Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field
Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Penn, M.J. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2004 |
|---|
| Schlagwörter: |
|---|
| Anmerkung: |
© Kluwer Academic Publishers 2004 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 222(2004), 1 vom: Juli, Seite 61-78 |
|---|---|
| Übergeordnetes Werk: |
volume:222 ; year:2004 ; number:1 ; month:07 ; pages:61-78 |
| Links: |
|---|
| DOI / URN: |
10.1023/B:SOLA.0000036850.34404.5f |
|---|
| Katalog-ID: |
OLC2033597008 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | OLC2033597008 | ||
| 003 | DE-627 | ||
| 005 | 20230504045723.0 | ||
| 007 | tu | ||
| 008 | 200819s2004 xx ||||| 00| ||eng c | ||
| 024 | 7 | |a 10.1023/B:SOLA.0000036850.34404.5f |2 doi | |
| 035 | |a (DE-627)OLC2033597008 | ||
| 035 | |a (DE-He213)B:SOLA.0000036850.34404.5f-p | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 082 | 0 | 4 | |a 530 |q VZ |
| 084 | |a 16,12 |2 ssgn | ||
| 100 | 1 | |a Penn, M.J. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field |
| 264 | 1 | |c 2004 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a ohne Hilfsmittel zu benutzen |b n |2 rdamedia | ||
| 338 | |a Band |b nc |2 rdacarrier | ||
| 500 | |a © Kluwer Academic Publishers 2004 | ||
| 520 | |a Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal integration time are introduced. Specific expressions are developed for the 1σ measurement errors for coronal intensity, coronal electron density, coronal velocity, and coronal magnetic field measurements using emission lines and including a background. | ||
| 650 | 4 | |a Measurement Error | |
| 650 | 4 | |a Integration Time | |
| 650 | 4 | |a Field Measurement | |
| 650 | 4 | |a Emission Line | |
| 650 | 4 | |a Background Signal | |
| 700 | 1 | |a Lin, H. |4 aut | |
| 700 | 1 | |a Tomczyk, S. |4 aut | |
| 700 | 1 | |a Elmore, D. |4 aut | |
| 700 | 1 | |a Judge, P. |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Solar physics |d Kluwer Academic Publishers, 1967 |g 222(2004), 1 vom: Juli, Seite 61-78 |w (DE-627)129856010 |w (DE-600)281593-X |w (DE-576)015160033 |x 0038-0938 |7 nnns |
| 773 | 1 | 8 | |g volume:222 |g year:2004 |g number:1 |g month:07 |g pages:61-78 |
| 856 | 4 | 1 | |u https://doi.org/10.1023/B:SOLA.0000036850.34404.5f |z lizenzpflichtig |3 Volltext |
| 912 | |a GBV_USEFLAG_A | ||
| 912 | |a SYSFLAG_A | ||
| 912 | |a GBV_OLC | ||
| 912 | |a SSG-OLC-PHY | ||
| 912 | |a SSG-OLC-AST | ||
| 912 | |a SSG-OPC-AST | ||
| 912 | |a GBV_ILN_11 | ||
| 912 | |a GBV_ILN_24 | ||
| 912 | |a GBV_ILN_40 | ||
| 912 | |a GBV_ILN_47 | ||
| 912 | |a GBV_ILN_70 | ||
| 951 | |a AR | ||
| 952 | |d 222 |j 2004 |e 1 |c 07 |h 61-78 | ||
| author_variant |
m p mp h l hl s t st d e de p j pj |
|---|---|
| matchkey_str |
article:00380938:2004----::akrudnuemaueetrosfhcrnlnestdniy |
| hierarchy_sort_str |
2004 |
| publishDate |
2004 |
| allfields |
10.1023/B:SOLA.0000036850.34404.5f doi (DE-627)OLC2033597008 (DE-He213)B:SOLA.0000036850.34404.5f-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Penn, M.J. verfasserin aut Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field 2004 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2004 Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal integration time are introduced. Specific expressions are developed for the 1σ measurement errors for coronal intensity, coronal electron density, coronal velocity, and coronal magnetic field measurements using emission lines and including a background. Measurement Error Integration Time Field Measurement Emission Line Background Signal Lin, H. aut Tomczyk, S. aut Elmore, D. aut Judge, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 222(2004), 1 vom: Juli, Seite 61-78 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:222 year:2004 number:1 month:07 pages:61-78 https://doi.org/10.1023/B:SOLA.0000036850.34404.5f lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 222 2004 1 07 61-78 |
| spelling |
10.1023/B:SOLA.0000036850.34404.5f doi (DE-627)OLC2033597008 (DE-He213)B:SOLA.0000036850.34404.5f-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Penn, M.J. verfasserin aut Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field 2004 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2004 Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal integration time are introduced. Specific expressions are developed for the 1σ measurement errors for coronal intensity, coronal electron density, coronal velocity, and coronal magnetic field measurements using emission lines and including a background. Measurement Error Integration Time Field Measurement Emission Line Background Signal Lin, H. aut Tomczyk, S. aut Elmore, D. aut Judge, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 222(2004), 1 vom: Juli, Seite 61-78 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:222 year:2004 number:1 month:07 pages:61-78 https://doi.org/10.1023/B:SOLA.0000036850.34404.5f lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 222 2004 1 07 61-78 |
