Mica: The mirror coronagraph for Argentina

As part of the new German-Argentinian Solar Observatory in El Leoncito, San Juan, Argentina, a new ground-based solar telescope (MICA) began to operate in August 1997. MICA is an advanced mirror coronagraph, its design being an almost exact copy of the LASCO-C1 instrument. Since its installation, it...

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Autores principales: Stenborg, G., Schwenn, R., Srivastava, N., Inhester, B., Podlipnik, B., Rovira, M., Francile, C.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00386308_v87_n1-2_p307_Stenborg
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spelling todo:paper_00386308_v87_n1-2_p307_Stenborg2023-10-03T14:49:13Z Mica: The mirror coronagraph for Argentina Stenborg, G. Schwenn, R. Srivastava, N. Inhester, B. Podlipnik, B. Rovira, M. Francile, C. Corona Coronagraph As part of the new German-Argentinian Solar Observatory in El Leoncito, San Juan, Argentina, a new ground-based solar telescope (MICA) began to operate in August 1997. MICA is an advanced mirror coronagraph, its design being an almost exact copy of the LASCO-C1 instrument. Since its installation, it has been imaging the inner solar corona (1.05 to 2.0 solar radii) in two spectral ranges corresponding to the emission lines of the Fe XIV and Fe X ions. The instrument can image the corona as fast as every minute. Thus, it is ideally suited to study fast processes in the inner corona. In this way, it is a good complement for the LASCO-C1 instrument. After a brief review of the instrument, we present some recent observations showing the capabilities of the instrument. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00386308_v87_n1-2_p307_Stenborg
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Corona
Coronagraph
spellingShingle Corona
Coronagraph
Stenborg, G.
Schwenn, R.
Srivastava, N.
Inhester, B.
Podlipnik, B.
Rovira, M.
Francile, C.
Mica: The mirror coronagraph for Argentina
topic_facet Corona
Coronagraph
description As part of the new German-Argentinian Solar Observatory in El Leoncito, San Juan, Argentina, a new ground-based solar telescope (MICA) began to operate in August 1997. MICA is an advanced mirror coronagraph, its design being an almost exact copy of the LASCO-C1 instrument. Since its installation, it has been imaging the inner solar corona (1.05 to 2.0 solar radii) in two spectral ranges corresponding to the emission lines of the Fe XIV and Fe X ions. The instrument can image the corona as fast as every minute. Thus, it is ideally suited to study fast processes in the inner corona. In this way, it is a good complement for the LASCO-C1 instrument. After a brief review of the instrument, we present some recent observations showing the capabilities of the instrument.
format JOUR
author Stenborg, G.
Schwenn, R.
Srivastava, N.
Inhester, B.
Podlipnik, B.
Rovira, M.
Francile, C.
author_facet Stenborg, G.
Schwenn, R.
Srivastava, N.
Inhester, B.
Podlipnik, B.
Rovira, M.
Francile, C.
author_sort Stenborg, G.
title Mica: The mirror coronagraph for Argentina
title_short Mica: The mirror coronagraph for Argentina
title_full Mica: The mirror coronagraph for Argentina
title_fullStr Mica: The mirror coronagraph for Argentina
title_full_unstemmed Mica: The mirror coronagraph for Argentina
title_sort mica: the mirror coronagraph for argentina
url http://hdl.handle.net/20.500.12110/paper_00386308_v87_n1-2_p307_Stenborg
work_keys_str_mv AT stenborgg micathemirrorcoronagraphforargentina
AT schwennr micathemirrorcoronagraphforargentina
AT srivastavan micathemirrorcoronagraphforargentina
AT inhesterb micathemirrorcoronagraphforargentina
AT podlipnikb micathemirrorcoronagraphforargentina
AT roviram micathemirrorcoronagraphforargentina
AT francilec micathemirrorcoronagraphforargentina
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