Trace — The transition region and coronal explorer
Abstract TRACE is a single-instrument solar mission that will be put into a Sunsynchronous polar orbit and will obtain continuous solar observations for about 8 months per year. It will collect images of solar plasmas at temperatures from $ 10^{4} $ to $ 10^{7} $ K, with 1-arcsec spatial resolution...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Strong, K. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1994 |
|---|
| Anmerkung: |
© Kluwer Academic Publishers 1994 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Kluwer Academic Publishers, 1962, 70(1994), 1-2 vom: Okt., Seite 119-122 |
|---|---|
| Übergeordnetes Werk: |
volume:70 ; year:1994 ; number:1-2 ; month:10 ; pages:119-122 |
| Links: |
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| DOI / URN: |
10.1007/BF00777855 |
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OLC2033675904 |
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| 520 | |a Abstract TRACE is a single-instrument solar mission that will be put into a Sunsynchronous polar orbit and will obtain continuous solar observations for about 8 months per year. It will collect images of solar plasmas at temperatures from $ 10^{4} $ to $ 10^{7} $ K, with 1-arcsec spatial resolution and excellent temporal resolution and continuity. With such data, we expect to gain a new understanding of many solar and stellar problems ranging from coronal heating to impulsive magnetohydrodynamic phenomena. | ||
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| 700 | 1 | |a Wolfson, C. J. |4 aut | |
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10.1007/BF00777855 doi (DE-627)OLC2033675904 (DE-He213)BF00777855-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Strong, K. verfasserin aut Trace — The transition region and coronal explorer 1994 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1994 Abstract TRACE is a single-instrument solar mission that will be put into a Sunsynchronous polar orbit and will obtain continuous solar observations for about 8 months per year. It will collect images of solar plasmas at temperatures from $ 10^{4} $ to $ 10^{7} $ K, with 1-arcsec spatial resolution and excellent temporal resolution and continuity. With such data, we expect to gain a new understanding of many solar and stellar problems ranging from coronal heating to impulsive magnetohydrodynamic phenomena. Bruner, M. aut Tarbell, T. aut Title, A. aut Wolfson, C. J. aut Enthalten in Space science reviews Kluwer Academic Publishers, 1962 70(1994), 1-2 vom: Okt., Seite 119-122 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:70 year:1994 number:1-2 month:10 pages:119-122 https://doi.org/10.1007/BF00777855 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2015 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 70 1994 1-2 10 119-122 |
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10.1007/BF00777855 doi (DE-627)OLC2033675904 (DE-He213)BF00777855-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Strong, K. verfasserin aut Trace — The transition region and coronal explorer 1994 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1994 Abstract TRACE is a single-instrument solar mission that will be put into a Sunsynchronous polar orbit and will obtain continuous solar observations for about 8 months per year. It will collect images of solar plasmas at temperatures from $ 10^{4} $ to $ 10^{7} $ K, with 1-arcsec spatial resolution and excellent temporal resolution and continuity. With such data, we expect to gain a new understanding of many solar and stellar problems ranging from coronal heating to impulsive magnetohydrodynamic phenomena. Bruner, M. aut Tarbell, T. aut Title, A. aut Wolfson, C. J. aut Enthalten in Space science reviews Kluwer Academic Publishers, 1962 70(1994), 1-2 vom: Okt., Seite 119-122 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:70 year:1994 number:1-2 month:10 pages:119-122 https://doi.org/10.1007/BF00777855 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2015 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 70 1994 1-2 10 119-122 |
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Abstract TRACE is a single-instrument solar mission that will be put into a Sunsynchronous polar orbit and will obtain continuous solar observations for about 8 months per year. It will collect images of solar plasmas at temperatures from $ 10^{4} $ to $ 10^{7} $ K, with 1-arcsec spatial resolution and excellent temporal resolution and continuity. With such data, we expect to gain a new understanding of many solar and stellar problems ranging from coronal heating to impulsive magnetohydrodynamic phenomena. © Kluwer Academic Publishers 1994 |
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Abstract TRACE is a single-instrument solar mission that will be put into a Sunsynchronous polar orbit and will obtain continuous solar observations for about 8 months per year. It will collect images of solar plasmas at temperatures from $ 10^{4} $ to $ 10^{7} $ K, with 1-arcsec spatial resolution and excellent temporal resolution and continuity. With such data, we expect to gain a new understanding of many solar and stellar problems ranging from coronal heating to impulsive magnetohydrodynamic phenomena. © Kluwer Academic Publishers 1994 |
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Abstract TRACE is a single-instrument solar mission that will be put into a Sunsynchronous polar orbit and will obtain continuous solar observations for about 8 months per year. It will collect images of solar plasmas at temperatures from $ 10^{4} $ to $ 10^{7} $ K, with 1-arcsec spatial resolution and excellent temporal resolution and continuity. With such data, we expect to gain a new understanding of many solar and stellar problems ranging from coronal heating to impulsive magnetohydrodynamic phenomena. © Kluwer Academic Publishers 1994 |
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Trace — The transition region and coronal explorer |
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