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Reuven Ramaty PowerPoint PPT Presentation
Reuven Ramaty - Paul Scherrer Institute (Alex Zehnder) ... Late arcade development (April 21, 2002) Coronal connectivity via SEPs. Slide 16. Slide 16 ...
Paul Scherrer Institute (Alex Zehnder) ... Late arcade development (April 21, 2002) Coronal connectivity via SEPs. Slide 16. Slide 16 ...
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Apresenta PowerPoint PPT Presentation
Apresenta - Selecione o quadro... M. Ruberck La Rochefoucald Plat o Dalai Lama Bhagavad Gita Ramatis Prov rbio Hindu Arist teles Shakespeare Krishnamurti Emmet Fox Jesus A ...
Selecione o quadro... M. Ruberck La Rochefoucald Plat o Dalai Lama Bhagavad Gita Ramatis Prov rbio Hindu Arist teles Shakespeare Krishnamurti Emmet Fox Jesus A ...
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Apresenta PowerPoint PPT Presentation
Apresenta - Selecione o quadro... M. Ruberck La Rochefoucald Plat o Dalai Lama Bhagavad Gita Ramatis Prov rbio Hindu Arist teles Shakespeare Krishnamurti Emmet Fox Jesus A ...
Selecione o quadro... M. Ruberck La Rochefoucald Plat o Dalai Lama Bhagavad Gita Ramatis Prov rbio Hindu Arist teles Shakespeare Krishnamurti Emmet Fox Jesus A ...
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Apresenta PowerPoint PPT Presentation
Apresenta - Selecione o quadro... M. Ruberck La Rochefoucald Plat o Dalai Lama Bhagavad Gita Ramatis Prov rbio Hindu Arist teles Shakespeare Krishnamurti Emmet Fox Jesus A ...
Selecione o quadro... M. Ruberck La Rochefoucald Plat o Dalai Lama Bhagavad Gita Ramatis Prov rbio Hindu Arist teles Shakespeare Krishnamurti Emmet Fox Jesus A ...
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Catia Grimani PowerPoint PPT Presentation
Catia Grimani - Figure from http://cossc.gsfc.nasa.gov/images/epo/gallery/pulsars ... fraction of them lies outside their host remnants as a function of age. ...
Figure from http://cossc.gsfc.nasa.gov/images/epo/gallery/pulsars ... fraction of them lies outside their host remnants as a function of age. ...
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Origin%20of%20>%20100%20GHz%20radio%20emission PowerPoint PPT Presentation
Origin%20of%20>%20100%20GHz%20radio%20emission - Laboratoire d'Etudes Spatiale et d'Instrumentation en ... 2.7 for E Eb = 1.2 for E Eb. observed = 1.3. Peak a = 1.5. Trottet et al. 1998. RHESSI 4-8 April 06 ...
Laboratoire d'Etudes Spatiale et d'Instrumentation en ... 2.7 for E Eb = 1.2 for E Eb. observed = 1.3. Peak a = 1.5. Trottet et al. 1998. RHESSI 4-8 April 06 ...
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Prototype for an Information Market in Israel PowerPoint PPT Presentation
Prototype for an Information Market in Israel - Prototype for an Information Market in Israel. Preliminary Stage ... Boolean stocks (War and X as prime minister) Interdisciplinary Center Hertzeliya. Goals (ideas) ...
Prototype for an Information Market in Israel. Preliminary Stage ... Boolean stocks (War and X as prime minister) Interdisciplinary Center Hertzeliya. Goals (ideas) ...
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Cristina Chifor (a) PowerPoint PPT Presentation
Cristina Chifor (a) - Solar Flare X-ray Emission Cristina Chifor (a) Ken Phillips (b) , Brian Dennis (c) DAMTP, University of Cambridge, UK Mullard Space Science Lab, UK
Solar Flare X-ray Emission Cristina Chifor (a) Ken Phillips (b) , Brian Dennis (c) DAMTP, University of Cambridge, UK Mullard Space Science Lab, UK
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Solar flares, magnetars, and helioseismology PowerPoint PPT Presentation
Solar flares, magnetars, and helioseismology - HE astrophysicists tell helioseismologists where the flare ... Gallagher, P. personal communication 2004. Stanford, January 27 2005. Archive cartoon from ...
