Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO)

Abstract The Helioseismic and Magnetic Imager (HMI) investigation (Solar Phys. doi:10.1007/s11207-011-9834-2, 2011) will study the solar interior using helioseismic techniques as well as the magnetic field near the solar surface. The HMI instrument is part of the Solar Dynamics Observatory (SDO) tha...
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Autor*in:	Schou, J. [verfasserIn] Scherrer, P. H. Bush, R. I. Wachter, R. Couvidat, S. Rabello-Soares, M. C. Bogart, R. S. Hoeksema, J. T. Liu, Y. Duvall, T. L. Akin, D. J. Allard, B. A. Miles, J. W. Rairden, R. Shine, R. A. Tarbell, T. D. Title, A. M. Wolfson, C. J. Elmore, D. F. Norton, A. A. Tomczyk, S.

Format:	Artikel
Sprache:	Englisch

Erschienen:	2011

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

Anmerkung:	© The Author(s) 2011

Übergeordnetes Werk:	Enthalten in: Solar physics - Springer Netherlands, 1967, 275(2011), 1-2 vom: 04. Okt., Seite 229-259
Übergeordnetes Werk:	volume:275 ; year:2011 ; number:1-2 ; day:04 ; month:10 ; pages:229-259

Links:	Volltext

DOI / URN:	10.1007/s11207-011-9842-2

Katalog-ID:	OLC2033610004

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700	1		\|a Norton, A. A. \|4 aut
700	1		\|a Tomczyk, S. \|4 aut
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allfields	10.1007/s11207-011-9842-2 doi (DE-627)OLC2033610004 (DE-He213)s11207-011-9842-2-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Schou, J. verfasserin aut Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO) 2011 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2011 Abstract The Helioseismic and Magnetic Imager (HMI) investigation (Solar Phys. doi:10.1007/s11207-011-9834-2, 2011) will study the solar interior using helioseismic techniques as well as the magnetic field near the solar surface. The HMI instrument is part of the Solar Dynamics Observatory (SDO) that was launched on 11 February 2010. The instrument is designed to measure the Doppler shift, intensity, and vector magnetic field at the solar photosphere using the 6173 Å Fe i absorption line. The instrument consists of a front-window filter, a telescope, a set of waveplates for polarimetry, an image-stabilization system, a blocking filter, a five-stage Lyot filter with one tunable element, two wide-field tunable Michelson interferometers, a pair of $ 4096^{2} $ pixel cameras with independent shutters, and associated electronics. Each camera takes a full-disk image roughly every 3.75 seconds giving an overall cadence of 45 seconds for the Doppler, intensity, and line-of-sight magnetic-field measurements and a slower cadence for the full vector magnetic field. This article describes the design of the HMI instrument and provides an overview of the pre-launch calibration efforts. Overviews of the investigation, details of the calibrations, data handling, and the science analysis are provided in accompanying articles. Solar Dynamics Observatory Helioseismology, observations Instrumentation and data management Magnetic fields, photosphere Scherrer, P. H. aut Bush, R. I. aut Wachter, R. aut Couvidat, S. aut Rabello-Soares, M. C. aut Bogart, R. S. aut Hoeksema, J. T. aut Liu, Y. aut Duvall, T. L. aut Akin, D. J. aut Allard, B. A. aut Miles, J. W. aut Rairden, R. aut Shine, R. A. aut Tarbell, T. D. aut Title, A. M. aut Wolfson, C. J. aut Elmore, D. F. aut Norton, A. A. aut Tomczyk, S. aut Enthalten in Solar physics Springer Netherlands, 1967 275(2011), 1-2 vom: 04. Okt., Seite 229-259 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:275 year:2011 number:1-2 day:04 month:10 pages:229-259 https://doi.org/10.1007/s11207-011-9842-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 275 2011 1-2 04 10 229-259
