Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak
Abstract We report the observations of the solar chromosphere from a newly commissioned solar telescope at the incursion site near Pangong Tso lake in Merak (Leh/Ladakh). This new %$\hbox {H}_{\alpha }%$ telescope at the Merak site is identical to the Kodaikanal %$\hbox {H}_{\alpha }%$ telescope. Th...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Ravindra, B. [verfasserIn] Kesavan, Prabhu [verfasserIn] Thulasidharen, K. C. [verfasserIn] Rajalingam, M. [verfasserIn] Sagayanathan, K. [verfasserIn] Kamath, P. U. [verfasserIn] Dorjey, Namgyal [verfasserIn] Dorjee, Angchuk [verfasserIn] Kemkar, P. M. M. [verfasserIn] Dorjai, Tsewang [verfasserIn] Banyal, Ravinder K. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2018 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Journal of astrophysics and astronomy - Bangalore : Springer India, 1980, 39(2018), 5 vom: 27. Sept. |
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| Übergeordnetes Werk: |
volume:39 ; year:2018 ; number:5 ; day:27 ; month:09 |
| Links: |
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| DOI / URN: |
10.1007/s12036-018-9554-1 |
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| Katalog-ID: |
SPR023998148 |
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| 245 | 1 | 0 | |a Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak |
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| 520 | |a Abstract We report the observations of the solar chromosphere from a newly commissioned solar telescope at the incursion site near Pangong Tso lake in Merak (Leh/Ladakh). This new %$\hbox {H}_{\alpha }%$ telescope at the Merak site is identical to the Kodaikanal %$\hbox {H}_{\alpha }%$ telescope. The telescope was installed in the month of August 2017 at the Merak site. The telescope consists of a 20-cm doublet lens with additional re-imaging optics. A Lyot filter with 0.5 Å passband isolates the Balmer line of the hydrogen spectra to make the observations of the solar chromosphere. The observations made in %$\hbox {H}_{\alpha }%$ wavelength delineates the magnetic field directions at the sunspot and the quiet regions. A CCD detector records the images of the chromosphere with a pixel resolution of 0.27%$^{\prime \prime }%$ and covers 9.2%$^{\prime }%$ field-of-view. This telescope has a good guiding system that keeps the FoV in the intended position. We report the development of control software for tuning the filter unit, control detector system, observations and calibration of the data to make it useful for the scientific community. Some preliminary results obtained from the Merak %$\hbox {H}_{\alpha }%$ telescope are also presented. This high altitude facility is a timely addition to regularly obtain %$\hbox {H}_{\alpha }%$ images around the globe. | ||
| 650 | 4 | |a Sun: chromosphere |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Sun: |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a telescope |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Sun: |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a surge |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Kesavan, Prabhu |e verfasserin |4 aut | |
| 700 | 1 | |a Thulasidharen, K. C. |e verfasserin |4 aut | |
| 700 | 1 | |a Rajalingam, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Sagayanathan, K. |e verfasserin |4 aut | |
| 700 | 1 | |a Kamath, P. U. |e verfasserin |4 aut | |
| 700 | 1 | |a Dorjey, Namgyal |e verfasserin |4 aut | |
| 700 | 1 | |a Dorjee, Angchuk |e verfasserin |4 aut | |
| 700 | 1 | |a Kemkar, P. M. M. |e verfasserin |4 aut | |
| 700 | 1 | |a Dorjai, Tsewang |e verfasserin |4 aut | |
| 700 | 1 | |a Banyal, Ravinder K. |e verfasserin |4 aut | |
