy and the CME kinetic energy must be tightly correlated ... Formed before (Low, 2001) or during (Gosling et al., 1990) eruption? ...

Flare energy and the CME kinetic energy must be tightly correlated ... Formed before (Low, 2001) or during (Gosling et al., 1990) eruption? ...

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In Situ Observations of CMES in the Heliosphere PowerPoint PPT Presentation

In Situ Observations of CMES in the Heliosphere - In Situ Observations of CMES. in the Heliosphere ... [e.g., Gosling, 1990; Neugebauer and Goldstein, 1997] Variability in counter-streaming electrons ...

In Situ Observations of CMES. in the Heliosphere ... [e.g., Gosling, 1990; Neugebauer and Goldstein, 1997] Variability in counter-streaming electrons ...

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Reconstruction of CMEs from coordinated imaging and in situ observations - Reconstruction of CMEs from coordinated imaging and in situ observations

Reconstruction of CMEs from coordinated imaging and in situ observations

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THEORY OF SOLAR MAGNETIC FLUX ROPES: CMEs DYNAMICS PowerPoint PPT Presentation

THEORY OF SOLAR MAGNETIC FLUX ROPES: CMEs DYNAMICS - ... div B = 0. Demand that there be no singularities and that ... That is, find p(r), Jp(r), and Jt(r). Describe the physical meaning of the parameter q? ...

... div B = 0. Demand that there be no singularities and that ... That is, find p(r), Jp(r), and Jt(r). Describe the physical meaning of the parameter q? ...

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CMEs in Soft X-rays, impulsive flares, and homology PowerPoint PPT Presentation

CMEs in Soft X-rays, impulsive flares, and homology - CMEs in Soft X-rays, impulsive flares, and homology. Early SXT literature by Uchida et al., Klimchuk et al, Hudson et al., Manoharan ...

CMEs in Soft X-rays, impulsive flares, and homology. Early SXT literature by Uchida et al., Klimchuk et al, Hudson et al., Manoharan ...

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When will disruptive CMEs impact Earth? Coronagraph observations alone aren PowerPoint PPT Presentation

When will disruptive CMEs impact Earth? Coronagraph observations alone aren - When will disruptive CMEs impact Earth? Coronagraph observations alone aren t enough to make the forecast for the most geoeffective halo CMEs.

When will disruptive CMEs impact Earth? Coronagraph observations alone aren t enough to make the forecast for the most geoeffective halo CMEs.

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Orientations of Halo CMEs and Magnetic Clouds PowerPoint PPT Presentation

Orientations of Halo CMEs and Magnetic Clouds - Elongation of a halo CME closely matches the orientation of the erupting ... For about 60% of events the halo elongation and the MC orientation correspond to ...

Elongation of a halo CME closely matches the orientation of the erupting ... For about 60% of events the halo elongation and the MC orientation correspond to ...

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Orientations of Halo CMEs and Magnetic Clouds - 36th COSPAR, 17-22 July 2006, Beijing, CHINA. Oct 28 and Nov 18 2003 Events. Nov 18 2003 ... 36th COSPAR, 17-22 July 2006, Beijing, CHINA ...

36th COSPAR, 17-22 July 2006, Beijing, CHINA. Oct 28 and Nov 18 2003 Events. Nov 18 2003 ... 36th COSPAR, 17-22 July 2006, Beijing, CHINA ...

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Characteristics of Mode Parameters in the Source Regions of CMEs: A First Look PowerPoint PPT Presentation

Characteristics of Mode Parameters in the Source Regions of CMEs: A First Look - Characteristics of Mode Parameters in the Source Regions of CMEs: A First Look ... 2001-2003 within 30 of the central meridian to avoid fore-shortening effect. ...

Characteristics of Mode Parameters in the Source Regions of CMEs: A First Look ... 2001-2003 within 30 of the central meridian to avoid fore-shortening effect. ...

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Magnetic Structure and Evolution of CMEs: From Their Photospheric Source Regions to the Heliosphere - Magnetic Structure and Evolution of CMEs: From Their Photospheric Source Regions to the Heliosphere

Magnetic Structure and Evolution of CMEs: From Their Photospheric Source Regions to the Heliosphere

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Numerical Challenges in Modeling CMEs and SEP Events PowerPoint PPT Presentation

Numerical Challenges in Modeling CMEs and SEP Events - Emission is seen from top of the band (14 MHz) down to ~ 8 MHz and at ~ 14:05-15: ... a bewildering complex of many narrow-band emissions drifting downward from ~ 3-1 ...

