UV Observations with the Transition Region and Coronal Explorer
Abstract The Transition Region and Coronal Explorer is a space-borne solar telescope featuring high spatial and temporal resolution. TRACE images emission from solar plasmas in three extreme-ultraviolet (EUV) wavelengths and several ultraviolet (UV) wavelengths, covering selected ion temperatures fr...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Handy, B.N. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1998 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1998 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 183(1998), 1 vom: Nov., Seite 29-43 |
|---|---|
| Übergeordnetes Werk: |
volume:183 ; year:1998 ; number:1 ; month:11 ; pages:29-43 |
| Links: |
|---|
| DOI / URN: |
10.1023/A:1005079622620 |
|---|
| Katalog-ID: |
OLC2033586197 |
|---|
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| 245 | 1 | 0 | |a UV Observations with the Transition Region and Coronal Explorer |
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| 520 | |a Abstract The Transition Region and Coronal Explorer is a space-borne solar telescope featuring high spatial and temporal resolution. TRACE images emission from solar plasmas in three extreme-ultraviolet (EUV) wavelengths and several ultraviolet (UV) wavelengths, covering selected ion temperatures from 6000 K to 1 MK. The TRACE UV channel employs special optics to collect high-resolution solar images of the H i Lα line at 1216 Å, the C iv resonance doublet at 1548 and 1550 Å, the UV continuum near 1550 Å, and also a white-light image covering the spectrum from 2000–8000 Å. We present an analytical technique for creating photometrically accurate images of the C iv resonance lines from the data products collected by the TRACE UV channel. We use solar spectra from several space-borne instruments to represent a variety of solar conditions ranging from quiet Sun to active regions to derive a method, using a linear combination of filtered UV images, to generate an image of solar C iv 1550 Å emission. Systematic and statistical error estimates are also presented. This work indicates that C iv measurements will be reliable for intensities greater than 1014 photons s−1 cm−2 sr−1. This suggests that C iv 1550 Å images will be feasible with statistical error below 20% in the magnetic network, bright points, active regions, flares and other features bright in C iv. Below this intensity the derived image is dominated by systematic error and read noise from the CCD. | ||
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| 650 | 4 | |a Temporal Resolution | |
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| 700 | 1 | |a Title, A.M. |4 aut | |
| 700 | 1 | |a Wolfson, C.J. |4 aut | |
| 700 | 1 | |a Laforge, M.J. |4 aut | |
| 700 | 1 | |a Oliver, J.J. |4 aut | |
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10.1023/A:1005079622620 doi (DE-627)OLC2033586197 (DE-He213)A:1005079622620-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Handy, B.N. verfasserin aut UV Observations with the Transition Region and Coronal Explorer 1998 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1998 Abstract The Transition Region and Coronal Explorer is a space-borne solar telescope featuring high spatial and temporal resolution. TRACE images emission from solar plasmas in three extreme-ultraviolet (EUV) wavelengths and several ultraviolet (UV) wavelengths, covering selected ion temperatures from 6000 K to 1 MK. The TRACE UV channel employs special optics to collect high-resolution solar images of the H i Lα line at 1216 Å, the C iv resonance doublet at 1548 and 1550 Å, the UV continuum near 1550 Å, and also a white-light image covering the spectrum from 2000–8000 Å. We present an analytical technique for creating photometrically accurate images of the C iv resonance lines from the data products collected by the TRACE UV channel. We use solar spectra from several space-borne instruments to represent a variety of solar conditions ranging from quiet Sun to active regions to derive a method, using a linear combination of filtered UV images, to generate an image of solar C iv 1550 Å emission. Systematic and statistical error estimates are also presented. This work indicates that C iv measurements will be reliable for intensities greater than 1014 photons s−1 cm−2 sr−1. This suggests that C iv 1550 Å images will be feasible with statistical error below 20% in the magnetic network, bright points, active regions, flares and other features bright in C iv. Below this intensity the derived image is dominated by systematic error and read noise from the CCD. Flare Temporal Resolution Bright Point Solar Image Solar Condition Bruner, M.E. aut Tarbell, T.D. aut Title, A.M. aut Wolfson, C.J. aut Laforge, M.J. aut Oliver, J.J. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 183(1998), 1 vom: Nov., Seite 29-43 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:183 year:1998 number:1 month:11 pages:29-43 https://doi.org/10.1023/A:1005079622620 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 183 1998 1 11 29-43 |
