'Time profiles' presentation slideshows

OBSERVATION OF MICROWAVE OSCILLATIONS WITH SPATIAL RESOLUTION

OBSERVATION OF MICROWAVE OSCILLATIONS WITH SPATIAL RESOLUTION. V . E . Reznikova 1 , V . F . Melnikov 1 , K . Shibasaki 2 , V . M . Nakariakov 3 1 Radiophysical Research Institute, Nizhny Novgorod, Russia 2 Nobeyama Radio Observatory, NAOJ, Japan 3 University of Warwick, UK

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Electron Propagation in RHESSI flares

5 th General RHESSI Workshop, Locarno, Switzerland, 7-11 June 2005 Group 1 : Electron Acceleration and Propagation. Electron Propagation in RHESSI flares. Markus J. Aschwanden (LMSAL). Analysis of energy-dependent hard X-ray time delays:. Electron time-of-flight distance from dt/dE<0

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THREE-DIMENSIONAL ANISOTROPIC TRANSPORT OF SOLAR ENERGETIC PARTICLES IN THE INNER HELIOSPHERE

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20 JANUARY 2005 FLARE

20 JANUARY 2005 FLARE. Kuznetzov Sergey (PI), sergenik@srd.sinp.msu.ru, Kurt Victoria, vgk@srd.sinp.msu.ru, Yushkov Boris , clef@srd,sinp.msu.ru, Svertilov Sergey Skobeltzyn Institute of Nuclear Physics, Moscow State University

290 views • 20 slides

Remoxy In Vivo Abuse Resistance Studies

Remoxy In Vivo Abuse Resistance Studies. Ping Ji, PhD Senior Clinical Pharmacologist Office of Clinical Pharmacology Center of Drug Evaluation and Research Food and Drug Administration. In Vivo Abuse Resistance Studies. Physical Disruption Study Mastication (chewing) Study

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Flare-Associated Magnetic Field Changes Observed with HMI

Flare-Associated Magnetic Field Changes Observed with HMI. Permanent changes in photospheric magnetic fields have been observed to occur during solar flares (e.g., Sudol & Harvey 2005, Wang & Liu 2010, Petrie & Sudol 2010).

266 views • 15 slides

Towards Optics-Based Measurements in Ocean Observatories - The Argo program

Towards Optics-Based Measurements in Ocean Observatories - The Argo program E. Boss (H. Claustre , K. Johnson). What is Argo? Optical measurements on profiling floats. Integration of optical sensing into Argo. The Argo array. On average, a profile from 2000m every 10days.

281 views • 12 slides

Extended emission in short gamma-ray bursts registered by SPI-ACS of INTEGRAL observatory

Extended emission in short gamma-ray bursts registered by SPI-ACS of INTEGRAL observatory. Pavel Minaev 1, 2 , Alexei Pozanenko 1 , Vladimir Loznikov 1 1- Space Research Institute (Moscow, Russia) 2- Moscow State University (Moscow, Russia). GRB duration classification. ?.

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2. Essence 1. Choice of the time interval for imaging

2. Essence 1. Choice of the time interval for imaging NoRH correlation plots can be used for this. They can be misleading if the spatial structure is complex, but they show temporal variations of compact features. Then the image set over this time interval is produced.

112 views • 1 slides