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/s11207-011-9834-2

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: Contribution to journal › Article › peer-review

1125 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)
Pages (from-to)	207-227
Number of pages	21
Journal	Solar Physics
Volume	275
Issue number	1-2
DOIs	https://doi.org/10.1007/s11207-011-9834-2
State	Published - Jan 2012
Externally published	Yes

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

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

Access to Document

10.1007/s11207-011-9834-2

Fingerprint Dive into the research topics of 'The Helioseismic and Magnetic Imager (HMI) Investigation for the Solar Dynamics Observatory (SDO)'. Together they form a unique fingerprint.

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). Solar Physics, 275(1-2), 207-227. https://doi.org/10.1007/s11207-011-9834-2

@article{f0122b379f594d4db826ea227aaa4286,

title = "The Helioseismic and Magnetic Imager (HMI) Investigation for the Solar Dynamics Observatory (SDO)",

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",

note = "Funding Information: Acknowledgements The HMI project is supported by NASA contract NAS5-02139. Efforts to develop science analysis code for the pipeline have been supported by NASA grants NNG05GM85G, NNG06GE40G, NNX07AP61G, NNX09AB10G, NNX09AG81G, and NNX10AC55G. We wish to thank Elizabeth Citrin the NASA SDO Program Manager, Barbara Thompson and Dean Pesnell the SDO project scientists, Madhulika Guhathakurta the NASA LWS program scientist, Arthur Poland, George Withbroe, and Richard Fisher at NASA Headquarters for both formative and continuing support. Copyright: Copyright 2012 Elsevier B.V., All rights reserved.",

year = "2012",

month = jan,

doi = "10.1007/s11207-011-9834-2",

language = "English (US)",

volume = "275",

pages = "207--227",

journal = "Solar Physics",

issn = "0038-0938",

publisher = "Springer Netherlands",

number = "1-2",

}

The Helioseismic and Magnetic Imager (HMI) Investigation for the Solar Dynamics Observatory (SDO). / 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.

In: Solar Physics, Vol. 275, No. 1-2, 01.2012, p. 207-227.

Research output: Contribution to journal › Article › peer-review

TY - JOUR

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.

N1 - Funding Information: Acknowledgements The HMI project is supported by NASA contract NAS5-02139. Efforts to develop science analysis code for the pipeline have been supported by NASA grants NNG05GM85G, NNG06GE40G, NNX07AP61G, NNX09AB10G, NNX09AG81G, and NNX10AC55G. We wish to thank Elizabeth Citrin the NASA SDO Program Manager, Barbara Thompson and Dean Pesnell the SDO project scientists, Madhulika Guhathakurta the NASA LWS program scientist, Arthur Poland, George Withbroe, and Richard Fisher at NASA Headquarters for both formative and continuing support. Copyright: Copyright 2012 Elsevier B.V., All rights reserved.

PY - 2012/1

Y1 - 2012/1

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

UR - http://www.scopus.com/inward/record.url?scp=84855874213&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84855874213&partnerID=8YFLogxK

U2 - 10.1007/s11207-011-9834-2

DO - 10.1007/s11207-011-9834-2

M3 - Article

AN - SCOPUS:84855874213

VL - 275

SP - 207

EP - 227

JO - Solar Physics

JF - Solar Physics

SN - 0038-0938

IS - 1-2

ER -

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

Abstract

All Science Journal Classification (ASJC) codes

Keywords

Access to Document

Other files and links

Cite this