279 Rhessi PPTs View free & download

RHESSI Visibilities PowerPoint PPT Presentation

RHESSI Visibilities - The measured visibility is a complex ... Provide a compact representation of input imaging data Can provide starting point for imaging algorithms Useful for ...

The measured visibility is a complex ... Provide a compact representation of input imaging data Can provide starting point for imaging algorithms Useful for ...

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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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RHESSI Microflares PowerPoint PPT Presentation

RHESSI Microflares - RHESSI Microflares. Steven Christe1,2, S m Krucker2, Iain Hannah3, R. P. Lin1,2 ... Iain Hannah3, R. P. Lin1,2. 1Physics Department, University of California at ...

RHESSI Microflares. Steven Christe1,2, S m Krucker2, Iain Hannah3, R. P. Lin1,2 ... Iain Hannah3, R. P. Lin1,2. 1Physics Department, University of California at ...

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RHESSI Visibilities - Measured spatial frequency (arcsec-1): Magnitude determined by the angular pitch of the grid. ... spatial frequencies) Properties of visibilities (2) ...

Measured spatial frequency (arcsec-1): Magnitude determined by the angular pitch of the grid. ... spatial frequencies) Properties of visibilities (2) ...

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Measuring the Temperature of Hot Solar Flare Plasma with RHESSI PowerPoint PPT Presentation

Measuring the Temperature of Hot Solar Flare Plasma with RHESSI - Measuring the Temperature of Hot Solar Flare Plasma with RHESSI Amir Caspi1,2, Sam Krucker2, Robert P. Lin1,2 1 Department of Physics, University of California ...

Measuring the Temperature of Hot Solar Flare Plasma with RHESSI Amir Caspi1,2, Sam Krucker2, Robert P. Lin1,2 1 Department of Physics, University of California ...

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RHESSI Microflare Statistics PowerPoint PPT Presentation

RHESSI Microflare Statistics - Therm model. Non-therm model. Total Model. RHESSI/Meudon July ... Therm model. Non-therm model. Total Model. RHESSI/Meudon July 2004. 7. Thermal Time Profiles ...

Therm model. Non-therm model. Total Model. RHESSI/Meudon July ... Therm model. Non-therm model. Total Model. RHESSI/Meudon July 2004. 7. Thermal Time Profiles ...

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Coronal hard X-rays prior to RHESSI PowerPoint PPT Presentation

Coronal hard X-rays prior to RHESSI - The 'extended flare' (Frost & Dennis, OSO-7, Kiplinger, Cliver et al. ... Kiplinger, ApJ 453, 973 (1995) Squares = solar proton events ...

The 'extended flare' (Frost & Dennis, OSO-7, Kiplinger, Cliver et al. ... Kiplinger, ApJ 453, 973 (1995) Squares = solar proton events ...

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RHESSI Observations of Super-Hot (T > 30 MK) Plasma in Large Solar Flares PowerPoint PPT Presentation

RHESSI Observations of Super-Hot (T > 30 MK) Plasma in Large Solar Flares - RHESSI Observations of Super-Hot (T 30 MK) Plasma in Large Solar Flares Amir Caspi1 & Robert P. Lin1 1 Department of Physics & Space Sciences Laboratory,

RHESSI Observations of Super-Hot (T 30 MK) Plasma in Large Solar Flares Amir Caspi1 & Robert P. Lin1 1 Department of Physics & Space Sciences Laboratory,

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Combined WIND-RHESSI-TRACE studies PowerPoint PPT Presentation

Combined WIND-RHESSI-TRACE studies - Space Sciences Lab, UC Berkeley. The origin of solar impulsive energetic electrons: ... Electrons lose their. energy by collisions. X-ray emission. heating ...

Space Sciences Lab, UC Berkeley. The origin of solar impulsive energetic electrons: ... Electrons lose their. energy by collisions. X-ray emission. heating ...

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Energy-height relation for hard X-ray footpoint sources observed by RHESSI. PowerPoint PPT Presentation

Energy-height relation for hard X-ray footpoint sources observed by RHESSI. - Time evolution is represented by the brightness. The first interval is the. darkest one. ... Comparision between several models of density (Aschwanden et al. 2002) and ...