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10.1007/s12036-018-9554-1 doi (DE-627)SPR023998148 (SPR)s12036-018-9554-1-e DE-627 ger DE-627 rakwb eng 520 ASE 39.22 bkl Ravindra, B. verfasserin aut Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We report the observations of the solar chromosphere from a newly commissioned solar telescope at the incursion site near Pangong Tso lake in Merak (Leh/Ladakh). This new %$\hbox {H}_{\alpha }%$ telescope at the Merak site is identical to the Kodaikanal %$\hbox {H}_{\alpha }%$ telescope. The telescope was installed in the month of August 2017 at the Merak site. The telescope consists of a 20-cm doublet lens with additional re-imaging optics. A Lyot filter with 0.5 Å passband isolates the Balmer line of the hydrogen spectra to make the observations of the solar chromosphere. The observations made in %$\hbox {H}_{\alpha }%$ wavelength delineates the magnetic field directions at the sunspot and the quiet regions. A CCD detector records the images of the chromosphere with a pixel resolution of 0.27%$^{\prime \prime }%$ and covers 9.2%$^{\prime }%$ field-of-view. This telescope has a good guiding system that keeps the FoV in the intended position. We report the development of control software for tuning the filter unit, control detector system, observations and calibration of the data to make it useful for the scientific community. Some preliminary results obtained from the Merak %$\hbox {H}_{\alpha }%$ telescope are also presented. This high altitude facility is a timely addition to regularly obtain %$\hbox {H}_{\alpha }%$ images around the globe. Sun: chromosphere (dpeaa)DE-He213 Sun: (dpeaa)DE-He213 telescope (dpeaa)DE-He213 Sun: (dpeaa)DE-He213 surge (dpeaa)DE-He213 Kesavan, Prabhu verfasserin aut Thulasidharen, K. C. verfasserin aut Rajalingam, M. verfasserin aut Sagayanathan, K. verfasserin aut Kamath, P. U. verfasserin aut Dorjey, Namgyal verfasserin aut Dorjee, Angchuk verfasserin aut Kemkar, P. M. M. verfasserin aut Dorjai, Tsewang verfasserin aut Banyal, Ravinder K. verfasserin aut Enthalten in Journal of astrophysics and astronomy Bangalore : Springer India, 1980 39(2018), 5 vom: 27. Sept. (DE-627)358454131 (DE-600)2096381-6 0973-7758 nnns volume:39 year:2018 number:5 day:27 month:09 https://dx.doi.org/10.1007/s12036-018-9554-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 39.22 ASE AR 39 2018 5 27 09 |
| spelling |
10.1007/s12036-018-9554-1 doi (DE-627)SPR023998148 (SPR)s12036-018-9554-1-e DE-627 ger DE-627 rakwb eng 520 ASE 39.22 bkl Ravindra, B. verfasserin aut Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We report the observations of the solar chromosphere from a newly commissioned solar telescope at the incursion site near Pangong Tso lake in Merak (Leh/Ladakh). This new %$\hbox {H}_{\alpha }%$ telescope at the Merak site is identical to the Kodaikanal %$\hbox {H}_{\alpha }%$ telescope. The telescope was installed in the month of August 2017 at the Merak site. The telescope consists of a 20-cm doublet lens with additional re-imaging optics. A Lyot filter with 0.5 Å passband isolates the Balmer line of the hydrogen spectra to make the observations of the solar chromosphere. The observations made in %$\hbox {H}_{\alpha }%$ wavelength delineates the magnetic field directions at the sunspot and the quiet regions. A CCD detector records the images of the chromosphere with a pixel resolution of 0.27%$^{\prime \prime }%$ and covers 9.2%$^{\prime }%$ field-of-view. This telescope has a good guiding system that keeps the FoV in the intended position. We report the development of control software for tuning the filter unit, control detector system, observations and calibration of the data to make it useful for the scientific community. Some preliminary results obtained from the Merak %$\hbox {H}_{\alpha }%$ telescope are also presented. This high altitude facility is a timely addition to regularly obtain %$\hbox {H}_{\alpha }%$ images around the globe. Sun: chromosphere (dpeaa)DE-He213 Sun: (dpeaa)DE-He213 telescope (dpeaa)DE-He213 Sun: (dpeaa)DE-He213 surge (dpeaa)DE-He213 Kesavan, Prabhu verfasserin aut Thulasidharen, K. C. verfasserin aut Rajalingam, M. verfasserin aut Sagayanathan, K. verfasserin aut Kamath, P. U. verfasserin aut Dorjey, Namgyal verfasserin aut Dorjee, Angchuk verfasserin aut Kemkar, P. M. M. verfasserin aut Dorjai, Tsewang verfasserin aut Banyal, Ravinder K. verfasserin aut Enthalten in Journal of astrophysics and astronomy Bangalore : Springer India, 1980 39(2018), 5 vom: 27. Sept. (DE-627)358454131 (DE-600)2096381-6 0973-7758 nnns volume:39 year:2018 number:5 day:27 month:09 https://dx.doi.org/10.1007/s12036-018-9554-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 39.22 ASE AR 39 2018 5 27 09 |
