'Rhessi' presentation slideshows

The Non-Flare Temperature and Emission Measure Observed by RHESSI and SXI

The Non-Flare Temperature and Emission Measure Observed by RHESSI and SXI. J.McTiernan (SSL/UCB) J.Klimchuk (NRL) Fall 2003 AGU Meeting. Abstract:

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Loop-top altitude decrease in an X-class flare

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RHESSI OBSERVATIONS OF THE 2005 JANUARY 20 SOLAR FLARE

RHESSI OBSERVATIONS OF THE 2005 JANUARY 20 SOLAR FLARE. Gerald Share 1,2 , Ronald Murphy 2 , David Smith 3 , Gordon Hurford 4 , Allan Tylka 2 , and Robert Lin 4. 1 UMD, 2 NRL, 3 UCSC, 4 UCB. Supported by NASA SEC-GI & SR&T. SUMMARY

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First RHESSI Results Brian R. Dennis RHESSI Mission Scientist Code 682

First RHESSI Results Brian R. Dennis RHESSI Mission Scientist Code 682. Space Sciences Directorate Monthly Report Monday, 25 March 2002. The Reuven Ramaty High Energy Solar Spectroscopic Image - RHESSI. Solar Flares.

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First RHESSI Results Brian R. Dennis RHESSI Mission Scientist Code 682

First RHESSI Results Brian R. Dennis RHESSI Mission Scientist Code 682. Space Sciences Directorate Monthly Report Monday, 25 March 2002. The Reuven Ramaty High Energy Solar Spectroscopic Image - RHESSI. Solar Flares.

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Comparing Solar-Flare Acceleration of >~20 MeV Protons and Electrons Above Various Energies

National Aeronautics and Space Administration. Comparing Solar-Flare Acceleration of >~20 MeV Protons and Electrons Above Various Energies. Albert Y. Shih NASA Goddard Space Flight Center. Comparing ions and electrons. Do all flares accelerate ions and electrons?

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Cristina Chifor SESI Student Intern 2005 Solar Physics, Code 612 NASA/Goddard Space Flight Center

FE AND FE/NI SPECTRAL LINE COMPLEXES IN RHESSI SOFT X-RAYS. Cristina Chifor SESI Student Intern 2005 Solar Physics, Code 612 NASA/Goddard Space Flight Center Mentors: Dr. Ken Phillips & Dr. Brian Dennis. SOLAR FLARE X-RAYS. 2. Thermal Depends on the random thermal

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RHESSI Investigations of the Neupert Effect in Solar Flares

RHESSI Investigations of the Neupert Effect in Solar Flares. Brian R. Dennis AAS/SPD Meeting 6 June 2002. The Neupert Effect. The time integral of the hard X-ray emission closely matches the temporal variation of the soft X-ray emission.

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RHESSI Hard X-Ray Observations of an EUV Jet on August 21, 2003

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RHESSI Investigations of the Neupert Effect in Solar Flares

RHESSI Investigations of the Neupert Effect in Solar Flares. Brian R. Dennis AAS/SPD Meeting 6 June 2002. The Neupert Effect. The time integral of the hard X-ray emission closely matches the temporal variation of the soft X-ray emission.

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Flare footpoints in optical and UV

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X-ray and radio observations of the 20 February 2002 solar flare

X-ray and radio observations of the 20 February 2002 solar flare. Nicole Vilmer (Observatoire de Paris- LESIA) S. Krucker, R.P. Lin (Space Sciences Laboratory Berkeley) R.Schwartz ( LASP/GSFC & SSAI ) A. Klassen ( AIP Potsdam ) RHESSI team.

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GSFC Space Science Mission Operations (SSMO) and Space Weather

GSFC Space Science Mission Operations (SSMO) and Space Weather. Rick Harman Space Science Mission Operations. SSMO Spacecraft. SSMO Spacecraft. Stereo Behind. LRO, ARTEMIS. Sun. GEO: SDO. L1: ACE, SOHO, WIND. LEO: AIM, Fermi, IRIS, RHESSI, Swift, TIMED.

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RHESSI Press Conference

RHESSI Press Conference. Brian R. Dennis RHESSI Mission Scientist NASA Goddard Space Flight Center. AAS/SPD Meeting Albuquerque, NM Wednesday, 5 June 2002. The Reuven Ramaty High Energy Solar Spectrometer (RHESSI). Launched on 5 Feb. 2002 on Pegasus rocket

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