The stellar equations of state treat the Sun much like an ideal gas, wherein the photosphere is viewed as a sparse gaseous plasma. The temperatures inferred in the solar interior give some credence to these models, especially since it is counterintuitive that an object with internal temperatures in excess of 1 MK could be existing in the liquid state. Nonetheless, extreme temperatures, by themselves, are insufficient evidence for the states of matter. The presence of magnetic fields and gravity also impact the expected phase. In the end, it is the physical expression of a state that is required in establishing the proper phase of an object. The photosphere does not lend itself easily to treatment as a gase...
A historical summary of observations since 1960 raises questions about the standard solar model (SSM...
The Sun, because it is the star for which we have the largest set of observational constraints, is a...
The solar corona, the outer atmosphere of the Sun, is heated to millions of Kelvin. This is several ...
In this work, a liquid model of the Sun is presented wherein the entire solar mass is viewed as a hi...
The solar corona and chromosphere are often marked by eruptive features, such as flares, prominences...
UnrestrictedThe conditions in the solar interior are so extreme that it has so far been impossible t...
One of the basic questions of solar research is the nature of the Sun. We show here how the plasma n...
Our goal is to determine whether processes that led to the formation of planets in the solar system ...
One of the basic questions of solar research is the nature of the Sun. We show here how the plasma n...
The photosphere is the surface of the Sun that we see, and the direct source of its energy. It is do...
One of the basic questions of solar research is the nature of the Sun. We show here how the plasma n...
In this note, energy partition within the Sun is briefly addressed. It is argued that the laws of th...
International audienceContext. The Sun is the most constrained and well-studied of all stars. As a c...
History has the power to expose the origin and evolution of scientific ideas. How did humanity come ...
The chromosphere and corona of the Sun represent tenuous regions which are charac-terized by numerou...
A historical summary of observations since 1960 raises questions about the standard solar model (SSM...
The Sun, because it is the star for which we have the largest set of observational constraints, is a...
The solar corona, the outer atmosphere of the Sun, is heated to millions of Kelvin. This is several ...
In this work, a liquid model of the Sun is presented wherein the entire solar mass is viewed as a hi...
The solar corona and chromosphere are often marked by eruptive features, such as flares, prominences...
UnrestrictedThe conditions in the solar interior are so extreme that it has so far been impossible t...
One of the basic questions of solar research is the nature of the Sun. We show here how the plasma n...
Our goal is to determine whether processes that led to the formation of planets in the solar system ...
One of the basic questions of solar research is the nature of the Sun. We show here how the plasma n...
The photosphere is the surface of the Sun that we see, and the direct source of its energy. It is do...
One of the basic questions of solar research is the nature of the Sun. We show here how the plasma n...
In this note, energy partition within the Sun is briefly addressed. It is argued that the laws of th...
International audienceContext. The Sun is the most constrained and well-studied of all stars. As a c...
History has the power to expose the origin and evolution of scientific ideas. How did humanity come ...
The chromosphere and corona of the Sun represent tenuous regions which are charac-terized by numerou...
A historical summary of observations since 1960 raises questions about the standard solar model (SSM...
The Sun, because it is the star for which we have the largest set of observational constraints, is a...
The solar corona, the outer atmosphere of the Sun, is heated to millions of Kelvin. This is several ...