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Full Record Details
Persistent URL
http://purl.org/net/epubs/work/10916719
Record Status
Checked
Record Id
10916719
Title
Large-Scale Heliospheric Structure during Solar-Minimum Conditions using a 3D Time-Dependent Reconstruction Solar-Wind Model and STELab IPS Observations
Contributors
MM Bisi
,
BV Jackson
,
PP Hick
,
JM Clover
,
S Hamilton
,
M Tokumaru
,
K Fujiki
Abstract
Interplanetary scintillation (IPS) observations provide information about a large portion of the inner heliosphere. We have used Solar-Terrestrial Environment Laboratory (STELab) IPS velocity and g-level observations with our three-dimensional (3D) reconstruction model to determine velocities and densities of the inner heliosphere in three dimensions. We present these observations using synoptic maps generated from our time-dependent model that can measure changes with durations of less than one day. These synopses show large-scale stable solar-wind structure during solar-minimum conditions in relation to transients that are present during this period. These are also available as differences relative to the background. Here, we concentrate primarily on data covering the 2007-2009 International Heliophysical Year (IHY).
Organisation
STFC
,
RALSP
,
RALSP - SPD
Keywords
Heliosphere
Funding Information
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Licence Information:
Language
English (EN)
Type
Details
URI(s)
Local file(s)
Year
Journal Article
AIP Conf Proc
1216 (2010): 355-358. Is in proceedings of: Twelfth International Solar Wind Conference, Saint-Malo, France, 21-26 Jun 2009.
doi:10.1063/1.3395873
2010
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