Probing the Fundamental Physics of the Solar Corona with Lunar Solar Occultation Observations

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216305%3A26210%2F13%3APU100110" target="_blank" >RIV/00216305:26210/13:PU100110 - isvavai.cz</a>

Výsledek na webu

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DOI - Digital Object Identifier

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Jazyk výsledku

angličtina

Název v původním jazyce

Probing the Fundamental Physics of the Solar Corona with Lunar Solar Occultation Observations

Popis výsledku v původním jazyce

Imaging and spectroscopy of the solar corona, coupled with polarimetry, are the only tools available at present to capture signatures of physical rocesses responsible for coronal heating and solar wind acceleration within the first few solar radii abovethe solar limb. With the recent advent of mproved detector technology and image processing techniques, broad-band white light and narrow-band multi-wavelength observations of coronal forbidden lines, made during total solar eclipses, have started to yield new views about the thermodynamic and magnetic properties of coronal tructures. This paper outlines these unique capabilities, which until present, have been feasible primarily with observations during natural total solar clipses. This work also drawsattention to the exciting possibility of greatly increasing the frequency and duration of solar eclipse observations with Moon orbiting observatories utilizing lunar limb occultation of the solar disk for coronal measurements.

Název v anglickém jazyce

Probing the Fundamental Physics of the Solar Corona with Lunar Solar Occultation Observations

Popis výsledku anglicky

Imaging and spectroscopy of the solar corona, coupled with polarimetry, are the only tools available at present to capture signatures of physical rocesses responsible for coronal heating and solar wind acceleration within the first few solar radii abovethe solar limb. With the recent advent of mproved detector technology and image processing techniques, broad-band white light and narrow-band multi-wavelength observations of coronal forbidden lines, made during total solar eclipses, have started to yield new views about the thermodynamic and magnetic properties of coronal tructures. This paper outlines these unique capabilities, which until present, have been feasible primarily with observations during natural total solar clipses. This work also drawsattention to the exciting possibility of greatly increasing the frequency and duration of solar eclipse observations with Moon orbiting observatories utilizing lunar limb occultation of the solar disk for coronal measurements.

Druh

J_x - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)

CEP obor

BL - Fyzika plasmatu a výboje v plynech

OECD FORD obor

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Projekt

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Návaznosti

S - Specificky vyzkum na vysokych skolach

Rok uplatnění

2013

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Solar Physics

ISSN

0038-0938

e-ISSN

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Svazek periodika

2013 (285)

Číslo periodika v rámci svazku

1-2

Stát vydavatele periodika

NL - Nizozemsko

Počet stran výsledku

16

Strana od-do

9-24

Kód UT WoS článku

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EID výsledku v databázi Scopus

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