Time evolution is represented by the brightness. The first interval is the. darkest one. ... Comparision between several models of density (Aschwanden et al. 2002) and ...

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RHESSI and Radio Imaging Observations of Microflares PowerPoint PPT Presentation

RHESSI and Radio Imaging Observations of Microflares - Dept. of Astronomy, University of Maryland, College Park, MD and Lab for ... Time profiles of 17GHz and X-Ray time profile and spectrogram. 2002 May 03 ...

Dept. of Astronomy, University of Maryland, College Park, MD and Lab for ... Time profiles of 17GHz and X-Ray time profile and spectrogram. 2002 May 03 ...

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NoRH Observations of RHESSI Microflares PowerPoint PPT Presentation

NoRH Observations of RHESSI Microflares - NoRH Observations of RHESSI Microflares. M.R. Kundu, ... Dept. of Astronomy, University of Maryland, College Park, MD and Lab for ... RHESSI spectrogram. May 02 ...

NoRH Observations of RHESSI Microflares. M.R. Kundu, ... Dept. of Astronomy, University of Maryland, College Park, MD and Lab for ... RHESSI spectrogram. May 02 ...

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Characterizing Thermal and Non-Thermal Electron Populations in Solar Flares Using RHESSI PowerPoint PPT Presentation

Characterizing Thermal and Non-Thermal Electron Populations in Solar Flares Using RHESSI - 2 Space Sciences Laboratory, University of California, Berkeley, CA 94720. July 27, 2004 ... Obtain spectra based on source location ...

2 Space Sciences Laboratory, University of California, Berkeley, CA 94720. July 27, 2004 ... Obtain spectra based on source location ...

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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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Observing the Sun from space: Highlights from Yohkoh, SOHO, TRACE, RHESSI PowerPoint PPT Presentation

Observing the Sun from space: Highlights from Yohkoh, SOHO, TRACE, RHESSI - Title: PowerPoint Presentation - The Solar Atmosphere Structure and Activity Part I Author: jlc Last modified by: Hugh Hudson Created Date: 8/11/2004 7:26:30 PM

Title: PowerPoint Presentation - The Solar Atmosphere Structure and Activity Part I Author: jlc Last modified by: Hugh Hudson Created Date: 8/11/2004 7:26:30 PM

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Is the Standard Flare Model Still Adequate? -- A Review of Recent RHESSI X-Ray Observations PowerPoint PPT Presentation

Is the Standard Flare Model Still Adequate? -- A Review of Recent RHESSI X-Ray Observations - Relaxation of Sheared Magnetic fields. a Process of Contraction. Events List. The M1.2 flare of 2002-04-15 (Sui and Holman 2003) ...

Relaxation of Sheared Magnetic fields. a Process of Contraction. Events List. The M1.2 flare of 2002-04-15 (Sui and Holman 2003) ...

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Magnetic Reconnection Rate and RHESSI Hard XRay Imaging Spectroscopy of Well Resolved Xclass Flares - Magnetic Reconnection Rate and RHESSI Hard XRay Imaging Spectroscopy of Well Resolved Xclass Flares

Magnetic Reconnection Rate and RHESSI Hard XRay Imaging Spectroscopy of Well Resolved Xclass Flares

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Active region Xray jets observed with Hinode and RHESSI - Active region Xray jets observed with Hinode and RHESSI

Active region Xray jets observed with Hinode and RHESSI

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Hard XRay Solar Flare Polarimetry with RHESSI PowerPoint PPT Presentation

Hard XRay Solar Flare Polarimetry with RHESSI - A broader beam (covering the full front surface of the telescope tube) has been ... Bottom row shows results for wide incident beam (with spacecraft scattering) ...

A broader beam (covering the full front surface of the telescope tube) has been ... Bottom row shows results for wide incident beam (with spacecraft scattering) ...

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Time delay between hard X-ray and gamma ray lines observed by RHESSI during the 23 July event PowerPoint PPT Presentation

Time delay between hard X-ray and gamma ray lines observed by RHESSI during the 23 July event - X/ X/ X/ corona. Particle injection ... We use these injections to compute the X-ray at 1MeV and gamma ray flux time evolution ...

X/ X/ X/ corona. Particle injection ... We use these injections to compute the X-ray at 1MeV and gamma ray flux time evolution ...