Emission is seen from top of the band (14 MHz) down to ~ 8 MHz and at ~ 14:05-15: ... a bewildering complex of many narrow-band emissions drifting downward from ~ 3-1 ...

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Specification of the broad shell of dense plasma for halo CMEs PowerPoint PPT Presentation

Specification of the broad shell of dense plasma for halo CMEs - Halo CMEs are interpreted as the Thompson scattering of a broad shell or bubble ... Recent UV observations show that most of halo CMEs are ice cream cone-like. ...

Halo CMEs are interpreted as the Thompson scattering of a broad shell or bubble ... Recent UV observations show that most of halo CMEs are ice cream cone-like. ...

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Simultaneous Heliospheric Imager and Interplanetary Scintillation observations of CMEs and CIRs PowerPoint PPT Presentation

Simultaneous Heliospheric Imager and Interplanetary Scintillation observations of CMEs and CIRs - Solar System Physics Group. Simultaneous Heliospheric Imager and Interplanetary ... amplitude variations build up (Fresnel filter distance) favours observations of ...

Solar System Physics Group. Simultaneous Heliospheric Imager and Interplanetary ... amplitude variations build up (Fresnel filter distance) favours observations of ...

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A General Cone Model Approach to Heliospheric CMEs and SEP Modeling PowerPoint PPT Presentation

A General Cone Model Approach to Heliospheric CMEs and SEP Modeling - A General Cone Model Approach to Heliospheric CMEs and SEP Modeling . Magnetogram-based quiet . corona and solar wind model . The SEPs are modeled as a passive test ...

A General Cone Model Approach to Heliospheric CMEs and SEP Modeling . Magnetogram-based quiet . corona and solar wind model . The SEPs are modeled as a passive test ...

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Rapid Changes of Magnetic Fields Associated With Six X-Class Flares and Halo CMEs PowerPoint PPT Presentation

Rapid Changes of Magnetic Fields Associated With Six X-Class Flares and Halo CMEs - For all six events, leading magnetic flux had a rapid increase after flares. ... Three events showed new sunspot area, predominantly in the form of penumbra. ...

For all six events, leading magnetic flux had a rapid increase after flares. ... Three events showed new sunspot area, predominantly in the form of penumbra. ...

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Determination of the orientation of CME flux ropes for frontside full halo CMEs PowerPoint PPT Presentation

Determination of the orientation of CME flux ropes for frontside full halo CMEs - Determination of the orientation of CME flux ropes for. front-side full halo CMEs ... When = 50 degrees (see bottom row) the halo major axes correspond to ...

Determination of the orientation of CME flux ropes for. front-side full halo CMEs ... When = 50 degrees (see bottom row) the halo major axes correspond to ...

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Relationship Between Magnetic Clouds and Earth-Directed CMEs: Space Weather Research in Stanford Solar Group PowerPoint PPT Presentation

Relationship Between Magnetic Clouds and Earth-Directed CMEs: Space Weather Research in Stanford Solar Group - Here D-Bs duration, B-Bs intensity, Le-MC latitude, Fo-DSF latitude. ... Fig. 3 Multiple regressions for the duration, T, and intensity, I, ...

Here D-Bs duration, B-Bs intensity, Le-MC latitude, Fo-DSF latitude. ... Fig. 3 Multiple regressions for the duration, T, and intensity, I, ...

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The Halo CMEs Speeds and Energy of Their Related Active Regions PowerPoint PPT Presentation

The Halo CMEs Speeds and Energy of Their Related Active Regions - Studies further demonstrate correlation between the soft X-ray flux of flares ... We have examined here two measures of free energy of solar active regions; we ...

Studies further demonstrate correlation between the soft X-ray flux of flares ... We have examined here two measures of free energy of solar active regions; we ...

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3-D Pre-Eruption Magnetic Field Configuration Involved in 28 Oct 2003 Fast Halo CMEs PowerPoint PPT Presentation

3-D Pre-Eruption Magnetic Field Configuration Involved in 28 Oct 2003 Fast Halo CMEs - Low-density twisted ropes emerging within UCRs are the condition for emerging ... the plasma density in the emerging flux rope must be low ...

Low-density twisted ropes emerging within UCRs are the condition for emerging ... the plasma density in the emerging flux rope must be low ...

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Coronal and Interplanetary Magnetic Fields in October-November 2003 and November 7 2004 CMEs PowerPoint PPT Presentation

Coronal and Interplanetary Magnetic Fields in October-November 2003 and November 7 2004 CMEs - magnetic fields in order to understand the. connection between CMEs and ... it was strongly inclined to the ecliptic plane, it had negative helicity and the ...

magnetic fields in order to understand the. connection between CMEs and ... it was strongly inclined to the ecliptic plane, it had negative helicity and the ...

