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 ...
Particle accelerator that uses the electric field induced by a ... Fast electrons in particle physics. X-rays (radiation oncology) Best e--accelerators now ...
Solar Radio Astronomy. Adriana V. R. Silva. Center for Radio Astronomy ... 17 GHz: Nobeyama Solar Heliograph. 212 and 405 GHz: Submillimetric Solar Telescope ...
How are charged particles accelerated to relativistic energies ? ... EGRET (NASA) Solar and Heliospheric Observatory / EIT (ESA/NASA) log(frequency [Hz] ...
Betatron Maria Kazachenko Physics department Montana State University What is betatron? Outline Methods of electrons acceleration (historically) Van de Graaf high ...
Inversions of Flaring Radio Emissions. Gregory D. Fleishman. Relevant ... many radio bursts ... 2.Nonthermal radio emission depends not only on the ...
Centimeter and Millimeter Observations of Very Young Binary and Multiple Systems ... J. M. Torrelles (IEEC, Spain), J. M. Girart (U. Barcelona, Spain) ...
Lee et al 2000, - dynamics of spectral properties, electron anisotropy ... Fleishman & Melnikov 2003, - influence of electron pitch angle anisotropy ...
X-ray Observations of Stars. Rachel Osten. University of Maryland, NASA/GSFC ... ACIS image of Gl569, resolving the brown dwarf binary (Bab) from the M star primary ...
A hypothesis or theory is clear, decisive, and positive but it is believed by ... (But, they should have period modulation - the 'crazy tadpole wavelet spectra ...
Radio interferometry with elements (antennas) separated by hundreds ... flare stars (AD Leo) colliding winds (WR stars) SNe. GRBs. Maser emission from molecules ...
Radio interferometry with elements (antennas) separated ... parallax ok out to 10 kpc. 13. 14. 15. OH. H2O. SiO. 100 --- 10000 AU. 100s of AU. 16. Photosphere ...
... nonLTE radiative/convective equilibrium models for M, L, T dwarfs ... VB 10 ... As Teff decreases the atmospheres become far less ionized and poor ...
Solar origin of SEP events and dynamical ... the angular spread of the CMEs which reach their full extend in a few minutes. ... The July 14 2000 Halo CME event ...
Located at Taurus at 140 pc. Bolometric luminosity of 30 Lsun. Embedded in dense core (1000 AU) ... as circular polarization characteristics of southern source ...
... at the lower solar atmosphere gyrating around the magnetic field (gyro) ... Electrons gyrate along the field line and interact with the oblique whistler ...
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 ...
Black holes is the end state of a massive star in which gravitational ... A black hole is so compact that it has an escape velocity greater than the speed ...
Quiet Solar disk at 10,000 K (most pixels are at this temperature): QS ... See also Hanaoka & Shinkawa, 1999 on covering of bright plage by erupted filament ...
Rachel Osten (P): Detected variable 3.6 cm and 6 cm emission from the M8.5 V ... Ray Jayarardhana: Accreting brown dwarfs are slow rotators, so disk locking ...
Theoretical Model Images and Spectra for Comparison with HESSI and Microwave ... in part by the NASA Sun-Earth Connection Program. The Model Flare Loop ...
... Microwave and Hard X-Rays. Ayumi ASAI1, Hiroshi NAKAJIMA1, Masumi SHIMOJO1, Stephen M. WHITE2, Hugh ... 1: Nobeyama Solar Radio Observatory/NAOJ, 2:University of ...
Observations. ... The sensitivity range in this line has a maximum ... measured of (10 12)% resulted in incomprehensible magnetic fields of ~300 G at ~100 Mm. ...