We report an initial study of temperature and emission measure distributions along four steady loops observed with the Transition Region and Coronal Explorer (TRACE) at the limb of the Sun. The temperature diagnostic is the filter ratio of the extreme-ultraviolet 171-angstrom and 195-angstrom passbands. The emission measure diagnostic is the count rate in the 171-angstrom passband. We find essentially no temperature variation along the loops. We compare the observed loop structure with theoretical isothermal and nonisothermal static loop structure
Abstract. This study focuses on the diagnostic capabilities of the TRACE and SOHO-CDS instruments to...
New and advanced space-based observing facilities continue to lower the resolution limit and detect ...
The CHIANTI spectral code is used to estimate line and continuum intensity contributions to the TRAC...
Aims.We analyze a well-defined loop system detected in a time-resolved observation in several spectr...
This thesis presents an observational analysis of structures in the solar corona. The plasmafl in th...
In the present work SOHO Coronal Diagnostic Spectrometer (CDS) observations of a quiescent active re...
This work is prompted by evidence of sharply peaked emission measure distributions in active stars a...
The Enthalpy Based Thermal Evolution of Loops approximate model for static and dynamic coronal loops...
We study the temporal evolution of coronal loops using data from the Solar X-ray Imager (SXI) on boa...
Determining the preferred spatial location of the energy input to solar coronal loops would be an im...
Magnetic loops are building blocks of the closed-field corona. While active region loops are readily...
We derived the temperature distributions along the 16 steady loops observed with the Yohkoh Soft X-r...
We examine the temperature structure of static coronal active region loops in regimes where thermal ...
Coronal loops form the basic building blocks of the magnetically closed solar corona yet much is sti...
Magnetic loops are building blocks of the closed-field corona. While active region loops are readily...
Abstract. This study focuses on the diagnostic capabilities of the TRACE and SOHO-CDS instruments to...
New and advanced space-based observing facilities continue to lower the resolution limit and detect ...
The CHIANTI spectral code is used to estimate line and continuum intensity contributions to the TRAC...
Aims.We analyze a well-defined loop system detected in a time-resolved observation in several spectr...
This thesis presents an observational analysis of structures in the solar corona. The plasmafl in th...
In the present work SOHO Coronal Diagnostic Spectrometer (CDS) observations of a quiescent active re...
This work is prompted by evidence of sharply peaked emission measure distributions in active stars a...
The Enthalpy Based Thermal Evolution of Loops approximate model for static and dynamic coronal loops...
We study the temporal evolution of coronal loops using data from the Solar X-ray Imager (SXI) on boa...
Determining the preferred spatial location of the energy input to solar coronal loops would be an im...
Magnetic loops are building blocks of the closed-field corona. While active region loops are readily...
We derived the temperature distributions along the 16 steady loops observed with the Yohkoh Soft X-r...
We examine the temperature structure of static coronal active region loops in regimes where thermal ...
Coronal loops form the basic building blocks of the magnetically closed solar corona yet much is sti...
Magnetic loops are building blocks of the closed-field corona. While active region loops are readily...
Abstract. This study focuses on the diagnostic capabilities of the TRACE and SOHO-CDS instruments to...
New and advanced space-based observing facilities continue to lower the resolution limit and detect ...
The CHIANTI spectral code is used to estimate line and continuum intensity contributions to the TRAC...