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Validating Onepoint Inversion Solution of the Elliptic Cone Model for FullHalo CMEs PowerPoint PPT Presentation

Validating Onepoint Inversion Solution of the Elliptic Cone Model for FullHalo CMEs - Most of halo CMEs can be reproduced by projecting the elliptic bases onto the ... Definition of five halo parameters, Dse, a, Saxh, Sayh, ?. ...

Most of halo CMEs can be reproduced by projecting the elliptic bases onto the ... Definition of five halo parameters, Dse, a, Saxh, Sayh, ?. ...

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Anemone Structure of AR NOAA 10798 and Related GeoEffective Flares and CMEs PowerPoint PPT Presentation

Anemone Structure of AR NOAA 10798 and Related GeoEffective Flares and CMEs - Focusing on the features of the sun (photosphere and corona) 8/23 24 25 26 27. Dst Index ... twisted magnetic structure lies beneath the photosphere! ...

Focusing on the features of the sun (photosphere and corona) 8/23 24 25 26 27. Dst Index ... twisted magnetic structure lies beneath the photosphere! ...

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Improvement of Inversion Solutions for Type C Halo CMEs Using the Elliptic Cone Model PowerPoint PPT Presentation

Improvement of Inversion Solutions for Type C Halo CMEs Using the Elliptic Cone Model - 2.3 Reexamination of the effect of projection on d when ?0 and 70 ... The reexamination further confirms that. d=dh-db-? ? (4.1) the inversion equations become ...

2.3 Reexamination of the effect of projection on d when ?0 and 70 ... The reexamination further confirms that. d=dh-db-? ? (4.1) the inversion equations become ...

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????? - The understandings of the generation mechanisms are important. ... CMEs MHD simulation direct comparison with observation (Shiota et al. 2005, ...

The understandings of the generation mechanisms are important. ... CMEs MHD simulation direct comparison with observation (Shiota et al. 2005, ...

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The STEREO Heliospheric Imager (HI): PowerPoint PPT Presentation

The STEREO Heliospheric Imager (HI): - The STEREO Heliospheric Imager (HI): How to detect CMEs in the Heliosphere Richard Harrison, Chris Davis & Chris Eyles

The STEREO Heliospheric Imager (HI): How to detect CMEs in the Heliosphere Richard Harrison, Chris Davis & Chris Eyles

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3-D Imaging - ... (SECCHI, John Cook; commercially available) ... Automated detection of CMEs (David Berghmans) ... (Reiser, Cook, Newmark, Crane, Yahil, Gosnell, Puetter) ...

... (SECCHI, John Cook; commercially available) ... Automated detection of CMEs (David Berghmans) ... (Reiser, Cook, Newmark, Crane, Yahil, Gosnell, Puetter) ...

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What can we learn from nonlinear forcefree extrapolations PowerPoint PPT Presentation

What can we learn from nonlinear forcefree extrapolations - What are the most suitable magnetic configurations for flares and CMEs? ... injection of helicity through photosphere, expelled in CMEs (R gnier et al. 2005) ...

What are the most suitable magnetic configurations for flares and CMEs? ... injection of helicity through photosphere, expelled in CMEs (R gnier et al. 2005) ...

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HI Operations Document PowerPoint PPT Presentation

HI Operations Document - ... archive software and data handling, inspection ... Particle acceleration at CME shocks S. Matthews The relationship between CMEs and magnetic clouds ...

... archive software and data handling, inspection ... Particle acceleration at CME shocks S. Matthews The relationship between CMEs and magnetic clouds ...

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ESCUELA SUPERIOR DE INGENIERA MECNICA Y ELCTRICA, IPN, MXICO, INSTITUTO DE GEOFSICA, UNAM, MXICO, MA PowerPoint PPT Presentation

ESCUELA SUPERIOR DE INGENIERA MECNICA Y ELCTRICA, IPN, MXICO, INSTITUTO DE GEOFSICA, UNAM, MXICO, MA - ESCUELA SUPERIOR DE INGENIER A MEC NICA Y EL CTRICA, IPN, M XICO, ... Gosling 76. AV. SPEED (km/s) A. CMES. O. CMES. FOV (SR) PERIOD. MISION. REFERENCE. 8/31/09 ...

ESCUELA SUPERIOR DE INGENIER A MEC NICA Y EL CTRICA, IPN, M XICO, ... Gosling 76. AV. SPEED (km/s) A. CMES. O. CMES. FOV (SR) PERIOD. MISION. REFERENCE. 8/31/09 ...