HE astrophysicists tell helioseismologists where the flare ... Gallagher, P. personal communication 2004. Stanford, January 27 2005. Archive cartoon from ...
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Radio Signatures of Coronal Magnetic Fields and Reconnections PowerPoint PPT Presentation
Radio Signatures of Coronal Magnetic Fields and Reconnections - Measurement of coronal magnetic fields - Radio diagnosis as one possibility ... Millisecond radio spikes on Nov 2, 1997 (Huang, 2004) Nobeyama Symposium, 2004 ...
Measurement of coronal magnetic fields - Radio diagnosis as one possibility ... Millisecond radio spikes on Nov 2, 1997 (Huang, 2004) Nobeyama Symposium, 2004 ...
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The Timing of Hard X Rays and Radio Waves in Solar Flares PowerPoint PPT Presentation
The Timing of Hard X Rays and Radio Waves in Solar Flares - The Timing of Hard X Rays and Radio Waves in Solar Flares ... Example: Radio Spectrogram vs. Demodulated RHESSI. HXR/Radio Correlation. Linear trend ...
The Timing of Hard X Rays and Radio Waves in Solar Flares ... Example: Radio Spectrogram vs. Demodulated RHESSI. HXR/Radio Correlation. Linear trend ...
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Regularized%20Mean%20and%20Accelerated%20Electron%20Flux%20Spectra%20in%20Solar%20Flares PowerPoint PPT Presentation
Regularized%20Mean%20and%20Accelerated%20Electron%20Flux%20Spectra%20in%20Solar%20Flares - Michele Piana, Anna Maria Massone (INFM, UdR di Genova), A. Gordon Emslie (The ... To find an electron spectrum is to solve a least square problem: ...
Michele Piana, Anna Maria Massone (INFM, UdR di Genova), A. Gordon Emslie (The ... To find an electron spectrum is to solve a least square problem: ...
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FASR Presentation PowerPoint PPT Presentation
FASR Presentation - photon spectrum ( ) [ph s-1 cm-2 keV-1] observed at Earth... low-energy cutoff problem may be ... energies may now be. computed without ECO! (Emslie, 2003) ...
photon spectrum ( ) [ph s-1 cm-2 keV-1] observed at Earth... low-energy cutoff problem may be ... energies may now be. computed without ECO! (Emslie, 2003) ...
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More phenomena difficult to observe PowerPoint PPT Presentation
More phenomena difficult to observe - really, this is what is injected into the source by colliding p's, 's =2, Tmax = 3 GeV/nucl ... of X-ray flux with angle is the Laplace transform of the neutron ...
really, this is what is injected into the source by colliding p's, 's =2, Tmax = 3 GeV/nucl ... of X-ray flux with angle is the Laplace transform of the neutron ...
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Compositional Characteristics of SEP Events PowerPoint PPT Presentation
Compositional Characteristics of SEP Events - Consistent with Bastille Day QFe from SEPICA and SAMPEX. Compare with QFe from other events: 1992 event remarkably similar to Bastille Day event. ...
Consistent with Bastille Day QFe from SEPICA and SAMPEX. Compare with QFe from other events: 1992 event remarkably similar to Bastille Day event. ...
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First Results of Joint OVSA and HESSI Observations PowerPoint PPT Presentation
First Results of Joint OVSA and HESSI Observations - ... in several acceleration episodes, apparently independently of the ... In first acceleration episode, 25 keV X-rays progressively harden (from d ~ 7.5-4.7) ...
... in several acceleration episodes, apparently independently of the ... In first acceleration episode, 25 keV X-rays progressively harden (from d ~ 7.5-4.7) ...
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Far infrared emission of solar flares PowerPoint PPT Presentation
Far infrared emission of solar flares - How are charged particles accelerated to relativistic energies ? ... EGRET (NASA) Solar and Heliospheric Observatory / EIT (ESA/NASA) log(frequency [Hz] ...
How are charged particles accelerated to relativistic energies ? ... EGRET (NASA) Solar and Heliospheric Observatory / EIT (ESA/NASA) log(frequency [Hz] ...
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William Thompson PowerPoint PPT Presentation
William Thompson - SolarSoft is a collection of software used for a wide ... NRH: Nan ay Radio Heliograph. NRO: Nobeyama Radio Observatory. Radioheliograph. Radio Polarimeters ...