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10.1023/A:1005079622620 doi (DE-627)OLC2033586197 (DE-He213)A:1005079622620-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Handy, B.N. verfasserin aut UV Observations with the Transition Region and Coronal Explorer 1998 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1998 Abstract The Transition Region and Coronal Explorer is a space-borne solar telescope featuring high spatial and temporal resolution. TRACE images emission from solar plasmas in three extreme-ultraviolet (EUV) wavelengths and several ultraviolet (UV) wavelengths, covering selected ion temperatures from 6000 K to 1 MK. The TRACE UV channel employs special optics to collect high-resolution solar images of the H i Lα line at 1216 Å, the C iv resonance doublet at 1548 and 1550 Å, the UV continuum near 1550 Å, and also a white-light image covering the spectrum from 2000–8000 Å. We present an analytical technique for creating photometrically accurate images of the C iv resonance lines from the data products collected by the TRACE UV channel. We use solar spectra from several space-borne instruments to represent a variety of solar conditions ranging from quiet Sun to active regions to derive a method, using a linear combination of filtered UV images, to generate an image of solar C iv 1550 Å emission. Systematic and statistical error estimates are also presented. This work indicates that C iv measurements will be reliable for intensities greater than 1014 photons s−1 cm−2 sr−1. This suggests that C iv 1550 Å images will be feasible with statistical error below 20% in the magnetic network, bright points, active regions, flares and other features bright in C iv. Below this intensity the derived image is dominated by systematic error and read noise from the CCD. Flare Temporal Resolution Bright Point Solar Image Solar Condition Bruner, M.E. aut Tarbell, T.D. aut Title, A.M. aut Wolfson, C.J. aut Laforge, M.J. aut Oliver, J.J. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 183(1998), 1 vom: Nov., Seite 29-43 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:183 year:1998 number:1 month:11 pages:29-43 https://doi.org/10.1023/A:1005079622620 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 183 1998 1 11 29-43 |
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10.1023/A:1005079622620 doi (DE-627)OLC2033586197 (DE-He213)A:1005079622620-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Handy, B.N. verfasserin aut UV Observations with the Transition Region and Coronal Explorer 1998 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1998 Abstract The Transition Region and Coronal Explorer is a space-borne solar telescope featuring high spatial and temporal resolution. TRACE images emission from solar plasmas in three extreme-ultraviolet (EUV) wavelengths and several ultraviolet (UV) wavelengths, covering selected ion temperatures from 6000 K to 1 MK. The TRACE UV channel employs special optics to collect high-resolution solar images of the H i Lα line at 1216 Å, the C iv resonance doublet at 1548 and 1550 Å, the UV continuum near 1550 Å, and also a white-light image covering the spectrum from 2000–8000 Å. We present an analytical technique for creating photometrically accurate images of the C iv resonance lines from the data products collected by the TRACE UV channel. We use solar spectra from several space-borne instruments to represent a variety of solar conditions ranging from quiet Sun to active regions to derive a method, using a linear combination of filtered UV images, to generate an image of solar C iv 1550 Å emission. Systematic and statistical error estimates are also presented. This work indicates that C iv measurements will be reliable for intensities greater than 1014 photons s−1 cm−2 sr−1. This suggests that C iv 1550 Å images will be feasible with statistical error below 20% in the magnetic network, bright points, active regions, flares and other features bright in C iv. Below this intensity the derived image is dominated by systematic error and read noise from the CCD. Flare Temporal Resolution Bright Point Solar Image Solar Condition Bruner, M.E. aut Tarbell, T.D. aut Title, A.M. aut Wolfson, C.J. aut Laforge, M.J. aut Oliver, J.J. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 183(1998), 1 vom: Nov., Seite 29-43 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:183 year:1998 number:1 month:11 pages:29-43 https://doi.org/10.1023/A:1005079622620 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 183 1998 1 11 29-43 |
