A Burst with Double Radio Spectrum Observed up to 212 GHz
暂无分享,去创建一个
[1] J. Raulin,et al. Origin of the Submillimeter Radio Emission During the Time-Extended Phase of a Solar Flare , 2011, 1109.5729.
[2] M. Aschwanden,et al. Implications of X-ray Observations for Electron Acceleration and Propagation in Solar Flares , 2011, 1109.6496.
[3] G. Mann,et al. The Relationship Between Solar Radio and Hard X-ray Emission , 2011, 1109.6629.
[4] E. Kontar,et al. SUB-THz RADIATION MECHANISMS IN SOLAR FLARES , 2009, 0911.5335.
[5] H. Levato,et al. Submillimeter and X-ray observations of an X class flare , 2009, 0908.2339.
[6] C. Mandrini,et al. A solar burst with a spectral component observed only above 100 GHz during an M class flare , 2008 .
[7] Robert N. Martin,et al. New telescopes for ground-based solar observations at submillimeter and mid-infrared , 2008, Astronomical Telescopes + Instrumentation.
[8] S. Krucker,et al. Radio Submillimeter and γ-Ray Observations of the 2003 October 28 Solar Flare , 2008 .
[9] J. Raulin,et al. Evidence that Synchrotron Emission from Nonthermal Electrons Produces the Increasing Submillimeter Spectral Component in Solar Flares , 2007 .
[10] Joaquim E. R. Costa,et al. A very narrow gyrosynchrotron spectrum during a solar flare , 2006 .
[11] J. Raulin,et al. Can microbunch instability on solar flare accelerated electron beams account for bright broadband coherent synchrotron microwaves , 2006 .
[12] T. Lüthi,et al. Determination of the location and effective angular size of solar flares with a 210 GHz multibeam radiometer , 2004 .
[13] T. Lüthi,et al. First observation of a solar X-class flare in the submillimeter range with KOSMA , 2004 .
[14] Joaquim E. R. Costa,et al. A New Solar Burst Spectral Component Emitting Only in the Terahertz Range , 2004 .
[15] J. Brown,et al. Nonsolar astronomy with the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) , 2003, SPIE Astronomical Telescopes + Instrumentation.
[16] M. Aschwanden,et al. The RHESSI Imaging Concept , 2002 .
[17] V. Melnikov,et al. Fast temporal variations of the circular polarization degree during a microwave solar burst , 1999 .
[18] J. Raulin,et al. Instantaneous positions of microwave solar bursts: Properties and validity of the multiple beam observations , 1999 .
[19] R. Sunyaev,et al. A multiwavelength analysis of an electron-dominated gamma-ray event associated with a disk solar flare , 1998 .
[20] W. Neupert,et al. EIT: Extreme-ultraviolet Imaging Telescope for the SOHO mission , 1995 .
[21] H. Nakajima,et al. Gamma-ray and millimeter-wave emissions from the 1991 June X-class solar flares , 1994 .
[22] Alan M. Title,et al. The solar oscillations investigation - Michelson Doppler Imager. , 1992 .
[23] M. Kundu,et al. The high-frequency characteristics of solar radio bursts , 1992 .
[24] K. Klein,et al. Microwave diagnostics of energetic electrons in flares , 1986 .
[25] P. Kaufmann. The New Itapetinga Radio Observatory, from Mackenzie University, São Paulo, Brasil , 1971 .
[26] R. Ramaty. Gyrosynchrotron emission and absorption in a magnetoactive plasma , 1969 .
[27] J. Raulin,et al. First detection of the impulsive and extended phases of a solar radio burst above 200 GHz , 2002 .
[28] K. L. Harvey,et al. Observations of moving magnetic features near sunspots , 1973 .