SolarSoft is a collection of software used for a wide ... NRH: Nan ay Radio Heliograph. NRO: Nobeyama Radio Observatory. Radioheliograph. Radio Polarimeters ...
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LASP Summer Internship 2004 PowerPoint PPT Presentation
LASP Summer Internship 2004 - Mentors: Dr. Ken Phillips & Dr. Brian Dennis ... Electron kinetic energy higher than average thermal energy of ... Pint Of Ale. MORE COMPLICATIONS: INSTRUMENTAL ...
Mentors: Dr. Ken Phillips & Dr. Brian Dennis ... Electron kinetic energy higher than average thermal energy of ... Pint Of Ale. MORE COMPLICATIONS: INSTRUMENTAL ...
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EL OBSERVATORIO SOLAR MEXICANO DE GRAN ALTURA (OSOMEGA): PowerPoint PPT Presentation
EL OBSERVATORIO SOLAR MEXICANO DE GRAN ALTURA (OSOMEGA): - Bernhard Lyot coloc aqu su nuevo coronografo en los 1930s y vi por primera ... La direcci n se resuelve con las g ndolas inferiores. Hay 4 g ndolas: 2 resuelven N-S ...
Bernhard Lyot coloc aqu su nuevo coronografo en los 1930s y vi por primera ... La direcci n se resuelve con las g ndolas inferiores. Hay 4 g ndolas: 2 resuelven N-S ...
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Dcapage laser associ au procd Cold Spray PowerPoint PPT Presentation
Dcapage laser associ au procd Cold Spray - Transfert de technologie : Accompagnement des entreprises dans leur d marche ... Contr le alignement faisceau. Cession Licences : PROTAL. BC CLAD. HISTOIRES A SUCCES ...
Transfert de technologie : Accompagnement des entreprises dans leur d marche ... Contr le alignement faisceau. Cession Licences : PROTAL. BC CLAD. HISTOIRES A SUCCES ...
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MSU PowerPoint PPT Presentation
MSU - MSU The Group Webpage: solar.physics.montana.edu Solar Physics Group MSU Solar Physics is TRACE RHESSI and Max Millennium SSEL s MOSES Transition Region And ...
MSU The Group Webpage: solar.physics.montana.edu Solar Physics Group MSU Solar Physics is TRACE RHESSI and Max Millennium SSEL s MOSES Transition Region And ...
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2nd RHESSI/NESSI PowerPoint PPT Presentation
2nd RHESSI/NESSI - Title: PowerPoint Presentation Last modified by: Luqin Created Date: 1/1/1601 12:00:00 AM Document presentation format: Other titles
Title: PowerPoint Presentation Last modified by: Luqin Created Date: 1/1/1601 12:00:00 AM Document presentation format: Other titles
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The all-sky distribution of 511 keV electron-positron annihilation emission PowerPoint PPT Presentation
The all-sky distribution of 511 keV electron-positron annihilation emission - The bulge emission is spherically symmetric and is centred on the galactic ... The bulge emission arises from a different source which has only a weak or no ...
The bulge emission is spherically symmetric and is centred on the galactic ... The bulge emission arises from a different source which has only a weak or no ...
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Sesi PowerPoint PPT Presentation
Sesi - Title: Presentaci n de PowerPoint Author: Adri n Eduardo Sampietro Last modified by: OEM Created Date: 7/6/2005 6:49:06 PM Document presentation format
Title: Presentaci n de PowerPoint Author: Adri n Eduardo Sampietro Last modified by: OEM Created Date: 7/6/2005 6:49:06 PM Document presentation format
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High Energy Astronomy PowerPoint PPT Presentation
High Energy Astronomy - The Sun Makes History ... If it wasn't for the Sun, the Norse would probably have colonised America 500 ... energy processes in the Sun are best studied using ...
The Sun Makes History ... If it wasn't for the Sun, the Norse would probably have colonised America 500 ... energy processes in the Sun are best studied using ...
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Overview of Space Sciences Laboratory PowerPoint PPT Presentation
Overview of Space Sciences Laboratory - Automated ground/space communication. Space physics: upper-atmosphere, solar, ... Connecting campus research to space efforts. Facility opened in 1966 ...