spelling	10.1007/s11207-011-9842-2 doi (DE-627)OLC2033610004 (DE-He213)s11207-011-9842-2-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Schou, J. verfasserin aut Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO) 2011 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2011 Abstract The Helioseismic and Magnetic Imager (HMI) investigation (Solar Phys. doi:10.1007/s11207-011-9834-2, 2011) will study the solar interior using helioseismic techniques as well as the magnetic field near the solar surface. The HMI instrument is part of the Solar Dynamics Observatory (SDO) that was launched on 11 February 2010. The instrument is designed to measure the Doppler shift, intensity, and vector magnetic field at the solar photosphere using the 6173 Å Fe i absorption line. The instrument consists of a front-window filter, a telescope, a set of waveplates for polarimetry, an image-stabilization system, a blocking filter, a five-stage Lyot filter with one tunable element, two wide-field tunable Michelson interferometers, a pair of $ 4096^{2} $ pixel cameras with independent shutters, and associated electronics. Each camera takes a full-disk image roughly every 3.75 seconds giving an overall cadence of 45 seconds for the Doppler, intensity, and line-of-sight magnetic-field measurements and a slower cadence for the full vector magnetic field. This article describes the design of the HMI instrument and provides an overview of the pre-launch calibration efforts. Overviews of the investigation, details of the calibrations, data handling, and the science analysis are provided in accompanying articles. Solar Dynamics Observatory Helioseismology, observations Instrumentation and data management Magnetic fields, photosphere Scherrer, P. H. aut Bush, R. I. aut Wachter, R. aut Couvidat, S. aut Rabello-Soares, M. C. aut Bogart, R. S. aut Hoeksema, J. T. aut Liu, Y. aut Duvall, T. L. aut Akin, D. J. aut Allard, B. A. aut Miles, J. W. aut Rairden, R. aut Shine, R. A. aut Tarbell, T. D. aut Title, A. M. aut Wolfson, C. J. aut Elmore, D. F. aut Norton, A. A. aut Tomczyk, S. aut Enthalten in Solar physics Springer Netherlands, 1967 275(2011), 1-2 vom: 04. Okt., Seite 229-259 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:275 year:2011 number:1-2 day:04 month:10 pages:229-259 https://doi.org/10.1007/s11207-011-9842-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 275 2011 1-2 04 10 229-259
allfields_unstemmed	10.1007/s11207-011-9842-2 doi (DE-627)OLC2033610004 (DE-He213)s11207-011-9842-2-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Schou, J. verfasserin aut Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO) 2011 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2011 Abstract The Helioseismic and Magnetic Imager (HMI) investigation (Solar Phys. doi:10.1007/s11207-011-9834-2, 2011) will study the solar interior using helioseismic techniques as well as the magnetic field near the solar surface. The HMI instrument is part of the Solar Dynamics Observatory (SDO) that was launched on 11 February 2010. The instrument is designed to measure the Doppler shift, intensity, and vector magnetic field at the solar photosphere using the 6173 Å Fe i absorption line. The instrument consists of a front-window filter, a telescope, a set of waveplates for polarimetry, an image-stabilization system, a blocking filter, a five-stage Lyot filter with one tunable element, two wide-field tunable Michelson interferometers, a pair of $ 4096^{2} $ pixel cameras with independent shutters, and associated electronics. Each camera takes a full-disk image roughly every 3.75 seconds giving an overall cadence of 45 seconds for the Doppler, intensity, and line-of-sight magnetic-field measurements and a slower cadence for the full vector magnetic field. This article describes the design of the HMI instrument and provides an overview of the pre-launch calibration efforts. Overviews of the investigation, details of the calibrations, data handling, and the science analysis are provided in accompanying articles. Solar Dynamics Observatory Helioseismology, observations Instrumentation and data management Magnetic fields, photosphere Scherrer, P. H. aut Bush, R. I. aut Wachter, R. aut Couvidat, S. aut Rabello-Soares, M. C. aut Bogart, R. S. aut Hoeksema, J. T. aut Liu, Y. aut Duvall, T. L. aut Akin, D. J. aut Allard, B. A. aut Miles, J. W. aut Rairden, R. aut Shine, R. A. aut Tarbell, T. D. aut Title, A. M. aut Wolfson, C. J. aut Elmore, D. F. aut Norton, A. A. aut Tomczyk, S. aut Enthalten in Solar physics Springer Netherlands, 1967 275(2011), 1-2 vom: 04. Okt., Seite 229-259 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:275 year:2011 number:1-2 day:04 month:10 pages:229-259 https://doi.org/10.1007/s11207-011-9842-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 275 2011 1-2 04 10 229-259