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10.1007/s12036-018-9554-1 doi (DE-627)SPR023998148 (SPR)s12036-018-9554-1-e DE-627 ger DE-627 rakwb eng 520 ASE 39.22 bkl Ravindra, B. verfasserin aut Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We report the observations of the solar chromosphere from a newly commissioned solar telescope at the incursion site near Pangong Tso lake in Merak (Leh/Ladakh). This new %$\hbox {H}_{\alpha }%$ telescope at the Merak site is identical to the Kodaikanal %$\hbox {H}_{\alpha }%$ telescope. The telescope was installed in the month of August 2017 at the Merak site. The telescope consists of a 20-cm doublet lens with additional re-imaging optics. A Lyot filter with 0.5 Å passband isolates the Balmer line of the hydrogen spectra to make the observations of the solar chromosphere. The observations made in %$\hbox {H}_{\alpha }%$ wavelength delineates the magnetic field directions at the sunspot and the quiet regions. A CCD detector records the images of the chromosphere with a pixel resolution of 0.27%$^{\prime \prime }%$ and covers 9.2%$^{\prime }%$ field-of-view. This telescope has a good guiding system that keeps the FoV in the intended position. We report the development of control software for tuning the filter unit, control detector system, observations and calibration of the data to make it useful for the scientific community. Some preliminary results obtained from the Merak %$\hbox {H}_{\alpha }%$ telescope are also presented. This high altitude facility is a timely addition to regularly obtain %$\hbox {H}_{\alpha }%$ images around the globe. Sun: chromosphere (dpeaa)DE-He213 Sun: (dpeaa)DE-He213 telescope (dpeaa)DE-He213 Sun: (dpeaa)DE-He213 surge (dpeaa)DE-He213 Kesavan, Prabhu verfasserin aut Thulasidharen, K. C. verfasserin aut Rajalingam, M. verfasserin aut Sagayanathan, K. verfasserin aut Kamath, P. U. verfasserin aut Dorjey, Namgyal verfasserin aut Dorjee, Angchuk verfasserin aut Kemkar, P. M. M. verfasserin aut Dorjai, Tsewang verfasserin aut Banyal, Ravinder K. verfasserin aut Enthalten in Journal of astrophysics and astronomy Bangalore : Springer India, 1980 39(2018), 5 vom: 27. Sept. (DE-627)358454131 (DE-600)2096381-6 0973-7758 nnns volume:39 year:2018 number:5 day:27 month:09 https://dx.doi.org/10.1007/s12036-018-9554-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 39.22 ASE AR 39 2018 5 27 09 |
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10.1007/s12036-018-9554-1 doi (DE-627)SPR023998148 (SPR)s12036-018-9554-1-e DE-627 ger DE-627 rakwb eng 520 ASE 39.22 bkl Ravindra, B. verfasserin aut Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We report the observations of the solar chromosphere from a newly commissioned solar telescope at the incursion site near Pangong Tso lake in Merak (Leh/Ladakh). This new %$\hbox {H}_{\alpha }%$ telescope at the Merak site is identical to the Kodaikanal %$\hbox {H}_{\alpha }%$ telescope. The telescope was installed in the month of August 2017 at the Merak site. The telescope consists of a 20-cm doublet lens with additional re-imaging optics. A Lyot filter with 0.5 Å passband isolates the Balmer line of the hydrogen spectra to make the observations of the solar chromosphere. The observations made in %$\hbox {H}_{\alpha }%$ wavelength delineates the magnetic field directions at the sunspot and the quiet regions. A CCD detector records the images of the chromosphere with a pixel resolution of 0.27%$^{\prime \prime }%$ and covers 9.2%$^{\prime }%$ field-of-view. This telescope has a good guiding system that keeps the FoV in the intended position. We report the development of control software for tuning the filter unit, control detector system, observations and calibration of the data to make it useful for the scientific community. Some preliminary results obtained from the Merak %$\hbox {H}_{\alpha }%$ telescope are also presented. This high altitude facility is a timely addition to regularly obtain %$\hbox {H}_{\alpha }%$ images around the globe. Sun: chromosphere (dpeaa)DE-He213 Sun: (dpeaa)DE-He213 telescope (dpeaa)DE-He213 Sun: (dpeaa)DE-He213 surge (dpeaa)DE-He213 Kesavan, Prabhu verfasserin aut Thulasidharen, K. C. verfasserin aut Rajalingam, M. verfasserin aut Sagayanathan, K. verfasserin aut Kamath, P. U. verfasserin aut Dorjey, Namgyal verfasserin aut Dorjee, Angchuk verfasserin aut Kemkar, P. M. M. verfasserin aut Dorjai, Tsewang verfasserin aut Banyal, Ravinder K. verfasserin aut Enthalten in Journal of astrophysics and astronomy Bangalore : Springer India, 1980 39(2018), 5 vom: 27. Sept. (DE-627)358454131 (DE-600)2096381-6 0973-7758 nnns volume:39 year:2018 number:5 day:27 month:09 https://dx.doi.org/10.1007/s12036-018-9554-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 39.22 ASE AR 39 2018 5 27 09 |