Automated ground/space communication. Space physics: upper-atmosphere, solar, ... Connecting campus research to space efforts. Facility opened in 1966 ...
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Institute of Astronomy, PowerPoint PPT Presentation
Institute of Astronomy, - GOES class M1.0. 6 12 keV. 12 25 keV. 25 50 keV. 50 100 keV ... Particle gains energy in qvE, but loses in antiparallel interactions ...
GOES class M1.0. 6 12 keV. 12 25 keV. 25 50 keV. 50 100 keV ... Particle gains energy in qvE, but loses in antiparallel interactions ...
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Delayed X and GammaRay Line Emission from Solar Flare Radioactivity PowerPoint PPT Presentation
Delayed X and GammaRay Line Emission from Solar Flare Radioactivity - Delayed X- and Gamma-Ray Line Emission. from Solar Flare Radioactivity ... The Gamma-Ray Imager ... an artist's Cosmic Vision. From J. Kn dlseder, ESLAB Symposium 2005 ...
Delayed X- and Gamma-Ray Line Emission. from Solar Flare Radioactivity ... The Gamma-Ray Imager ... an artist's Cosmic Vision. From J. Kn dlseder, ESLAB Symposium 2005 ...
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Solar flare observations with INTEGRALSPI PowerPoint PPT Presentation
Solar flare observations with INTEGRALSPI - Photosphere. No PAS. Strong PAS. The magnetic loop model. IEEC, Barcelona, September 23, 2004 ... PHOTOSPHERE. CORONA. isotropic accelerated- particle release ...
Photosphere. No PAS. Strong PAS. The magnetic loop model. IEEC, Barcelona, September 23, 2004 ... PHOTOSPHERE. CORONA. isotropic accelerated- particle release ...
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Studies on the 2002 July 23 Flare with RHESSI PowerPoint PPT Presentation
Studies on the 2002 July 23 Flare with RHESSI - Electron Bremsstrahlung Hard X-ray Spectra, Electron Distributions and ... Radio and hard X-ray images of high-energy electrons in a compact X-class solar ...
Electron Bremsstrahlung Hard X-ray Spectra, Electron Distributions and ... Radio and hard X-ray images of high-energy electrons in a compact X-class solar ...
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Present and Future Research Directions and Space Missions for the Space Sciences Laboratory at Univ. of California, Berkeley PowerPoint PPT Presentation
Present and Future Research Directions and Space Missions for the Space Sciences Laboratory at Univ. of California, Berkeley - Present and Future Research Directions and Space Missions for ... Spectrogram plot: time-energy, colors represent counts. RHESSI and GOES. GOES in LINEAR scale! ...
Present and Future Research Directions and Space Missions for ... Spectrogram plot: time-energy, colors represent counts. RHESSI and GOES. GOES in LINEAR scale! ...
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Observational Evidence for Chromospheric Evaporation PowerPoint PPT Presentation
Observational Evidence for Chromospheric Evaporation - ... in Science and Technology (CAST) studentship from Queen's University Belfast and ... of the American Astornomical Society for being awarded an SPD Studentship. ...
... in Science and Technology (CAST) studentship from Queen's University Belfast and ... of the American Astornomical Society for being awarded an SPD Studentship. ...
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Center to Limb Variation of Hard X-Ray Spectra from RHESSI J.McTiernan (SSL/UCB) PowerPoint PPT Presentation
Center to Limb Variation of Hard X-Ray Spectra from RHESSI J.McTiernan (SSL/UCB) - If Coulomb collisions are the dominant scattering mechanism for accelerated ... instruments have never found any noticeable anisotropy in solar flare X-rays. ...
If Coulomb collisions are the dominant scattering mechanism for accelerated ... instruments have never found any noticeable anisotropy in solar flare X-rays. ...
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Mostly Electron Acceleration and Hard Xrays PowerPoint PPT Presentation
Mostly Electron Acceleration and Hard Xrays - Renounce simple dipole models (Zirin, Doschek, Trottet) ... ALL acceleration is by electric fields (Coulomb, Newton) ... Amp re, Faraday constraints ...
Renounce simple dipole models (Zirin, Doschek, Trottet) ... ALL acceleration is by electric fields (Coulomb, Newton) ... Amp re, Faraday constraints ...