| allfields_unstemmed |
10.1023/B:SOLA.0000036850.34404.5f doi (DE-627)OLC2033597008 (DE-He213)B:SOLA.0000036850.34404.5f-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Penn, M.J. verfasserin aut Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field 2004 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2004 Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal integration time are introduced. Specific expressions are developed for the 1σ measurement errors for coronal intensity, coronal electron density, coronal velocity, and coronal magnetic field measurements using emission lines and including a background. Measurement Error Integration Time Field Measurement Emission Line Background Signal Lin, H. aut Tomczyk, S. aut Elmore, D. aut Judge, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 222(2004), 1 vom: Juli, Seite 61-78 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:222 year:2004 number:1 month:07 pages:61-78 https://doi.org/10.1023/B:SOLA.0000036850.34404.5f lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 222 2004 1 07 61-78 |
| allfieldsGer |
10.1023/B:SOLA.0000036850.34404.5f doi (DE-627)OLC2033597008 (DE-He213)B:SOLA.0000036850.34404.5f-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Penn, M.J. verfasserin aut Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field 2004 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2004 Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal integration time are introduced. Specific expressions are developed for the 1σ measurement errors for coronal intensity, coronal electron density, coronal velocity, and coronal magnetic field measurements using emission lines and including a background. Measurement Error Integration Time Field Measurement Emission Line Background Signal Lin, H. aut Tomczyk, S. aut Elmore, D. aut Judge, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 222(2004), 1 vom: Juli, Seite 61-78 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:222 year:2004 number:1 month:07 pages:61-78 https://doi.org/10.1023/B:SOLA.0000036850.34404.5f lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 222 2004 1 07 61-78 |
| allfieldsSound |
10.1023/B:SOLA.0000036850.34404.5f doi (DE-627)OLC2033597008 (DE-He213)B:SOLA.0000036850.34404.5f-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Penn, M.J. verfasserin aut Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field 2004 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2004 Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal integration time are introduced. Specific expressions are developed for the 1σ measurement errors for coronal intensity, coronal electron density, coronal velocity, and coronal magnetic field measurements using emission lines and including a background. Measurement Error Integration Time Field Measurement Emission Line Background Signal Lin, H. aut Tomczyk, S. aut Elmore, D. aut Judge, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 222(2004), 1 vom: Juli, Seite 61-78 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:222 year:2004 number:1 month:07 pages:61-78 https://doi.org/10.1023/B:SOLA.0000036850.34404.5f lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 222 2004 1 07 61-78 |
| language |
English |
| source |
Enthalten in Solar physics 222(2004), 1 vom: Juli, Seite 61-78 volume:222 year:2004 number:1 month:07 pages:61-78 |
| sourceStr |
Enthalten in Solar physics 222(2004), 1 vom: Juli, Seite 61-78 volume:222 year:2004 number:1 month:07 pages:61-78 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| topic_facet |
Measurement Error Integration Time Field Measurement Emission Line Background Signal |
| dewey-raw |
530 |
| isfreeaccess_bool |
false |
| container_title |
Solar physics |
| authorswithroles_txt_mv |
Penn, M.J. @@aut@@ Lin, H. @@aut@@ Tomczyk, S. @@aut@@ Elmore, D. @@aut@@ Judge, P. @@aut@@ |
| publishDateDaySort_date |
2004-07-01T00:00:00Z |
| hierarchy_top_id |
129856010 |
| dewey-sort |
3530 |
| id |
OLC2033597008 |
| language_de |
englisch |
| fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2033597008</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504045723.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2004 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1023/B:SOLA.0000036850.34404.5f</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2033597008</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)B:SOLA.0000036850.34404.5f-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Penn, M.J.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2004</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Kluwer Academic Publishers 2004</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal integration time are introduced. Specific expressions are developed for the 1σ measurement errors for coronal intensity, coronal electron density, coronal velocity, and coronal magnetic field measurements using emission lines and including a background.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Measurement Error</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Integration Time</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Field Measurement</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Emission Line</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Background Signal</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lin, H.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tomczyk, S.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Elmore, D.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Judge, P.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Solar physics</subfield><subfield code="d">Kluwer Academic Publishers, 1967</subfield><subfield code="g">222(2004), 1 vom: Juli, Seite 61-78</subfield><subfield code="w">(DE-627)129856010</subfield><subfield code="w">(DE-600)281593-X</subfield><subfield code="w">(DE-576)015160033</subfield><subfield code="x">0038-0938</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:222</subfield><subfield code="g">year:2004</subfield><subfield code="g">number:1</subfield><subfield code="g">month:07</subfield><subfield code="g">pages:61-78</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1023/B:SOLA.0000036850.34404.5f</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">222</subfield><subfield code="j">2004</subfield><subfield code="e">1</subfield><subfield code="c">07</subfield><subfield code="h">61-78</subfield></datafield></record></collection>
|
| author |
Penn, M.J. |
| spellingShingle |
Penn, M.J. ddc 530 ssgn 16,12 misc Measurement Error misc Integration Time misc Field Measurement misc Emission Line misc Background Signal Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field |
| authorStr |
Penn, M.J. |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)129856010 |
| format |
Article |
| dewey-ones |
530 - Physics |
| delete_txt_mv |
keep |
| author_role |
aut aut aut aut aut |
| collection |
OLC |
| remote_str |
false |
| illustrated |
Not Illustrated |
| issn |
0038-0938 |
| topic_title |
530 VZ 16,12 ssgn Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field Measurement Error Integration Time Field Measurement Emission Line Background Signal |
| topic |
ddc 530 ssgn 16,12 misc Measurement Error misc Integration Time misc Field Measurement misc Emission Line misc Background Signal |
| topic_unstemmed |
ddc 530 ssgn 16,12 misc Measurement Error misc Integration Time misc Field Measurement misc Emission Line misc Background Signal |
| topic_browse |
ddc 530 ssgn 16,12 misc Measurement Error misc Integration Time misc Field Measurement misc Emission Line misc Background Signal |
| format_facet |
Aufsätze Gedruckte Aufsätze |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
nc |
| hierarchy_parent_title |
Solar physics |
| hierarchy_parent_id |
129856010 |
| dewey-tens |
530 - Physics |
| hierarchy_top_title |
Solar physics |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)129856010 (DE-600)281593-X (DE-576)015160033 |
| title |
Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field |
| ctrlnum |
(DE-627)OLC2033597008 (DE-He213)B:SOLA.0000036850.34404.5f-p |
| title_full |
Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field |
| author_sort |
Penn, M.J. |
| journal |
Solar physics |
| journalStr |
Solar physics |
| lang_code |
eng |
| isOA_bool |
false |
| dewey-hundreds |
500 - Science |
| recordtype |
marc |
| publishDateSort |
2004 |
| contenttype_str_mv |
txt |
| container_start_page |
61 |
| author_browse |
Penn, M.J. Lin, H. Tomczyk, S. Elmore, D. Judge, P. |
| container_volume |
222 |
| class |
530 VZ 16,12 ssgn |
| format_se |
Aufsätze |
| author-letter |
Penn, M.J. |
| doi_str_mv |
10.1023/B:SOLA.0000036850.34404.5f |
| dewey-full |
530 |
| title_sort |