allfieldsGer	10.1007/s11207-011-9842-2 doi (DE-627)OLC2033610004 (DE-He213)s11207-011-9842-2-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Schou, J. verfasserin aut Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO) 2011 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2011 Abstract The Helioseismic and Magnetic Imager (HMI) investigation (Solar Phys. doi:10.1007/s11207-011-9834-2, 2011) will study the solar interior using helioseismic techniques as well as the magnetic field near the solar surface. The HMI instrument is part of the Solar Dynamics Observatory (SDO) that was launched on 11 February 2010. The instrument is designed to measure the Doppler shift, intensity, and vector magnetic field at the solar photosphere using the 6173 Å Fe i absorption line. The instrument consists of a front-window filter, a telescope, a set of waveplates for polarimetry, an image-stabilization system, a blocking filter, a five-stage Lyot filter with one tunable element, two wide-field tunable Michelson interferometers, a pair of $ 4096^{2} $ pixel cameras with independent shutters, and associated electronics. Each camera takes a full-disk image roughly every 3.75 seconds giving an overall cadence of 45 seconds for the Doppler, intensity, and line-of-sight magnetic-field measurements and a slower cadence for the full vector magnetic field. This article describes the design of the HMI instrument and provides an overview of the pre-launch calibration efforts. Overviews of the investigation, details of the calibrations, data handling, and the science analysis are provided in accompanying articles. Solar Dynamics Observatory Helioseismology, observations Instrumentation and data management Magnetic fields, photosphere Scherrer, P. H. aut Bush, R. I. aut Wachter, R. aut Couvidat, S. aut Rabello-Soares, M. C. aut Bogart, R. S. aut Hoeksema, J. T. aut Liu, Y. aut Duvall, T. L. aut Akin, D. J. aut Allard, B. A. aut Miles, J. W. aut Rairden, R. aut Shine, R. A. aut Tarbell, T. D. aut Title, A. M. aut Wolfson, C. J. aut Elmore, D. F. aut Norton, A. A. aut Tomczyk, S. aut Enthalten in Solar physics Springer Netherlands, 1967 275(2011), 1-2 vom: 04. Okt., Seite 229-259 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:275 year:2011 number:1-2 day:04 month:10 pages:229-259 https://doi.org/10.1007/s11207-011-9842-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 275 2011 1-2 04 10 229-259
allfieldsSound	10.1007/s11207-011-9842-2 doi (DE-627)OLC2033610004 (DE-He213)s11207-011-9842-2-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Schou, J. verfasserin aut Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO) 2011 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2011 Abstract The Helioseismic and Magnetic Imager (HMI) investigation (Solar Phys. doi:10.1007/s11207-011-9834-2, 2011) will study the solar interior using helioseismic techniques as well as the magnetic field near the solar surface. The HMI instrument is part of the Solar Dynamics Observatory (SDO) that was launched on 11 February 2010. The instrument is designed to measure the Doppler shift, intensity, and vector magnetic field at the solar photosphere using the 6173 Å Fe i absorption line. The instrument consists of a front-window filter, a telescope, a set of waveplates for polarimetry, an image-stabilization system, a blocking filter, a five-stage Lyot filter with one tunable element, two wide-field tunable Michelson interferometers, a pair of $ 4096^{2} $ pixel cameras with independent shutters, and associated electronics. Each camera takes a full-disk image roughly every 3.75 