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Evidence for Magnetic Reconnection in Flares Observed With RHESSI PowerPoint PPT Presentation

Evidence for Magnetic Reconnection in Flares Observed With RHESSI - Overview of the classical flare models. RHESSI observations of four flares ... Thank SPD for providing travel support via the studentship award. Looptop Centroid ...

Overview of the classical flare models. RHESSI observations of four flares ... Thank SPD for providing travel support via the studentship award. Looptop Centroid ...

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The relative timing of RHESSI and radio Phoenix2 fine structures PowerPoint PPT Presentation

The relative timing of RHESSI and radio Phoenix2 fine structures - The relative timing of RHESSI and radio (Phoenix-2) fine structures ... Error bars: perturb solution until log L drops by unity. A problem case. Attenuator in ...

The relative timing of RHESSI and radio (Phoenix-2) fine structures ... Error bars: perturb solution until log L drops by unity. A problem case. Attenuator in ...

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Optimizing RHESSI XRay Imaging for Compact Sources PowerPoint PPT Presentation

Optimizing RHESSI XRay Imaging for Compact Sources - Optimizing RHESSI X-Ray Imaging for Compact Sources ... RHESSI X-ray imaging is possible with angular resolution as fine as 2 arcsec ...

Optimizing RHESSI X-Ray Imaging for Compact Sources ... RHESSI X-ray imaging is possible with angular resolution as fine as 2 arcsec ...

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RHESSI Xray Spectral Analysis PowerPoint PPT Presentation

RHESSI Xray Spectral Analysis - ... that result in lower than expected pulse amplitudes, electronic effects at high count rates such as pulse pile-up and change in gain, detector-to-detector ...

... that result in lower than expected pulse amplitudes, electronic effects at high count rates such as pulse pile-up and change in gain, detector-to-detector ...

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RHESSI and SOHOCDS Observations of Chromospheric Evaporation in Solar Flares PowerPoint PPT Presentation

RHESSI and SOHOCDS Observations of Chromospheric Evaporation in Solar Flares - Electrons are accelerated during impulsive phase of solar flare ... Chromosphere unable to radiate energy deposited by non-thermal electrons. Velocities 400 km/s ...

Electrons are accelerated during impulsive phase of solar flare ... Chromosphere unable to radiate energy deposited by non-thermal electrons. Velocities 400 km/s ...

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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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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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Pre-flare%20Energy%20Storage PowerPoint PPT Presentation

Pre-flare%20Energy%20Storage - burst. Stored globally. Dec. 10, 2004. RHESSI/SOHO/TRACE. Steady ... burst: latency. Rapidly released. via local E field. Dec. 10, 2004. RHESSI/SOHO/TRACE ...

burst. Stored globally. Dec. 10, 2004. RHESSI/SOHO/TRACE. Steady ... burst: latency. Rapidly released. via local E field. Dec. 10, 2004. RHESSI/SOHO/TRACE ...

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Diapositive%201 PowerPoint PPT Presentation

Diapositive%201 - Flux du bruit de fond. Fit reproduisant le mieux le flux total le ... raie du bruit de fond. Analyse spectrale de RHESSI Indice spectral des photons = -1.6 ...

Flux du bruit de fond. Fit reproduisant le mieux le flux total le ... raie du bruit de fond. Analyse spectrale de RHESSI Indice spectral des photons = -1.6 ...

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OSPEX - OSPEX Object Spectral Executive. OSPEX new, but completely separate, object ... RHESSI Spectrum FITS File. Use spectrum object through GUI or CLI ...

OSPEX Object Spectral Executive. OSPEX new, but completely separate, object ... RHESSI Spectrum FITS File. Use spectrum object through GUI or CLI ...

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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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X-ray imaging PowerPoint PPT Presentation

X-ray imaging - RHESSI X-ray imaging during HXR peak: X-ray imaging. Two ribbon flare with HXR footpoints (contours) with thermal loop (image) movie ...

RHESSI X-ray imaging during HXR peak: X-ray imaging. Two ribbon flare with HXR footpoints (contours) with thermal loop (image) movie ...

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Pre-eruption energy release: PowerPoint PPT Presentation

Pre-eruption energy release: - Pre-eruption energy release: Tether or not? Farnik et al. 2003. Tether-cutting? ... RHESSI July 23, 2002 data give an entirely different picture (see ApJL ...