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Working Group 3: Radio correlations PowerPoint PPT Presentation
Working Group 3: Radio correlations - Working Group 3: Radio correlations
Working Group 3: Radio correlations
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Energetic Particles in the Solar Atmosphere PowerPoint PPT Presentation
Energetic Particles in the Solar Atmosphere - Flares - relativistic electrons, ion beams, neutrons, pions ... respect to photospheric intersection of coronal magnetic separatrix surfaces (also, Demoulin, ...
Flares - relativistic electrons, ion beams, neutrons, pions ... respect to photospheric intersection of coronal magnetic separatrix surfaces (also, Demoulin, ...
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PowerPoint Presentation Magnetic Reconnection and Mass Acceleration in Solar Flares and Coronal Mass PowerPoint PPT Presentation
PowerPoint Presentation Magnetic Reconnection and Mass Acceleration in Solar Flares and Coronal Mass - Lee et al. 1998 (Y. Liu) (TRACE) a large flare observed in different wavelengths (Qiu et al. ... (Forbes-Priest-Lin) CME front. filament. flare. breakout model ...
Lee et al. 1998 (Y. Liu) (TRACE) a large flare observed in different wavelengths (Qiu et al. ... (Forbes-Priest-Lin) CME front. filament. flare. breakout model ...
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Relations between concurrent hard Xray sources in solar flares M' Battaglia and A' O' Benz PowerPoint PPT Presentation
Relations between concurrent hard Xray sources in solar flares M' Battaglia and A' O' Benz - ?? 2 may be explained by an intermediate situation between the two extremes. ... seems to be at work, differing in one flare for the two legs of the loop. ...
?? 2 may be explained by an intermediate situation between the two extremes. ... seems to be at work, differing in one flare for the two legs of the loop. ...
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Solar flare observations with INTEGRALSPI PowerPoint PPT Presentation
Solar flare observations with INTEGRALSPI - Solar flare observations with INTEGRAL/SPI. IEEC, Barcelona, September 23, 2004 (M. Gros, J. Kiener, V. Tatischeff et al.) TRACE & RHESSI, 28-Oct ... IBIS. SPI ...
Solar flare observations with INTEGRAL/SPI. IEEC, Barcelona, September 23, 2004 (M. Gros, J. Kiener, V. Tatischeff et al.) TRACE & RHESSI, 28-Oct ... IBIS. SPI ...
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Missions PowerPoint PPT Presentation
Missions - Senior Review. The Living With a Star (LWS) Sentinels Mission. R. P. Lin ... Cruise: 2 yr 3-11 months to final configuration, Science starts 60 days after launch ...
Senior Review. The Living With a Star (LWS) Sentinels Mission. R. P. Lin ... Cruise: 2 yr 3-11 months to final configuration, Science starts 60 days after launch ...
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Magnetic Reconnection and Particle PowerPoint PPT Presentation
Magnetic Reconnection and Particle - To provide an overview of current ideas about the role of, and ... (2) Supra-Arcade Downflows in LDEs. Observational Support for Reconnection: ...
To provide an overview of current ideas about the role of, and ... (2) Supra-Arcade Downflows in LDEs. Observational Support for Reconnection: ...
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Electron Acceleration and Transport in Microwave Flaring Loops PowerPoint PPT Presentation
Electron Acceleration and Transport in Microwave Flaring Loops - Lee et al 2000, - dynamics of spectral properties, electron anisotropy ... Fleishman & Melnikov 2003, - influence of electron pitch angle anisotropy ...
Lee et al 2000, - dynamics of spectral properties, electron anisotropy ... Fleishman & Melnikov 2003, - influence of electron pitch angle anisotropy ...
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The synthesis of 26Al and 60Fe in massive stars and their current abundances in our Galaxy PowerPoint PPT Presentation
The synthesis of 26Al and 60Fe in massive stars and their current abundances in our Galaxy - Istituto Nazionale di AstroFisica (Istituto di Astrofisica Spaziale e Fisica Cosmica) ... though the ground and the metastable 26Al states are properly taken into ...
Istituto Nazionale di AstroFisica (Istituto di Astrofisica Spaziale e Fisica Cosmica) ... though the ground and the metastable 26Al states are properly taken into ...
