Detail publikačního výsledku

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

HABBAL, S.; MORGAN, H.; DRUCKMÜLLER, M.; DING, A.; COOPER, J.; DAW, A.; SITTLER, E.

Originální název

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

Anglický název

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

Druh

Článek recenzovaný mimo WoS a Scopus

Originální abstrakt

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 above the 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 draws attention 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.

Anglický abstrakt

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 above the 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 draws attention 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.

Klíčová slova

Corona , Eclipse, Solar wind

Klíčová slova v angličtině

Corona , Eclipse, Solar wind

Autoři

HABBAL, S.; MORGAN, H.; DRUCKMÜLLER, M.; DING, A.; COOPER, J.; DAW, A.; SITTLER, E.

Rok RIV

2016

Vydáno

01.07.2013

Nakladatel

Springer

ISSN

0038-0938

Periodikum

SOLAR PHYSICS

Svazek

2013 (285)

Číslo

1-2

Stát

Nizozemsko

Strany od

9

Strany do

24

Strany počet

16

BibTex

@article{BUT94444,
  author="Shadia Rifai {Habbal} and Huw {Morgan} and Miloslav {Druckmüller} and Adalbert {Ding} and John. F. {Cooper} and Adrian {Daw} and Edward C. {Sittler}",
  title="Probing the Fundamental Physics of the Solar Corona with Lunar Solar Occultation Observations",
  journal="SOLAR PHYSICS",
  year="2013",
  volume="2013 (285)",
  number="1-2",
  pages="9--24",
  issn="0038-0938"
}