Boundary conditions on model solar chromospheres

Abstract It is shown that the gas pressure in the corona provides a rather stringent boundary condition on model chromospheres and limits the thickness of those regions of the chromosphere in which the temperature is less than 10 000 K to less than or about 2000 km.

Gespeichert in:

Autor*in:	Athay, R. Grant [verfasserIn]

Format:	Artikel
Sprache:	Englisch

Erschienen:	1969

Schlagwörter:	Boundary Condition Solar Chromosphere Stringent Boundary Model Chromosphere Stringent Boundary Condition

Anmerkung:	© D. Reidel Publishing Company 1969

Übergeordnetes Werk:	Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 9(1969), 1 vom: Sept., Seite 51-55
Übergeordnetes Werk:	volume:9 ; year:1969 ; number:1 ; month:09 ; pages:51-55

Links:	Volltext

DOI / URN:	10.1007/BF00145727

Katalog-ID:	OLC2033520137

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abstract	Abstract It is shown that the gas pressure in the corona provides a rather stringent boundary condition on model chromospheres and limits the thickness of those regions of the chromosphere in which the temperature is less than 10 000 K to less than or about 2000 km. © D. Reidel Publishing Company 1969
abstractGer	Abstract It is shown that the gas pressure in the corona provides a rather stringent boundary condition on model chromospheres and limits the thickness of those regions of the chromosphere in which the temperature is less than 10 000 K to less than or about 2000 km. © D. Reidel Publishing Company 1969
abstract_unstemmed	Abstract It is shown that the gas pressure in the corona provides a rather stringent boundary condition on model chromospheres and limits the thickness of those regions of the chromosphere in which the temperature is less than 10 000 K to less than or about 2000 km. © D. Reidel Publishing Company 1969
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