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Microwave and hard X-ray imaging observations of energetic electrons in solar flares: event of 2003 June 17 PowerPoint PPT Presentation
Microwave and hard X-ray imaging observations of energetic electrons in solar flares: event of 2003 June 17 - Microwave and hard X-ray imaging observations of energetic electrons in solar ... Hard X-ray emission, on the other hand, is produced by bremsstrahlung from ...
Microwave and hard X-ray imaging observations of energetic electrons in solar ... Hard X-ray emission, on the other hand, is produced by bremsstrahlung from ...
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The LowEnergy Cutoff to the Nonthermal Electron Spectrum Determined From RHESSI Observations PowerPoint PPT Presentation
The LowEnergy Cutoff to the Nonthermal Electron Spectrum Determined From RHESSI Observations - Flat cutoff. Expected Photon Spectrum. Flattening. Ecutoff = 25 keV ... Flat Cutoff Energy: 51 keV. Albedo Correction. No Albedo correction ...
Flat cutoff. Expected Photon Spectrum. Flattening. Ecutoff = 25 keV ... Flat Cutoff Energy: 51 keV. Albedo Correction. No Albedo correction ...
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Sesi PowerPoint PPT Presentation
Sesi - MARIO ... The Nines of Reliability/Availability. 0.01. 0.1. 1. Cost ($/kWh) ... The Nines of Reliability/Availability. E-Business.com. 100000. 10000 ...
MARIO ... The Nines of Reliability/Availability. 0.01. 0.1. 1. Cost ($/kWh) ... The Nines of Reliability/Availability. E-Business.com. 100000. 10000 ...
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Tijana Prodanovic PowerPoint PPT Presentation
Tijana Prodanovic - But no strong evidence for pion 'bump' ... so that 'pion bump' stays below observed Galactic ... 'Pion bump' not observed in extragalactic gamma-ray background ...
But no strong evidence for pion 'bump' ... so that 'pion bump' stays below observed Galactic ... 'Pion bump' not observed in extragalactic gamma-ray background ...
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Gandolfa PowerPoint PPT Presentation
Gandolfa - Luzzatto-Pompas Il significato dei colori In quelle tarde nottate invernali e primaverili riflettendo sui miei tanti lustri, ...
Luzzatto-Pompas Il significato dei colori In quelle tarde nottate invernali e primaverili riflettendo sui miei tanti lustri, ...
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The Role of Nuclei-Nuclei Interactions in the Production of Gamma-Ray Lines in Some Solar Flares PowerPoint PPT Presentation
The Role of Nuclei-Nuclei Interactions in the Production of Gamma-Ray Lines in Some Solar Flares - With a high probability, the gamma-ray line emission of 28Si from this flare was ... investigation of different aspects of solar gamma rays remains very significant. ...
With a high probability, the gamma-ray line emission of 28Si from this flare was ... investigation of different aspects of solar gamma rays remains very significant. ...
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Initiation and Acceleration of a Flareassociated Coronal Mass Ejection PowerPoint PPT Presentation
Initiation and Acceleration of a Flareassociated Coronal Mass Ejection - While expanding, the appearance of the feature remains remarkably constant as it ... field-of-view, which moves away from the surface with an exponential ...
While expanding, the appearance of the feature remains remarkably constant as it ... field-of-view, which moves away from the surface with an exponential ...
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Diapositiva 1 PowerPoint PPT Presentation
Diapositiva 1 - sudden release of energy stored in the magnetic field (up to ... and chromosphere. large flares occur only at. solar maximum. heat plasma and accelerate ...
sudden release of energy stored in the magnetic field (up to ... and chromosphere. large flares occur only at. solar maximum. heat plasma and accelerate ...
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Current and Future Solar Observing Missions PowerPoint PPT Presentation
Current and Future Solar Observing Missions - Current and Future Solar Observing Missions
Current and Future Solar Observing Missions
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Nonthermal Spectral Flattening in Early Impulsive Flares PowerPoint PPT Presentation
Nonthermal Spectral Flattening in Early Impulsive Flares - Criteria for early impulsive flares: (1) the 25-50 keV flux increases significantly in the flares; ... of the 34 selected flares were found to show spectral ...
Criteria for early impulsive flares: (1) the 25-50 keV flux increases significantly in the flares; ... of the 34 selected flares were found to show spectral ...
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