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ON THE RELATION BETWEEN FILAMENT ERUPTIONS, FLARES, AND CORONAL MASS EJECTIONS PowerPoint PPT Presentation

ON THE RELATION BETWEEN FILAMENT ERUPTIONS, FLARES, AND CORONAL MASS EJECTIONS - ON THE RELATION BETWEEN FILAMENT ERUPTIONS, FLARES, AND CORONAL MASS EJECTIONS ... CMEs --- LASCO C2 coronagraph images and the CME catalog to determine. ...

ON THE RELATION BETWEEN FILAMENT ERUPTIONS, FLARES, AND CORONAL MASS EJECTIONS ... CMEs --- LASCO C2 coronagraph images and the CME catalog to determine. ...

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The STEREO Mission PowerPoint PPT Presentation

The STEREO Mission - Characterize the propagation of CMEs through the heliosphere ... IMPACT: 1 min aves of B, 1 min aves solar wind moments and selected SEP fluxes ...

Characterize the propagation of CMEs through the heliosphere ... IMPACT: 1 min aves of B, 1 min aves solar wind moments and selected SEP fluxes ...

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STEREO AND SPACE WEATHER PowerPoint PPT Presentation

STEREO AND SPACE WEATHER - Characterize the propagation of CMEs through the heliosphere ... The Bastille Day' Event. Models of 3D Coronal Magnetic Topology ...

Characterize the propagation of CMEs through the heliosphere ... The Bastille Day' Event. Models of 3D Coronal Magnetic Topology ...

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Coronal IP Shocks Nat Gopalswamy NASA/GSFC PowerPoint PPT Presentation

Coronal IP Shocks Nat Gopalswamy NASA/GSFC - Easier to shock the corona in the transverse direction? (Gopalswamy, Kaiser & Pick, 2000) ... 1. CMEs accelerate low in the corona. ...

Easier to shock the corona in the transverse direction? (Gopalswamy, Kaiser & Pick, 2000) ... 1. CMEs accelerate low in the corona. ...

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Diapositive 1 PowerPoint PPT Presentation

Diapositive 1 - Halo CME May 02 1998. Disk observations. CMEs and shocks. CME wrapped by shock ... Flanks: blast wave .5. Coronal shocks and CME driven shocks. FASR Freq. range ...

Halo CME May 02 1998. Disk observations. CMEs and shocks. CME wrapped by shock ... Flanks: blast wave .5. Coronal shocks and CME driven shocks. FASR Freq. range ...

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The STEREO Mission - Characterize the propagation of CMEs through the heliosphere ... Heliospheric Imager (HI1, HI2)- Observes Coronal Mass Ejections from the Sun to ...

Characterize the propagation of CMEs through the heliosphere ... Heliospheric Imager (HI1, HI2)- Observes Coronal Mass Ejections from the Sun to ...

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How Does Free Magnetic Energy Enter the Corona? PowerPoint PPT Presentation

How Does Free Magnetic Energy Enter the Corona? - Quiescent filaments are longer- lived than AR filaments, but can also produce halo CMEs. ... ( Eruptions come days later, or occur without flux emergence. ...

Quiescent filaments are longer- lived than AR filaments, but can also produce halo CMEs. ... ( Eruptions come days later, or occur without flux emergence. ...

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3D Heliospheric Reconstructions from the SECCHI White Light Coronagraphs Onboard STEREO: Overview of the NRL Approach PowerPoint PPT Presentation

3D Heliospheric Reconstructions from the SECCHI White Light Coronagraphs Onboard STEREO: Overview of the NRL Approach - Naval Research Lab. A Yahill, T. Gosnell, R. Puetter. Pixon LLC. Goal ... CME's - models - prepare for SECCHI, effect of observing angle, velocity, ...

Naval Research Lab. A Yahill, T. Gosnell, R. Puetter. Pixon LLC. Goal ... CME's - models - prepare for SECCHI, effect of observing angle, velocity, ...

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Photospheric Flows and Solar Flares PowerPoint PPT Presentation

Photospheric Flows and Solar Flares - Why investigate correlations between photospheric magnetic field & flares/CMEs? ... of average unsigned field |BR|, (mean, variance, skew, kurtosis), denoted M(|BR ...

Why investigate correlations between photospheric magnetic field & flares/CMEs? ... of average unsigned field |BR|, (mean, variance, skew, kurtosis), denoted M(|BR ...

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Cmes PowerPoint PPT Presentations