seconds giving an overall cadence of 45 seconds for the Doppler, intensity, and line-of-sight magnetic-field measurements and a slower cadence for the full vector magnetic field. This article describes the design of the HMI instrument and provides an overview of the pre-launch calibration efforts. Overviews of the investigation, details of the calibrations, data handling, and the science analysis are provided in accompanying articles. Solar Dynamics Observatory Helioseismology, observations Instrumentation and data management Magnetic fields, photosphere Scherrer, P. H. aut Bush, R. I. aut Wachter, R. aut Couvidat, S. aut Rabello-Soares, M. C. aut Bogart, R. S. aut Hoeksema, J. T. aut Liu, Y. aut Duvall, T. L. aut Akin, D. J. aut Allard, B. A. aut Miles, J. W. aut Rairden, R. aut Shine, R. A. aut Tarbell, T. D. aut Title, A. M. aut Wolfson, C. J. aut Elmore, D. F. aut Norton, A. A. aut Tomczyk, S. aut Enthalten in Solar physics Springer Netherlands, 1967 275(2011), 1-2 vom: 04. Okt., Seite 229-259 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:275 year:2011 number:1-2 day:04 month:10 pages:229-259 https://doi.org/10.1007/s11207-011-9842-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 275 2011 1-2 04 10 229-259
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topic_facet	Solar Dynamics Observatory Helioseismology, observations Instrumentation and data management Magnetic fields, photosphere
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authorswithroles_txt_mv	Schou, J. @@aut@@ Scherrer, P. H. @@aut@@ Bush, R. I. @@aut@@ Wachter, R. @@aut@@ Couvidat, S. @@aut@@ Rabello-Soares, M. C. @@aut@@ Bogart, R. S. @@aut@@ Hoeksema, J. T. @@aut@@ Liu, Y. @@aut@@ Duvall, T. L. @@aut@@ Akin, D. J. @@aut@@ Allard, B. A. @@aut@@ Miles, J. W. @@aut@@ Rairden, R. @@aut@@ Shine, R. A. @@aut@@ Tarbell, T. D. @@aut@@ Title, A. M. @@aut@@ Wolfson, C. J. @@aut@@ Elmore, D. F. @@aut@@ Norton, A. A. @@aut@@ Tomczyk, S. @@aut@@
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author	Schou, J.
spellingShingle	Schou, J. ddc 530 ssgn 16,12 misc Solar Dynamics Observatory misc Helioseismology, observations misc Instrumentation and data management misc Magnetic fields, photosphere Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO)
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topic_title	530 VZ 16,12 ssgn Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO) Solar Dynamics Observatory Helioseismology, observations Instrumentation and data management Magnetic fields, photosphere
topic	ddc 530 ssgn 16,12 misc Solar Dynamics Observatory misc Helioseismology, observations misc Instrumentation and data management misc Magnetic fields, photosphere
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title	Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO)
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title_full	Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO)
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author_browse	Schou, J. Scherrer, P. H. Bush, R. I. Wachter, R. Couvidat, S. Rabello-Soares, M. C. Bogart, R. S. Hoeksema, J. T. Liu, Y. Duvall, T. L. Akin, D. J. Allard, B. A. Miles, J. W. Rairden, R. Shine, R. A. Tarbell, T. D. Title, A. M. Wolfson, C. J. Elmore, D. F. Norton, A. A. Tomczyk, S.
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title_sort	design and ground calibration of the helioseismic and magnetic imager (hmi) instrument on the solar dynamics observatory (sdo)
title_auth	Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO)