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10.1007/s12036-018-9554-1 doi (DE-627)SPR023998148 (SPR)s12036-018-9554-1-e DE-627 ger DE-627 rakwb eng 520 ASE 39.22 bkl Ravindra, B. verfasserin aut Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We report the observations of the solar chromosphere from a newly commissioned solar telescope at the incursion site near Pangong Tso lake in Merak (Leh/Ladakh). This new %$\hbox {H}_{\alpha }%$ telescope at the Merak site is identical to the Kodaikanal %$\hbox {H}_{\alpha }%$ telescope. The telescope was installed in the month of August 2017 at the Merak site. The telescope consists of a 20-cm doublet lens with additional re-imaging optics. A Lyot filter with 0.5 Å passband isolates the Balmer line of the hydrogen spectra to make the observations of the solar chromosphere. The observations made in %$\hbox {H}_{\alpha }%$ wavelength delineates the magnetic field directions at the sunspot and the quiet regions. A CCD detector records the images of the chromosphere with a pixel resolution of 0.27%$^{\prime \prime }%$ and covers 9.2%$^{\prime }%$ field-of-view. This telescope has a good guiding system that keeps the FoV in the intended position. We report the development of control software for tuning the filter unit, control detector system, observations and calibration of the data to make it useful for the scientific community. Some preliminary results obtained from the Merak %$\hbox {H}_{\alpha }%$ telescope are also presented. This high altitude facility is a timely addition to regularly obtain %$\hbox {H}_{\alpha }%$ images around the globe. Sun: chromosphere (dpeaa)DE-He213 Sun: (dpeaa)DE-He213 telescope (dpeaa)DE-He213 Sun: (dpeaa)DE-He213 surge (dpeaa)DE-He213 Kesavan, Prabhu verfasserin aut Thulasidharen, K. C. verfasserin aut Rajalingam, M. verfasserin aut Sagayanathan, K. verfasserin aut Kamath, P. U. verfasserin aut Dorjey, Namgyal verfasserin aut Dorjee, Angchuk verfasserin aut Kemkar, P. M. M. verfasserin aut Dorjai, Tsewang verfasserin aut Banyal, Ravinder K. verfasserin aut Enthalten in Journal of astrophysics and astronomy Bangalore : Springer India, 1980 39(2018), 5 vom: 27. Sept. (DE-627)358454131 (DE-600)2096381-6 0973-7758 nnns volume:39 year:2018 number:5 day:27 month:09 https://dx.doi.org/10.1007/s12036-018-9554-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 39.22 ASE AR 39 2018 5 27 09 |
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Enthalten in Journal of astrophysics and astronomy 39(2018), 5 vom: 27. Sept. volume:39 year:2018 number:5 day:27 month:09 |
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Ravindra, B. @@aut@@ Kesavan, Prabhu @@aut@@ Thulasidharen, K. C. @@aut@@ Rajalingam, M. @@aut@@ Sagayanathan, K. @@aut@@ Kamath, P. U. @@aut@@ Dorjey, Namgyal @@aut@@ Dorjee, Angchuk @@aut@@ Kemkar, P. M. M. @@aut@@ Dorjai, Tsewang @@aut@@ Banyal, Ravinder K. @@aut@@ |
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This new %$\hbox {H}_{\alpha }%$ telescope at the Merak site is identical to the Kodaikanal %$\hbox {H}_{\alpha }%$ telescope. The telescope was installed in the month of August 2017 at the Merak site. The telescope consists of a 20-cm doublet lens with additional re-imaging optics. A Lyot filter with 0.5 Å passband isolates the Balmer line of the hydrogen spectra to make the observations of the solar chromosphere. The observations made in %$\hbox {H}_{\alpha }%$ wavelength delineates the magnetic field directions at the sunspot and the quiet regions. A CCD detector records the images of the chromosphere with a pixel resolution of 0.27%$^{\prime \prime }%$ and covers 9.2%$^{\prime }%$ field-of-view. This telescope has a good guiding system that keeps the FoV in the intended position. We report the development of control software for tuning the filter unit, control detector system, observations and calibration of the data to make it useful for the scientific community. Some preliminary results obtained from the Merak %$\hbox {H}_{\alpha }%$ telescope are also presented. 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|
