Microwave Mode Coupling Above Active Regions as a Coronal Density Diagnostic
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Stephen M. White | Mukul R. Kundu | Zoran Mikic | S. White | Jeongwoo Lee | Z. Mikić | A. Mcclymont | Jeongwoo Lee | A. N. McClymont | M. R. Kundu
[1] Z. Mikić,et al. PROBLEMS AND PROGRESS IN COMPUTING THREE-DIMENSIONAL CORONAL ACTIVE REGION MAGNETIC FIELDS FROM BOUNDARY DATA , 1997 .
[2] Stephen M. White,et al. Radio Observations of Gyroresonance Emission from Coronal Magnetic Fields , 1997 .
[3] Z. Mikić,et al. RECONSTRUCTION OF THE THREE-DIMENSIONAL CORONAL MAGNETIC FIELD , 1997 .
[4] S. White,et al. SIGNATURES OF CORONAL CURRENTS IN MICROWAVE IMAGES , 1997 .
[5] K. Shibasaki,et al. Coronal magnetic fields from microwave polarization observations , 1996 .
[6] V. Zheleznyakov,et al. Linear mode coupling and polarization features of radiation in current sheets. , 1996 .
[7] N. Gopalswamy,et al. Polarization features of solar radio emission and possible existence of current sheets in active regions , 1994 .
[8] G. Holman,et al. Coronal Magnetic Structures Observing Campaign. 3: Coronal plasma and magnetic field diagnostics derived from multiwaveband active region observations , 1994 .
[9] C. Alissandrakis,et al. Detection of Linear Polarization in the Microwave Emission of Solar Active Regions , 1994 .
[10] G. Thejappa,et al. Observations of mode coupling in the solar corona and bipolar noise storms , 1992 .
[11] M. Kundu,et al. Large-scale features of the sun at 20 centimeter wavelength , 1991 .
[12] G. Rottman,et al. The solar coronal density irregularity n squared bar/(n bar) squared derived from simultaneous measurements of the EUV and K-coronal brightness , 1990 .
[13] M. Kundu,et al. Structure and polarization of active region microwave emission , 1984 .
[14] C. Alissandrakis,et al. On the computation of constant alpha force-free magnetic field , 1981 .
[15] D. Melrose. Small-scale inhomogeneities in the solar corona: Evidence from meter-λ radio bursts , 1975 .
[16] M. Cohen. Magnetoionic Mode Coupling at High Frequencies. , 1960 .