abstract	Abstract The Helioseismic and Magnetic Imager (HMI) investigation (Solar Phys. doi:10.1007/s11207-011-9834-2, 2011) will study the solar interior using helioseismic techniques as well as the magnetic field near the solar surface. The HMI instrument is part of the Solar Dynamics Observatory (SDO) that was launched on 11 February 2010. The instrument is designed to measure the Doppler shift, intensity, and vector magnetic field at the solar photosphere using the 6173 Å Fe i absorption line. The instrument consists of a front-window filter, a telescope, a set of waveplates for polarimetry, an image-stabilization system, a blocking filter, a five-stage Lyot filter with one tunable element, two wide-field tunable Michelson interferometers, a pair of $ 4096^{2} $ pixel cameras with independent shutters, and associated electronics. Each camera takes a full-disk image roughly every 3.75 seconds giving an overall cadence of 45 seconds for the Doppler, intensity, and line-of-sight magnetic-field measurements and a slower cadence for the full vector magnetic field. This article describes the design of the HMI instrument and provides an overview of the pre-launch calibration efforts. Overviews of the investigation, details of the calibrations, data handling, and the science analysis are provided in accompanying articles. © The Author(s) 2011
abstractGer	Abstract The Helioseismic and Magnetic Imager (HMI) investigation (Solar Phys. doi:10.1007/s11207-011-9834-2, 2011) will study the solar interior using helioseismic techniques as well as the magnetic field near the solar surface. The HMI instrument is part of the Solar Dynamics Observatory (SDO) that was launched on 11 February 2010. The instrument is designed to measure the Doppler shift, intensity, and vector magnetic field at the solar photosphere using the 6173 Å Fe i absorption line. The instrument consists of a front-window filter, a telescope, a set of waveplates for polarimetry, an image-stabilization system, a blocking filter, a five-stage Lyot filter with one tunable element, two wide-field tunable Michelson interferometers, a pair of $ 4096^{2} $ pixel cameras with independent shutters, and associated electronics. Each camera takes a full-disk image roughly every 3.75 seconds giving an overall cadence of 45 seconds for the Doppler, intensity, and line-of-sight magnetic-field measurements and a slower cadence for the full vector magnetic field. This article describes the design of the HMI instrument and provides an overview of the pre-launch calibration efforts. Overviews of the investigation, details of the calibrations, data handling, and the science analysis are provided in accompanying articles. © The Author(s) 2011
abstract_unstemmed	Abstract The Helioseismic and Magnetic Imager (HMI) investigation (Solar Phys. doi:10.1007/s11207-011-9834-2, 2011) will study the solar interior using helioseismic techniques as well as the magnetic field near the solar surface. The HMI instrument is part of the Solar Dynamics Observatory (SDO) that was launched on 11 February 2010. The instrument is designed to measure the Doppler shift, intensity, and vector magnetic field at the solar photosphere using the 6173 Å Fe i absorption line. The instrument consists of a front-window filter, a telescope, a set of waveplates for polarimetry, an image-stabilization system, a blocking filter, a five-stage Lyot filter with one tunable element, two wide-field tunable Michelson interferometers, a pair of $ 4096^{2} $ pixel cameras with independent shutters, and associated electronics. Each camera takes a full-disk image roughly every 3.75 seconds giving an overall cadence of 45 seconds for the Doppler, intensity, and line-of-sight magnetic-field measurements and a slower cadence for the full vector magnetic field. This article describes the design of the HMI instrument and provides an overview of the pre-launch calibration efforts. Overviews of the investigation, details of the calibrations, data handling, and the science analysis are provided in accompanying articles. © The Author(s) 2011
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title_short	Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO)
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author2	Scherrer, P. H. Bush, R. I. Wachter, R. Couvidat, S. Rabello-Soares, M. C. Bogart, R. S. Hoeksema, J. T. Liu, Y. Duvall, T. L. Akin, D. J. Allard, B. A. Miles, J. W. Rairden, R. Shine, R. A. Tarbell, T. D. Title, A. M. Wolfson, C. J. Elmore, D. F. Norton, A. A. Tomczyk, S.
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