Large-Scale Heliospheric Structure during Solar-Minimum Conditions using a 3D Time-Dependent Reconstruction Solar-Wind Model and STELab IPS Observations

M. M. Bisi, B. V. Jackson, P. P. Hick, J. M. Clover, S. Hamilton, M. Tokumaru, K. Fujiki

Research output: Chapter in Book/Report/Conference proceedingConference Proceeding (Non-Journal item)

2 Citations (SciVal)

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).
Original languageEnglish
Title of host publicationAIP Conference Proceedings
Subtitle of host publicationTwelfth International Solar Wind Conference
Pages355-358
Number of pages4
Volume1216
DOIs
Publication statusPublished - 01 Mar 2010
EventTwelfth International Solar Wind Conference - Saint-Malo, France
Duration: 21 Jun 200926 Jun 2009

Conference

ConferenceTwelfth International Solar Wind Conference
Country/TerritoryFrance
CitySaint-Malo
Period21 Jun 200926 Jun 2009

Fingerprint

Dive into the research topics of 'Large-Scale Heliospheric Structure during Solar-Minimum Conditions using a 3D Time-Dependent Reconstruction Solar-Wind Model and STELab IPS Observations'. Together they form a unique fingerprint.

Cite this