background-induced measurement errors of the coronal intensity, density, velocity, and magnetic field |
| title_auth |
Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field |
| abstract |
Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal integration time are introduced. Specific expressions are developed for the 1σ measurement errors for coronal intensity, coronal electron density, coronal velocity, and coronal magnetic field measurements using emission lines and including a background. © Kluwer Academic Publishers 2004 |
| abstractGer |
Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal integration time are introduced. Specific expressions are developed for the 1σ measurement errors for coronal intensity, coronal electron density, coronal velocity, and coronal magnetic field measurements using emission lines and including a background. © Kluwer Academic Publishers 2004 |
| abstract_unstemmed |
Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal integration time are introduced. Specific expressions are developed for the 1σ measurement errors for coronal intensity, coronal electron density, coronal velocity, and coronal magnetic field measurements using emission lines and including a background. © Kluwer Academic Publishers 2004 |
| collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 |
| container_issue |
1 |
| title_short |
Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field |
| url |
https://doi.org/10.1023/B:SOLA.0000036850.34404.5f |
| remote_bool |
false |
| author2 |
Lin, H. Tomczyk, S. Elmore, D. Judge, P. |
| author2Str |
Lin, H. Tomczyk, S. Elmore, D. Judge, P. |
| ppnlink |
129856010 |
| mediatype_str_mv |
n |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1023/B:SOLA.0000036850.34404.5f |
| up_date |
2024-07-03T17:37:36.672Z |
| _version_ |
1803580349267050496 |
| fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2033597008</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504045723.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2004 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1023/B:SOLA.0000036850.34404.5f</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2033597008</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)B:SOLA.0000036850.34404.5f-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Penn, M.J.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2004</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Kluwer Academic Publishers 2004</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The effect of a background signal on the signal-to-noise ratio is discussed, with particular application to ground-based observations of emission lines in the solar corona with the proposed Advanced Technology Solar Telescope. The concepts of effective coronal aperture and effective coronal integration time are introduced. Specific expressions are developed for the 1σ measurement errors for coronal intensity, coronal electron density, coronal velocity, and coronal magnetic field measurements using emission lines and including a background.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Measurement Error</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Integration Time</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Field Measurement</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Emission Line</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Background Signal</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lin, H.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tomczyk, S.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Elmore, D.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Judge, P.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Solar physics</subfield><subfield code="d">Kluwer Academic Publishers, 1967</subfield><subfield code="g">222(2004), 1 vom: Juli, Seite 61-78</subfield><subfield code="w">(DE-627)129856010</subfield><subfield code="w">(DE-600)281593-X</subfield><subfield code="w">(DE-576)015160033</subfield><subfield code="x">0038-0938</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:222</subfield><subfield code="g">year:2004</subfield><subfield code="g">number:1</subfield><subfield code="g">month:07</subfield><subfield code="g">pages:61-78</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1023/B:SOLA.0000036850.34404.5f</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_24</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">222</subfield><subfield code="j">2004</subfield><subfield code="e">1</subfield><subfield code="c">07</subfield><subfield code="h">61-78</subfield></datafield></record></collection>
|
| score |
7.401744 |