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10.1023/A:1005079622620 doi (DE-627)OLC2033586197 (DE-He213)A:1005079622620-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Handy, B.N. verfasserin aut UV Observations with the Transition Region and Coronal Explorer 1998 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1998 Abstract The Transition Region and Coronal Explorer is a space-borne solar telescope featuring high spatial and temporal resolution. TRACE images emission from solar plasmas in three extreme-ultraviolet (EUV) wavelengths and several ultraviolet (UV) wavelengths, covering selected ion temperatures from 6000 K to 1 MK. The TRACE UV channel employs special optics to collect high-resolution solar images of the H i Lα line at 1216 Å, the C iv resonance doublet at 1548 and 1550 Å, the UV continuum near 1550 Å, and also a white-light image covering the spectrum from 2000–8000 Å. We present an analytical technique for creating photometrically accurate images of the C iv resonance lines from the data products collected by the TRACE UV channel. We use solar spectra from several space-borne instruments to represent a variety of solar conditions ranging from quiet Sun to active regions to derive a method, using a linear combination of filtered UV images, to generate an image of solar C iv 1550 Å emission. Systematic and statistical error estimates are also presented. This work indicates that C iv measurements will be reliable for intensities greater than 1014 photons s−1 cm−2 sr−1. This suggests that C iv 1550 Å images will be feasible with statistical error below 20% in the magnetic network, bright points, active regions, flares and other features bright in C iv. Below this intensity the derived image is dominated by systematic error and read noise from the CCD. Flare Temporal Resolution Bright Point Solar Image Solar Condition Bruner, M.E. aut Tarbell, T.D. aut Title, A.M. aut Wolfson, C.J. aut Laforge, M.J. aut Oliver, J.J. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 183(1998), 1 vom: Nov., Seite 29-43 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:183 year:1998 number:1 month:11 pages:29-43 https://doi.org/10.1023/A:1005079622620 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 183 1998 1 11 29-43 |
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10.1023/A:1005079622620 doi (DE-627)OLC2033586197 (DE-He213)A:1005079622620-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Handy, B.N. verfasserin aut UV Observations with the Transition Region and Coronal Explorer 1998 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1998 Abstract The Transition Region and Coronal Explorer is a space-borne solar telescope featuring high spatial and temporal resolution. TRACE images emission from solar plasmas in three extreme-ultraviolet (EUV) wavelengths and several ultraviolet (UV) wavelengths, covering selected ion temperatures from 6000 K to 1 MK. The TRACE UV channel employs special optics to collect high-resolution solar images of the H i Lα line at 1216 Å, the C iv resonance doublet at 1548 and 1550 Å, the UV continuum near 1550 Å, and also a white-light image covering the spectrum from 2000–8000 Å. We present an analytical technique for creating photometrically accurate images of the C iv resonance lines from the data products collected by the TRACE UV channel. We use solar spectra from several space-borne instruments to represent a variety of solar conditions ranging from quiet Sun to active regions to derive a method, using a linear combination of filtered UV images, to generate an image of solar C iv 1550 Å emission. Systematic and statistical error estimates are also presented. This work indicates that C iv measurements will be reliable for intensities greater than 1014 photons s−1 cm−2 sr−1. This suggests that C iv 1550 Å images will be feasible with statistical error below 20% in the magnetic network, bright points, active regions, flares and other features bright in C iv. Below this intensity the derived image is dominated by systematic error and read noise from the CCD. Flare Temporal Resolution Bright Point Solar Image Solar Condition Bruner, M.E. aut Tarbell, T.D. aut Title, A.M. aut Wolfson, C.J. aut Laforge, M.J. aut Oliver, J.J. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 183(1998), 1 vom: Nov., Seite 29-43 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:183 year:1998 number:1 month:11 pages:29-43 https://doi.org/10.1023/A:1005079622620 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 183 1998 1 11 29-43 |
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Handy, B.N. |
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530 VZ 16,12 ssgn UV Observations with the Transition Region and Coronal Explorer Flare Temporal Resolution Bright Point Solar Image Solar Condition |
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UV Observations with the Transition Region and Coronal Explorer |
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UV Observations with the Transition Region and Coronal Explorer |
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Handy, B.N. |
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Solar physics |
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1998 |
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Handy, B.N. Bruner, M.E. Tarbell, T.D. Title, A.M. Wolfson, C.J. Laforge, M.J. Oliver, J.J. |
