Publication detail

Imaging Comet ISON C/2012 S1 in the Inner Corona at Perihelion

DRUCKMÜLLER, M. HABBAL, S. ANIOL, P. DING, A. MORGAN, H.

English title

Imaging Comet ISON C/2012 S1 in the Inner Corona at Perihelion

Type

WoS Article

Language

en

Original abstract

Much anticipation and speculation were building around comet ISON, or C/2012 S1, discovered on 2012 September 21 by the International Scientific Optical Network telescope in Russia, and bound for the Sun on 2013 November 28, with a closest heliocentric approach distance of 2.7 R. Here we present the first white light image of the comet's trail through the inner corona. The image was taken with a wide field Lyot-type coronagraph from the Mees Observatory on Haleakala at 19:12 UT, past its perihelion passage at 18:45 UT. The perfect match between the comet's trail captured in the inner corona and the trail that had persisted across the field of view of 2-6 R of the Solar and Heliospheric Observatory Large Angle and Spectrometric Coronagraph Experiment/C2 coronagraph at 19:12 UT demonstrates that comet survived its perihelion passage.

Keywords in English

comets, C/2012 S1 ISON, Sun, corona

Released

2014-03-12

ISSN

2041-8205

Journal

Astrophysical Journal Letters

Volume

2014( 784)

Number

2

Pages from–to

22–25

Pages count

4

BIBTEX


@article{BUT106821,
  author="Miloslav {Druckmüller} and Shadia Rifai {Habbal} and Peter {Aniol} and Adalbert {Ding} and Huw {Morgan}",
  title="Imaging Comet ISON C/2012 S1 in the Inner Corona at Perihelion",
  journal="Astrophysical Journal Letters",
  year="2014",
  volume="2014( 784)",
  number="2",
  pages="22--25",
  doi="10.1088/2041-8205/784/2/L22",
  issn="2041-8205"
}