collapsing magnetic trap is the same for Fermi and betatron. mechanism. However, trap with dominant betatron acceleration confines particles better ...
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. ...
Some Ha kernels show no correnponding HXR burst. D:53cm Coronagraph. 9 Channel MSDP ... Elementary HXR bursts. Puzzling phenomena - Pre-heating in Ha ...
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. ...
The Timing of Hard X Rays and Radio Waves in Solar Flares ... Example: Radio Spectrogram vs. Demodulated RHESSI. HXR/Radio Correlation. Linear trend ...
Yohkoh Hard X-ray Telescope gave for the first time an opportunity for massive ... for HXRs (e.g. Frost & Dennis 1971, stereo-scopic papers of Kane) ...
the slit (05:19 UT). Reconnection Rate and Poynting Flux. microwave. HXR ... the slit (05: ... Poynting flux along each slit show good correlation with ...
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magnetic field line. Released energy by reconnection or induced energy into the region ... contour lines : magnetic field. Positive / Negative. E2. W2 ...
Hydrodynamic Modeling: Motivation. EUV is generally delayed to SXR as a consequence ... New code with analytical approximations to hydrodynamic evolution ...
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 ...
Energetic electrons acceleration: combined radio and X-ray diagnostics Hamish Reid1,2 Nicole Vilmer2 Eduard Kontar1 1University of Glasgow 2Observatoire de Paris
1 / 10. Comparison between Microwave and Hard X-ray Spectral Indices of Temporally and ... The time profiles of these frequencies are similar with each other. ...
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... sources are (at least) 10 times larger than those at the other ... IAU 223 Symposium, St. Petersburg, June 14 19 2004. Sartorius telescope @Kwasan Obs. ...
Some nice picture. Some nice pictures (continued) 20 July 2002. X3.3 flare on ... Hard X-ray source extends to 20-30'' over limb which when added to occultation ...
Cadence 1s 600 km/s. Continuum. 17 March 2002 Event B. 17 March 2002 Event A ... AR 9871 inside old remnant region. Inclusion of small interacting loops ...
... be able to count pulses faster then instrument dead ... is the channels balance and total number of pulses in both channels ... Accumulate pulses with HVtest ...
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 ...
Astronomy & Astrophysics. Group Profile. Prof John Brown (Astronomer ... Dr Alec Mackinnon (Dept. of Adult & Cont. Educ.) Dr Graham Woan. Faculty: Research and ...
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 ...
Electron Acceleration at the Solar Flare Reconnection Outflow Shocks. Gottfried Mann, Henry Aurass, and ... dynamic radio spectrogram height-time diagram ...
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 ...
NoRH Observations of RHESSI Microflares. M.R. Kundu, ... Dept. of Astronomy, University of Maryland, College Park, MD and Lab for ... RHESSI spectrogram. May 02 ...
Constraints on Particle Acceleration from Interplanetary Observations R. P. Lin together with L. Wang, S. Krucker at UC Berkeley, G Mason at U. Maryland,
Tokamaks are pulsed devices limited by the plasma current; however, ... LHCD works through electron Landau damping around v~3vth. LHCD is calculated based on ...
... neoplasm, and rarely in men as a nonseminomatous testicular. tumor ... Metaplasia to the trophoblast from a nongonadal tissue such as primary lung cancer. ...
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 ...
... Microwave and Hard X-Rays. Ayumi ASAI1, Hiroshi NAKAJIMA1, Masumi SHIMOJO1, Stephen M. WHITE2, Hugh ... 1: Nobeyama Solar Radio Observatory/NAOJ, 2:University of ...
S. Masuda (STEL, Nagoya Univ.) TOF analysis (Aschwanden et al. 1996) ... Low-frequency component: trap and precipitation. Ne = 1 - 2 1011 cm-3. Trapping region ...
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 ...
Plasma velocities observed with CDS during impulsive phase of 2 flares ... CDS observations with slit above a rising filament magnetic field extrapolations ...
e - 100 MeV (Moses et al 1989), maybe higher. p - several GeV (neutron ... THEMIS H , H : excitation by particle beams (directly or through return current) ...