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uv observations with the transition region and coronal explorer |
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UV Observations with the Transition Region and Coronal Explorer |
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Abstract The Transition Region and Coronal Explorer is a space-borne solar telescope featuring high spatial and temporal resolution. TRACE images emission from solar plasmas in three extreme-ultraviolet (EUV) wavelengths and several ultraviolet (UV) wavelengths, covering selected ion temperatures from 6000 K to 1 MK. The TRACE UV channel employs special optics to collect high-resolution solar images of the H i Lα line at 1216 Å, the C iv resonance doublet at 1548 and 1550 Å, the UV continuum near 1550 Å, and also a white-light image covering the spectrum from 2000–8000 Å. We present an analytical technique for creating photometrically accurate images of the C iv resonance lines from the data products collected by the TRACE UV channel. We use solar spectra from several space-borne instruments to represent a variety of solar conditions ranging from quiet Sun to active regions to derive a method, using a linear combination of filtered UV images, to generate an image of solar C iv 1550 Å emission. Systematic and statistical error estimates are also presented. This work indicates that C iv measurements will be reliable for intensities greater than 1014 photons s−1 cm−2 sr−1. This suggests that C iv 1550 Å images will be feasible with statistical error below 20% in the magnetic network, bright points, active regions, flares and other features bright in C iv. Below this intensity the derived image is dominated by systematic error and read noise from the CCD. © Kluwer Academic Publishers 1998 |
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Abstract The Transition Region and Coronal Explorer is a space-borne solar telescope featuring high spatial and temporal resolution. TRACE images emission from solar plasmas in three extreme-ultraviolet (EUV) wavelengths and several ultraviolet (UV) wavelengths, covering selected ion temperatures from 6000 K to 1 MK. The TRACE UV channel employs special optics to collect high-resolution solar images of the H i Lα line at 1216 Å, the C iv resonance doublet at 1548 and 1550 Å, the UV continuum near 1550 Å, and also a white-light image covering the spectrum from 2000–8000 Å. We present an analytical technique for creating photometrically accurate images of the C iv resonance lines from the data products collected by the TRACE UV channel. We use solar spectra from several space-borne instruments to represent a variety of solar conditions ranging from quiet Sun to active regions to derive a method, using a linear combination of filtered UV images, to generate an image of solar C iv 1550 Å emission. Systematic and statistical error estimates are also presented. This work indicates that C iv measurements will be reliable for intensities greater than 1014 photons s−1 cm−2 sr−1. This suggests that C iv 1550 Å images will be feasible with statistical error below 20% in the magnetic network, bright points, active regions, flares and other features bright in C iv. Below this intensity the derived image is dominated by systematic error and read noise from the CCD. © Kluwer Academic Publishers 1998 |
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Abstract The Transition Region and Coronal Explorer is a space-borne solar telescope featuring high spatial and temporal resolution. TRACE images emission from solar plasmas in three extreme-ultraviolet (EUV) wavelengths and several ultraviolet (UV) wavelengths, covering selected ion temperatures from 6000 K to 1 MK. The TRACE UV channel employs special optics to collect high-resolution solar images of the H i Lα line at 1216 Å, the C iv resonance doublet at 1548 and 1550 Å, the UV continuum near 1550 Å, and also a white-light image covering the spectrum from 2000–8000 Å. We present an analytical technique for creating photometrically accurate images of the C iv resonance lines from the data products collected by the TRACE UV channel. We use solar spectra from several space-borne instruments to represent a variety of solar conditions ranging from quiet Sun to active regions to derive a method, using a linear combination of filtered UV images, to generate an image of solar C iv 1550 Å emission. Systematic and statistical error estimates are also presented. This work indicates that C iv measurements will be reliable for intensities greater than 1014 photons s−1 cm−2 sr−1. This suggests that C iv 1550 Å images will be feasible with statistical error below 20% in the magnetic network, bright points, active regions, flares and other features bright in C iv. Below this intensity the derived image is dominated by systematic error and read noise from the CCD. © Kluwer Academic Publishers 1998 |
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UV Observations with the Transition Region and Coronal Explorer |
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