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

doi:10.1063/1.3395873

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

Department of Physics

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

2 Citations (Scopus)

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 language	English
Title of host publication	AIP Conference Proceedings
Subtitle of host publication	Twelfth International Solar Wind Conference
Pages	355-358
Number of pages	4
Volume	1216
DOIs	https://doi.org/10.1063/1.3395873
Publication status	Published - 01 Mar 2010
Event	Twelfth International Solar Wind Conference - Saint-Malo, France Duration: 21 Jun 2009 → 26 Jun 2009

Conference

Conference	Twelfth International Solar Wind Conference
Country/Territory	France
City	Saint-Malo
Period	21 Jun 2009 → 26 Jun 2009

Access to Document

10.1063/1.3395873

Permanent link

Persistent link

Cite this

Bisi, M. M., Jackson, B. V., Hick, P. P., Clover, J. M., Hamilton, S., Tokumaru, M., & Fujiki, K. (2010). Large-Scale Heliospheric Structure during Solar-Minimum Conditions using a 3D Time-Dependent Reconstruction Solar-Wind Model and STELab IPS Observations. In AIP Conference Proceedings: Twelfth International Solar Wind Conference (Vol. 1216, pp. 355-358) https://doi.org/10.1063/1.3395873

@inproceedings{31be8929e135480aa75bb4756c10bd03,

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

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).",

author = "Bisi, {M. M.} and Jackson, {B. V.} and Hick, {P. P.} and Clover, {J. M.} and S. Hamilton and M. Tokumaru and K. Fujiki",

year = "2010",

month = mar,

day = "1",

doi = "10.1063/1.3395873",

language = "English",

volume = "1216",

pages = "355--358",

booktitle = "AIP Conference Proceedings",

note = "Twelfth International Solar Wind Conference ; Conference date: 21-06-2009 Through 26-06-2009",

}

Bisi, MM, Jackson, BV, Hick, PP, Clover, JM, Hamilton, S, Tokumaru, M & Fujiki, K 2010, Large-Scale Heliospheric Structure during Solar-Minimum Conditions using a 3D Time-Dependent Reconstruction Solar-Wind Model and STELab IPS Observations. in AIP Conference Proceedings: Twelfth International Solar Wind Conference. vol. 1216, pp. 355-358, Twelfth International Solar Wind Conference, Saint-Malo, France, 21 Jun 2009. https://doi.org/10.1063/1.3395873

Large-Scale Heliospheric Structure during Solar-Minimum Conditions using a 3D Time-Dependent Reconstruction Solar-Wind Model and STELab IPS Observations. / Bisi, M. M.; Jackson, B. V.; Hick, P. P. et al.
AIP Conference Proceedings: Twelfth International Solar Wind Conference. Vol. 1216 2010. p. 355-358.

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

TY - GEN

T1 - Large-Scale Heliospheric Structure during Solar-Minimum Conditions using a 3D Time-Dependent Reconstruction Solar-Wind Model and STELab IPS Observations

AU - Bisi, M. M.

AU - Jackson, B. V.

AU - Hick, P. P.

AU - Clover, J. M.

AU - Hamilton, S.

AU - Tokumaru, M.

AU - Fujiki, K.

PY - 2010/3/1

Y1 - 2010/3/1

N2 - 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).

AB - 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).

UR - http://hdl.handle.net/2160/9922

U2 - 10.1063/1.3395873

DO - 10.1063/1.3395873

M3 - Conference Proceeding (Non-Journal item)

VL - 1216

SP - 355

EP - 358

BT - AIP Conference Proceedings

T2 - Twelfth International Solar Wind Conference

Y2 - 21 June 2009 through 26 June 2009

ER -

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

Abstract

Conference

Access to Document

Permanent link

Other files and links

Fingerprint

Cite this