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An interpretation of the I-V phase background based on observed plasma jets

Academic Article
Publication Date:
2002
abstract:
The presence of a solar background in the phase difference between the intensity and velocity (I - V) p-mode oscillation signals recently has been interpreted in terms of downflows due to convection (Skartlien & Rast 2000) or due to chromospheric explosive events (Moretti et al. 2001a). In support of the latter, we present I and V characteristics of impulsive brightenings observed in the NaI D lines, show that these reproduce the frequency dependence of the I - V modulation background, and show that explanations invoking more frequently occurring phenomena such as seismic events are not likely in low-elle modulation data.
Iris type:
01.01 Articolo in rivista
List of contributors:
Moretti, PIER FRANCESCO
Authors of the University:
MORETTI PIER FRANCESCO
Handle:
https://iris.cnr.it/handle/20.500.14243/7525
Published in:
ASTRONOMY & ASTROPHYSICS (ONLINE)
Journal
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