| author |
Ravindra, B. |
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Ravindra, B. ddc 520 bkl 39.22 misc Sun: chromosphere misc Sun: misc telescope misc surge Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak |
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Ravindra, B. |
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520 - Astronomy & allied sciences |
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Not Illustrated |
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0973-7758 |
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520 ASE 39.22 bkl Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak Sun: chromosphere (dpeaa)DE-He213 Sun: (dpeaa)DE-He213 telescope (dpeaa)DE-He213 surge (dpeaa)DE-He213 |
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ddc 520 bkl 39.22 misc Sun: chromosphere misc Sun: misc telescope misc surge |
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ddc 520 bkl 39.22 misc Sun: chromosphere misc Sun: misc telescope misc surge |
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ddc 520 bkl 39.22 misc Sun: chromosphere misc Sun: misc telescope misc surge |
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Elektronische Aufsätze Aufsätze Elektronische Ressource |
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Journal of astrophysics and astronomy |
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520 - Astronomy |
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Journal of astrophysics and astronomy |
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Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak |
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(DE-627)SPR023998148 (SPR)s12036-018-9554-1-e |
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Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak |
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Ravindra, B. |
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Journal of astrophysics and astronomy |
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Journal of astrophysics and astronomy |
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500 - Science |
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2018 |
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Ravindra, B. Kesavan, Prabhu Thulasidharen, K. C. Rajalingam, M. Sagayanathan, K. Kamath, P. U. Dorjey, Namgyal Dorjee, Angchuk Kemkar, P. M. M. Dorjai, Tsewang Banyal, Ravinder K. |
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Elektronische Aufsätze |
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Ravindra, B. |
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10.1007/s12036-018-9554-1 |
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520 |
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verfasserin |
| title_sort |
installation of solar chromospheric telescope at the indian astronomical observatory, merak |
| title_auth |
Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak |
| abstract |
Abstract We report the observations of the solar chromosphere from a newly commissioned solar telescope at the incursion site near Pangong Tso lake in Merak (Leh/Ladakh). This new %$\hbox {H}_{\alpha }%$ telescope at the Merak site is identical to the Kodaikanal %$\hbox {H}_{\alpha }%$ telescope. The telescope was installed in the month of August 2017 at the Merak site. The telescope consists of a 20-cm doublet lens with additional re-imaging optics. A Lyot filter with 0.5 Å passband isolates the Balmer line of the hydrogen spectra to make the observations of the solar chromosphere. The observations made in %$\hbox {H}_{\alpha }%$ wavelength delineates the magnetic field directions at the sunspot and the quiet regions. A CCD detector records the images of the chromosphere with a pixel resolution of 0.27%$^{\prime \prime }%$ and covers 9.2%$^{\prime }%$ field-of-view. This telescope has a good guiding system that keeps the FoV in the intended position. We report the development of control software for tuning the filter unit, control detector system, observations and calibration of the data to make it useful for the scientific community. Some preliminary results obtained from the Merak %$\hbox {H}_{\alpha }%$ telescope are also presented. This high altitude facility is a timely addition to regularly obtain %$\hbox {H}_{\alpha }%$ images around the globe. |
