High Spatial Resolution Observations of the Solar Transition Region: Spicules and Microflares

1991 ◽  
pp. 83-96 ◽  
Author(s):  
John W. Cook
Keyword(s):  
Transition Region ◽  
Spatial Resolution ◽  
High Spatial Resolution ◽  
Solar Transition Region ◽  
Solar Transition

scholarly journals Dopplershifts in the solar transition region

2001 ◽  
Vol 378 (1) ◽  
pp. 257-265 ◽  
Author(s):  
C. Gontikakis ◽  
H. C. Dara ◽  
C. E. Alissandrakis ◽  
Th. G. Zachariadis ◽  
J.-C. Vial
Keyword(s):  
Transition Region ◽  
Solar Transition Region ◽  
Solar Transition

scholarly journals Observations of the Quiet Sun with 6″ Resolution

1980 ◽  
Vol 86 ◽  
pp. 53-55
Author(s):  
M. R. Kundu ◽  
A. P. Rao ◽  
F. T. Erskine ◽  
J. D. Bregman
Keyword(s):  
High Resolution ◽  
Radio Emission ◽  
Transition Region ◽  
Spatial Resolution ◽  
Radio Telescope ◽  
Solar Radio ◽  
High Spatial Resolution ◽  
Solar Radio Emission ◽  
Quiet Sun ◽  
Millimeter Wavelengths

Solar radio emission at centimeter and millimeter wavelengths originates in the chromosphere and transition region and is a useful probe for the temperature and density in these regions. High spatial resolution observations of the quiet sun provide valuable information on the structure of the solar atmosphere. We have performed high resolution (~ 6″ (E-W) x 15″ (N-S)) observations at 6 cm with the Westerbork Synthesis Radio Telescope (WSRT) in June 1976 in order to search for the radio analog of the supergranulation network and to study the extent and symmetry of limb brightening. The use of the WSRT for high spatial resolution solar mapping has been described by Bregman and Felli (1976), Kundu et al. (1977), and others.

scholarly journals On the Magnetic Structure of the Solar Transition Region

2008 ◽  
Vol 687 (2) ◽  
pp. 1388-1397 ◽  
Author(s):  
Philip Judge ◽  
Rebecca Centeno
Keyword(s):  
Magnetic Structure ◽  
Transition Region ◽  
Solar Transition Region ◽  
Solar Transition
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