Detail publikace

Fine Structures in the White-light Solar Corona at the 2006 Eclipse

PASACHOFF, M. RUŠIN, V. DRUCKMÜLLER, M. SANIGA, M.

Český název

Fine Structures in the White-light Solar Corona at the 2006 Eclipse

Anglický název

Fine Structures in the White-light Solar Corona at the 2006 Eclipse

Typ

článek v časopise - ostatní, Jost

Jazyk

en

Originální abstrakt

Observations of the total solar eclipse of 2006 March 29, as it crossed Africa from southwest to northeast into a Greek island and beyond, allowed correlations with near-simultaneous coronal observations from several spacecraft, including SOHO and TRACE. New methods of compositing images allow the recovery of higher resolution (100Y200) on coronal features than had normally been available in the past, reaching substantially higher resolutions than are currently available from space.We discuss a variety of the new methods and observations, and use them to provide the most detailed portrait possible of the Sun, at least on 2006 March 29.

Český abstrakt

Observations of the total solar eclipse of 2006 March 29, as it crossed Africa from southwest to northeast into a Greek island and beyond, allowed correlations with near-simultaneous coronal observations from several spacecraft, including SOHO and TRACE. New methods of compositing images allow the recovery of higher resolution (100Y200) on coronal features than had normally been available in the past, reaching substantially higher resolutions than are currently available from space.We discuss a variety of the new methods and observations, and use them to provide the most detailed portrait possible of the Sun, at least on 2006 March 29.

Anglický abstrakt

Observations of the total solar eclipse of 2006 March 29, as it crossed Africa from southwest to northeast into a Greek island and beyond, allowed correlations with near-simultaneous coronal observations from several spacecraft, including SOHO and TRACE. New methods of compositing images allow the recovery of higher resolution (100Y200) on coronal features than had normally been available in the past, reaching substantially higher resolutions than are currently available from space.We discuss a variety of the new methods and observations, and use them to provide the most detailed portrait possible of the Sun, at least on 2006 March 29.

Klíčová slova anglicky

solar corona, eclipse, image processing

Rok RIV

2007

Vydáno

10.08.2007

ISSN

0004-637X

Časopis

ASTROPHYSICAL JOURNAL

Ročník

665

Číslo

1

Strany od–do

824–829

Počet stran

5

BIBTEX


@article{BUT44072,
  author="M.J. {Pasachoff} and Vojtěch {Rušin} and Miloslav {Druckmüller} and Metod {Saniga},
  title="Fine Structures in the White-light Solar Corona at the 2006 Eclipse",
  journal="ASTROPHYSICAL JOURNAL",
  year="2007",
  volume="665",
  number="1",
  month="August",
  pages="824--829",
  issn="0004-637X"
}