| abstractGer |
Abstract We report the observations of the solar chromosphere from a newly commissioned solar telescope at the incursion site near Pangong Tso lake in Merak (Leh/Ladakh). This new %$\hbox {H}_{\alpha }%$ telescope at the Merak site is identical to the Kodaikanal %$\hbox {H}_{\alpha }%$ telescope. The telescope was installed in the month of August 2017 at the Merak site. The telescope consists of a 20-cm doublet lens with additional re-imaging optics. A Lyot filter with 0.5 Å passband isolates the Balmer line of the hydrogen spectra to make the observations of the solar chromosphere. The observations made in %$\hbox {H}_{\alpha }%$ wavelength delineates the magnetic field directions at the sunspot and the quiet regions. A CCD detector records the images of the chromosphere with a pixel resolution of 0.27%$^{\prime \prime }%$ and covers 9.2%$^{\prime }%$ field-of-view. This telescope has a good guiding system that keeps the FoV in the intended position. We report the development of control software for tuning the filter unit, control detector system, observations and calibration of the data to make it useful for the scientific community. Some preliminary results obtained from the Merak %$\hbox {H}_{\alpha }%$ telescope are also presented. This high altitude facility is a timely addition to regularly obtain %$\hbox {H}_{\alpha }%$ images around the globe. |
| abstract_unstemmed |
Abstract We report the observations of the solar chromosphere from a newly commissioned solar telescope at the incursion site near Pangong Tso lake in Merak (Leh/Ladakh). This new %$\hbox {H}_{\alpha }%$ telescope at the Merak site is identical to the Kodaikanal %$\hbox {H}_{\alpha }%$ telescope. The telescope was installed in the month of August 2017 at the Merak site. The telescope consists of a 20-cm doublet lens with additional re-imaging optics. A Lyot filter with 0.5 Å passband isolates the Balmer line of the hydrogen spectra to make the observations of the solar chromosphere. The observations made in %$\hbox {H}_{\alpha }%$ wavelength delineates the magnetic field directions at the sunspot and the quiet regions. A CCD detector records the images of the chromosphere with a pixel resolution of 0.27%$^{\prime \prime }%$ and covers 9.2%$^{\prime }%$ field-of-view. This telescope has a good guiding system that keeps the FoV in the intended position. We report the development of control software for tuning the filter unit, control detector system, observations and calibration of the data to make it useful for the scientific community. Some preliminary results obtained from the Merak %$\hbox {H}_{\alpha }%$ telescope are also presented. This high altitude facility is a timely addition to regularly obtain %$\hbox {H}_{\alpha }%$ images around the globe. |
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5 |
| title_short |
Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak |
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https://dx.doi.org/10.1007/s12036-018-9554-1 |
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Kesavan, Prabhu Thulasidharen, K. C. Rajalingam, M. Sagayanathan, K. Kamath, P. U. Dorjey, Namgyal Dorjee, Angchuk Kemkar, P. M. M. Dorjai, Tsewang Banyal, Ravinder K. |
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Kesavan, Prabhu Thulasidharen, K. C. Rajalingam, M. Sagayanathan, K. Kamath, P. U. Dorjey, Namgyal Dorjee, Angchuk Kemkar, P. M. M. Dorjai, Tsewang Banyal, Ravinder K. |
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2024-07-03T22:51:52.432Z |
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| score |
7.39968 |