Pre-eruption energy release: Tether or not? Farnik et al. 2003. Tether-cutting? ... RHESSI July 23, 2002 data give an entirely different picture (see ApJL ...

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Flare Flux vs. Magnetic Flux PowerPoint PPT Presentation

Flare Flux vs. Magnetic Flux - Fisher et al. (1998) found that active region (AR) non-flare soft X-ray luminosity is LSXR 1.19. ... RHESSI can do MUCH BETTER than my sophomoric approach! ...

Fisher et al. (1998) found that active region (AR) non-flare soft X-ray luminosity is LSXR 1.19. ... RHESSI can do MUCH BETTER than my sophomoric approach! ...

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Thermal and nonthermal contributions to the solar flare X-ray flux PowerPoint PPT Presentation

Thermal and nonthermal contributions to the solar flare X-ray flux - Thermal and nonthermal contributions to the solar flare X-ray flux ... Thin Shutters In (A1) Detector #4. 1-minute accumulations. RHESSI Count-rate Spectrum ...

Thermal and nonthermal contributions to the solar flare X-ray flux ... Thin Shutters In (A1) Detector #4. 1-minute accumulations. RHESSI Count-rate Spectrum ...

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Diagnostics of Non-thermal Electron Distribution using synthetic and flare spectra PowerPoint PPT Presentation

Diagnostics of Non-thermal Electron Distribution using synthetic and flare spectra - Diagnostics of Non-thermal Electron Distribution using synthetic ... RHESSI contours in two energy bands : 6 12 keV. and. 25 50 ... HEM acknowledges the ...

Diagnostics of Non-thermal Electron Distribution using synthetic ... RHESSI contours in two energy bands : 6 12 keV. and. 25 50 ... HEM acknowledges the ...

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Flare Thermal Energy PowerPoint PPT Presentation

Flare Thermal Energy - ... obtain temperature (T in degrees K) and emission measure (EM) ... Tmin = TGOES 1.4 keV (16 MK) EM (Tmin to Tmax) 2 1049 cm-3. RHESSI Area (A) 9 103 arcsec2 ...

... obtain temperature (T in degrees K) and emission measure (EM) ... Tmin = TGOES 1.4 keV (16 MK) EM (Tmin to Tmax) 2 1049 cm-3. RHESSI Area (A) 9 103 arcsec2 ...

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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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Dynamic General Vegetation Models and Climate Change: Current State and Future Potential PowerPoint PPT Presentation

Dynamic General Vegetation Models and Climate Change: Current State and Future Potential - Ron Neilson. Leader, MAPSS Team. Pacific Northwest Research Station. USDA ... H.J. Andrews at 800 m resolution. Regional Hydro-Ecological System (RHESSys) ...

Ron Neilson. Leader, MAPSS Team. Pacific Northwest Research Station. USDA ... H.J. Andrews at 800 m resolution. Regional Hydro-Ecological System (RHESSys) ...

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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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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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Households as ecological agents: PowerPoint PPT Presentation

Households as ecological agents: - Digital elevation model. Parcel data (Maryland Property View) High resolution aerial photography. Input to RHESSys: Regional Hydro-Ecologic Simulation System ...

Digital elevation model. Parcel data (Maryland Property View) High resolution aerial photography. Input to RHESSys: Regional Hydro-Ecologic Simulation System ...

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Visualization of Hydrologic and Ecologic Processes over Spatially Variable Terrain PowerPoint PPT Presentation

Visualization of Hydrologic and Ecologic Processes over Spatially Variable Terrain - ... through time (under different climate conditions, and ... RHESSys Ecological Process Modeling. Time Series Output. Spatial Output (Using GRASS GIS Software) ...

... through time (under different climate conditions, and ... RHESSys Ecological Process Modeling. Time Series Output. Spatial Output (Using GRASS GIS Software) ...

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Search for Xray emission from coronal electron beams associated with type III radio bursts PowerPoint PPT Presentation

Search for Xray emission from coronal electron beams associated with type III radio bursts - 12 beyond /-60 degrees. 2 have no RHESSI flare associated ... XR ? XR? Type III. Observed photon spectrum. e. I(e) Non-thermal emission: Partial thick-target ...

