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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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Progress in Understanding Radio Emission from Solar Flares PowerPoint PPT Presentation
Progress in Understanding Radio Emission from Solar Flares - Sample of 412 OVSA events (1.2-18 GHZ) ... Greyscale:-12 kev; Contours: 25-50 keV. Coronal thick-target flares. Veronig & Brown 2004 ...
Sample of 412 OVSA events (1.2-18 GHZ) ... Greyscale:-12 kev; Contours: 25-50 keV. Coronal thick-target flares. Veronig & Brown 2004 ...
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Future instrumentation for high-energy PowerPoint PPT Presentation
Future instrumentation for high-energy - OK, it's really the neutron and gamma-ray. detector proposed ... a spectrogram: AUI, NRAO/NSF, NJIT, et al. http://www.ovsa.njit.edu/fasr/ G. Graphics: NJIT/NSF ...
OK, it's really the neutron and gamma-ray. detector proposed ... a spectrogram: AUI, NRAO/NSF, NJIT, et al. http://www.ovsa.njit.edu/fasr/ G. Graphics: NJIT/NSF ...
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Discovery of Relativistic Positrons in Solar Flares with Microwave Imaging and Polarimetry PowerPoint PPT Presentation
Discovery of Relativistic Positrons in Solar Flares with Microwave Imaging and Polarimetry - Discovery of Relativistic Positrons in Solar Flares with Microwave Imaging and Polarimetry Gregory D. Fleishman, Alexander T. Altyntsev, Natalia S. Meshalkina
Discovery of Relativistic Positrons in Solar Flares with Microwave Imaging and Polarimetry Gregory D. Fleishman, Alexander T. Altyntsev, Natalia S. Meshalkina
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Inversions of Flaring Radio Emissions PowerPoint PPT Presentation
Inversions of Flaring Radio Emissions - Inversions of Flaring Radio Emissions. Gregory D. Fleishman. Relevant ... many radio bursts ... 2.Nonthermal radio emission depends not only on the ...
Inversions of Flaring Radio Emissions. Gregory D. Fleishman. Relevant ... many radio bursts ... 2.Nonthermal radio emission depends not only on the ...
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The Electromagnetic Spectrum PowerPoint PPT Presentation
The Electromagnetic Spectrum - The Electromagnetic Spectrum
The Electromagnetic Spectrum
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Multiwavelength Study of Magnetic Reconnection Associated with Sigmoid Eruption Chang Liu BBSONJIT 2 PowerPoint PPT Presentation
Multiwavelength Study of Magnetic Reconnection Associated with Sigmoid Eruption Chang Liu BBSONJIT 2 - Multiwavelength Study of Magnetic Reconnection Associated with Sigmoid Eruption Chang Liu BBSONJIT 2
Multiwavelength Study of Magnetic Reconnection Associated with Sigmoid Eruption Chang Liu BBSONJIT 2
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Space Weather Prediction at Big Bear Solar Observatory PowerPoint PPT Presentation
Space Weather Prediction at Big Bear Solar Observatory - Big Bear Solar Observatory. 3. BBSO White Light Image of Sun 8/20/1999. Sun's Temperature: ... Big Bear Solar Observatory. 7. 6/25/09. Big Bear Solar ...
Big Bear Solar Observatory. 3. BBSO White Light Image of Sun 8/20/1999. Sun's Temperature: ... Big Bear Solar Observatory. 7. 6/25/09. Big Bear Solar ...
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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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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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FASR Flare Science: Lessons from the Nobeyama Radioheliograph PowerPoint PPT Presentation
FASR Flare Science: Lessons from the Nobeyama Radioheliograph - The NoRH specifications that are important for flare research ... New simulations are underway by Vourlidas and Marque. see Vourlidas, 2004?Chapter 11 ...
The NoRH specifications that are important for flare research ... New simulations are underway by Vourlidas and Marque. see Vourlidas, 2004?Chapter 11 ...
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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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E3 Engineering Division PowerPoint PPT Presentation
E3 Engineering Division - First fast GPS scintillation receiver (50 sps) ... Sounding rocket GPS receivers. Decoding of first Galileo PRN code ( 83,000 hits on web site) Numerous papers ...
First fast GPS scintillation receiver (50 sps) ... Sounding rocket GPS receivers. Decoding of first Galileo PRN code ( 83,000 hits on web site) Numerous papers ...
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Upgrade of the Siberian Solar Radio Telescope PowerPoint PPT Presentation
Upgrade of the Siberian Solar Radio Telescope - Six antenna array example of the SSRT upgrading. The tuned. LO set. Fiber-optic cable and sampler. ... technical problems (for example, now it is considered two ...
Six antenna array example of the SSRT upgrading. The tuned. LO set. Fiber-optic cable and sampler. ... technical problems (for example, now it is considered two ...
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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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24 Oct 2001 A Cool, Dense Flare
24 Oct 2001 A Cool, Dense Flare - OVSA: 1-14.8 GHz, 2 s cadence, total flux, Stokes I ... TRACE: 171 A imaging, 40 s cadence (0.5') Yohkoh SXT: Single Al/Mg full disk image (4.92' ...
OVSA: 1-14.8 GHz, 2 s cadence, total flux, Stokes I ... TRACE: 171 A imaging, 40 s cadence (0.5') Yohkoh SXT: Single Al/Mg full disk image (4.92' ...


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