On the ultraviolet signatures of small scale heating in coronal loops

Astronomy and Astrophysics

Volumn 492, Issue 3, 2008, Pages 857-862

  Parenti, S ^a   Young, R ^b  

^a ROYAL OBSERVATORY OF BELGIUM   (Belgium)

^b RUTHERFORD APPLETON LABORATORY   (United Kingdom)

Author keywords

Methods: statistical; Plasmas; Sun: corona; Sun: UV radiation

Indexed keywords

AERODYNAMIC HEATING; ELECTROMAGNETIC WAVE EMISSION; FLUID DYNAMICS; FUNCTIONS; HEATING; IONS; LITHIUM; NEON; PLASMAS; PROBABILITY DENSITY FUNCTION; SOLAR ENERGY; SOLAR HEATING; SPECTROMETERS; SPECTROMETRY; STATISTICS; SUN; ULTRAVIOLET RADIATION; ULTRAVIOLET SPECTROSCOPY;

CHARACTERISTIC TEMPERATURES; CONTRIBUTION FUNCTIONS; CORONAL HEATING; CORONAL LOOPS; EMISSION LINES; HEATING FUNCTIONS; HIGH TEMPERATURES; HYDRODYNAMIC MODELS; IMAGING INSTRUMENTS; INTENSITY DISTRIBUTIONS; ISOELECTRONIC SEQUENCES; LITHIUM ISOELECTRONIC SEQUENCES; LOOP SYSTEMS; METHODS: STATISTICAL; NANOFLARES; POWER LAW INDICES; SMALL SCALES; STATISTICAL DISTRIBUTIONS; STATISTICAL PROPERTIES; STRONG RESONANCES; SUN: CORONA; SUN: UV RADIATION; ULTRA VIOLETS; ULTRAVIOLET EMISSIONS; UNRESOLVED SCALES; UV EMISSIONS;

STATISTICAL METHODS;

EID: 57649202591     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809928     Document Type: Article

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