12 beyond /-60 degrees. 2 have no RHESSI flare associated ... XR ? XR? Type III. Observed photon spectrum. e. I(e) Non-thermal emission: Partial thick-target ...

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Notes from the Heliophysics MO PowerPoint PPT Presentation

Notes from the Heliophysics MO - Alex Pevtsov Hinode, RHESSI, SOHO, TRACE. Arik Posner SOHO, Ulysses, Wind ... to study Heliophysics science, as demonstrated by the 2003 Halloween Storms. ...

Alex Pevtsov Hinode, RHESSI, SOHO, TRACE. Arik Posner SOHO, Ulysses, Wind ... to study Heliophysics science, as demonstrated by the 2003 Halloween Storms. ...

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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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Preflare phenomena in HXR, SXR PowerPoint PPT Presentation

Preflare phenomena in HXR, SXR - ... ... aaa GGGpppSSSsss tttFFFTTTOOOdddfff eee ...

... ... aaa GGGpppSSSsss tttFFFTTTOOOdddfff eee ...

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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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Radio and Hard X-Ray Imaging Observations of the M 5.7 Flare of 2002 March 14 PowerPoint PPT Presentation

Radio and Hard X-Ray Imaging Observations of the M 5.7 Flare of 2002 March 14 - Radio and Hard X-Ray Imaging Observations of the M 5.7 Flare of. 2002 March 14 ... This model isused to address the thermal/nonthermal and radio/HXR number problems. ...

Radio and Hard X-Ray Imaging Observations of the M 5.7 Flare of. 2002 March 14 ... This model isused to address the thermal/nonthermal and radio/HXR number problems. ...

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Diagnostics of flare activity level from turbulence parameters of photospheric plasma PowerPoint PPT Presentation

Diagnostics of flare activity level from turbulence parameters of photospheric plasma - Diagnostics of flare activity level from turbulence parameters of photospheric plasma ... non-linear dynamical system of magnetized plasma ...

Diagnostics of flare activity level from turbulence parameters of photospheric plasma ... non-linear dynamical system of magnetized plasma ...

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Coronal hard X-ray sources and associated decimetric/metric radio emissions PowerPoint PPT Presentation

Coronal hard X-ray sources and associated decimetric/metric radio emissions - Coronal hard X-ray sources and associated decimetric/metric radio emissions N. Vilmer D. Koutroumpa (Observatoire de Paris- LESIA) S.R Kane G. Hurford

Coronal hard X-ray sources and associated decimetric/metric radio emissions N. Vilmer D. Koutroumpa (Observatoire de Paris- LESIA) S.R Kane G. Hurford

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Size and Flux Asymmetry of Footpoint Sources PowerPoint PPT Presentation

Size and Flux Asymmetry of Footpoint Sources - They are also often asymmetric in size and magnetic field ... The size of the footpoint should be ... Old algorithms don't weight size sensitivity properly ...

They are also often asymmetric in size and magnetic field ... The size of the footpoint should be ... Old algorithms don't weight size sensitivity properly ...

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The Energetic Importance of Accelerated Electrons in Solar Flares PowerPoint PPT Presentation

The Energetic Importance of Accelerated Electrons in Solar Flares - ... in electrons is uncertain because of lower energy cutoff to spectrum. Thermal energy in plasma is uncertain because of uncertain volume, density, filling factor. ...

... in electrons is uncertain because of lower energy cutoff to spectrum. Thermal energy in plasma is uncertain because of uncertain volume, density, filling factor. ...

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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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Thick Target Coronal HXR Sources PowerPoint PPT Presentation

Thick Target Coronal HXR Sources - collapsing magnetic trap is the same for Fermi and betatron. mechanism. However, trap with dominant betatron acceleration confines particles better ...

collapsing magnetic trap is the same for Fermi and betatron. mechanism. However, trap with dominant betatron acceleration confines particles better ...

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Slajd 1 - Decay phase - HXR source observed 40 minutes after the maximum of the flare. ... HXR sources (above 15 keV) are visible even 6 hours after the maximum of the flare. ...

Decay phase - HXR source observed 40 minutes after the maximum of the flare. ... HXR sources (above 15 keV) are visible even 6 hours after the maximum of the flare. ...

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Rhessi PowerPoint PPT Presentations