The Helioseismic and Magnetic Imager (HMI) investigation for the Solar Dynamics Observatory (SDO)

P. H. Scherrer; J. Schou; R. I. Bush; A. G. Kosovichev; R. S. Bogart; J. T. Hoeksema; Y. Liu; T. L. Duvall; J. Zhao; A. M. Title; C. J. Schrijver; T. D. Tarbell; S. Tomczyk

doi:10.1007/978-1-4614-3673-7_10

The Helioseismic and Magnetic Imager (HMI) investigation for the Solar Dynamics Observatory (SDO)

P. H. Scherrer, J. Schou, R. I. Bush, A. G. Kosovichev, R. S. Bogart, J. T. Hoeksema, Y. Liu, T. L. Duvall, J. Zhao, A. M. Title, C. J. Schrijver, T. D. Tarbell, S. Tomczyk

Research output: Chapter in Book/Report/Conference proceeding › Chapter

7 Scopus citations

Abstract

The Helioseismic and Magnetic Imager (HMI) instrument and investigation as a part of the NASA Solar Dynamics Observatory (SDO) is designed to study convection-zone dynamics and the solar dynamo, the origin and evolution of sunspots, active regions, and complexes of activity, the sources and drivers of solar magnetic activity and disturbances, links between the internal processes and dynamics of the corona and heliosphere, and precursors of solar disturbances for space-weather forecasts. A brief overview of the instrument, investigation objectives, and standard data products is presented.

Original language	English (US)
Title of host publication	The Solar Dynamics Observatory
Publisher	Springer US
Pages	207-227
Number of pages	21
Volume	9781461436737
ISBN (Electronic)	9781461436737
ISBN (Print)	1461436729, 9781461436720
DOIs	https://doi.org/10.1007/978-1-4614-3673-7_10
State	Published - Nov 1 2012
Externally published	Yes

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

Keywords

Helioseismology
Instrumentation and data management
Magnetic fields, photosphere
Solar Dynamics Observatory

Access to Document

10.1007/978-1-4614-3673-7_10

Cite this

Scherrer, P. H., Schou, J., Bush, R. I., Kosovichev, A. G., Bogart, R. S., Hoeksema, J. T., Liu, Y., Duvall, T. L., Zhao, J., Title, A. M., Schrijver, C. J., Tarbell, T. D., & Tomczyk, S. (2012). The Helioseismic and Magnetic Imager (HMI) investigation for the Solar Dynamics Observatory (SDO). In The Solar Dynamics Observatory (Vol. 9781461436737, pp. 207-227). Springer US. https://doi.org/10.1007/978-1-4614-3673-7_10

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abstract = "The Helioseismic and Magnetic Imager (HMI) instrument and investigation as a part of the NASA Solar Dynamics Observatory (SDO) is designed to study convection-zone dynamics and the solar dynamo, the origin and evolution of sunspots, active regions, and complexes of activity, the sources and drivers of solar magnetic activity and disturbances, links between the internal processes and dynamics of the corona and heliosphere, and precursors of solar disturbances for space-weather forecasts. A brief overview of the instrument, investigation objectives, and standard data products is presented.",

keywords = "Helioseismology, Instrumentation and data management, Magnetic fields, photosphere, Solar Dynamics Observatory",

author = "Scherrer, {P. H.} and J. Schou and Bush, {R. I.} and Kosovichev, {A. G.} and Bogart, {R. S.} and Hoeksema, {J. T.} and Y. Liu and Duvall, {T. L.} and J. Zhao and Title, {A. M.} and Schrijver, {C. J.} and Tarbell, {T. D.} and S. Tomczyk",

year = "2012",

month = nov,

day = "1",

doi = "10.1007/978-1-4614-3673-7_10",

language = "English (US)",

isbn = "1461436729",

volume = "9781461436737",

pages = "207--227",

booktitle = "The Solar Dynamics Observatory",

publisher = "Springer US",

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Scherrer, PH, Schou, J, Bush, RI, Kosovichev, AG, Bogart, RS, Hoeksema, JT, Liu, Y, Duvall, TL, Zhao, J, Title, AM, Schrijver, CJ, Tarbell, TD & Tomczyk, S 2012, The Helioseismic and Magnetic Imager (HMI) investigation for the Solar Dynamics Observatory (SDO). in The Solar Dynamics Observatory. vol. 9781461436737, Springer US, pp. 207-227. https://doi.org/10.1007/978-1-4614-3673-7_10

TY - CHAP

T1 - The Helioseismic and Magnetic Imager (HMI) investigation for the Solar Dynamics Observatory (SDO)

AU - Scherrer, P. H.

AU - Schou, J.

AU - Bush, R. I.

AU - Kosovichev, A. G.

AU - Bogart, R. S.

AU - Hoeksema, J. T.

AU - Liu, Y.

AU - Duvall, T. L.

AU - Zhao, J.

AU - Title, A. M.

AU - Schrijver, C. J.

AU - Tarbell, T. D.

AU - Tomczyk, S.

PY - 2012/11/1

Y1 - 2012/11/1

N2 - The Helioseismic and Magnetic Imager (HMI) instrument and investigation as a part of the NASA Solar Dynamics Observatory (SDO) is designed to study convection-zone dynamics and the solar dynamo, the origin and evolution of sunspots, active regions, and complexes of activity, the sources and drivers of solar magnetic activity and disturbances, links between the internal processes and dynamics of the corona and heliosphere, and precursors of solar disturbances for space-weather forecasts. A brief overview of the instrument, investigation objectives, and standard data products is presented.

AB - The Helioseismic and Magnetic Imager (HMI) instrument and investigation as a part of the NASA Solar Dynamics Observatory (SDO) is designed to study convection-zone dynamics and the solar dynamo, the origin and evolution of sunspots, active regions, and complexes of activity, the sources and drivers of solar magnetic activity and disturbances, links between the internal processes and dynamics of the corona and heliosphere, and precursors of solar disturbances for space-weather forecasts. A brief overview of the instrument, investigation objectives, and standard data products is presented.

KW - Helioseismology

KW - Instrumentation and data management

KW - Magnetic fields, photosphere

KW - Solar Dynamics Observatory

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U2 - 10.1007/978-1-4614-3673-7_10

DO - 10.1007/978-1-4614-3673-7_10

M3 - Chapter

AN - SCOPUS:84949180388

SN - 1461436729

SN - 9781461436720

VL - 9781461436737

SP - 207

EP - 227

BT - The Solar Dynamics Observatory

PB - Springer US

ER -

The Helioseismic and Magnetic Imager (HMI) investigation for the Solar Dynamics Observatory (SDO)

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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