Aspects of Multi-Dimensional Modelling of Substellar Atmospheres

Christiane Helling; E. Pedretti; S. Berdyugina; A. A. Vidotto; B. Beeck; E. Baron; A. P. Showman; E. Agol; D. Homeier

Aspects of Multi-Dimensional Modelling of Substellar Atmospheres

Christiane Helling, E. Pedretti, S. Berdyugina, A. A. Vidotto, B. Beeck, E. Baron, A. P. Showman, E. Agol, D. Homeier

School of Physics and Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

Theoretical arguments and observations suggest that the atmospheres of Brown Dwarfs and planets are very dynamic on chemical and on physical time scales. The modelling of such substellar atmospheres has, hence, been much more demanding than initially anticipated. This Splinter(1) has combined new developments in atmosphere modelling, with novel observational techniques, and new challenges arising from planetary and space weather observations.

Original language	English
Title of host publication	16th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
Editors	CMJ JohnsKrull, MK Browning, AA West
Place of Publication	San Francisco
Publisher	Astronomical Society of the Pacific
Pages	403-414
Number of pages	12
ISBN (Print)	978-1-58381-776-6
Publication status	Published - 2011
Event	16th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - Seattle Duration: 28 Aug 2010 → 3 Sept 2010

Conference

Conference	16th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
City	Seattle
Period	28/08/10 → 3/09/10

Cite this

@inproceedings{cec816c0142148ebbc42163a19f977dc,

title = "Aspects of Multi-Dimensional Modelling of Substellar Atmospheres",

abstract = "Theoretical arguments and observations suggest that the atmospheres of Brown Dwarfs and planets are very dynamic on chemical and on physical time scales. The modelling of such substellar atmospheres has, hence, been much more demanding than initially anticipated. This Splinter(1) has combined new developments in atmosphere modelling, with novel observational techniques, and new challenges arising from planetary and space weather observations.",

author = "Christiane Helling and E. Pedretti and S. Berdyugina and Vidotto, {A. A.} and B. Beeck and E. Baron and Showman, {A. P.} and E. Agol and D. Homeier",

year = "2011",

language = "English",

isbn = "978-1-58381-776-6",

pages = "403--414",

editor = "CMJ JohnsKrull and MK Browning and AA West",

booktitle = "16th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun",

publisher = "Astronomical Society of the Pacific",

note = "16th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun ; Conference date: 28-08-2010 Through 03-09-2010",

}

Helling, C, Pedretti, E, Berdyugina, S, Vidotto, AA, Beeck, B, Baron, E, Showman, AP, Agol, E & Homeier, D 2011, Aspects of Multi-Dimensional Modelling of Substellar Atmospheres. in CMJ JohnsKrull, MK Browning & AA West (eds), 16th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. Astronomical Society of the Pacific, San Francisco, pp. 403-414, 16th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, Seattle, 28/08/10.

Aspects of Multi-Dimensional Modelling of Substellar Atmospheres. / Helling, Christiane; Pedretti, E.; Berdyugina, S. et al.
16th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. ed. / CMJ JohnsKrull; MK Browning; AA West. San Francisco: Astronomical Society of the Pacific, 2011. p. 403-414.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Aspects of Multi-Dimensional Modelling of Substellar Atmospheres

AU - Helling, Christiane

AU - Pedretti, E.

AU - Berdyugina, S.

AU - Vidotto, A. A.

AU - Beeck, B.

AU - Baron, E.

AU - Showman, A. P.

AU - Agol, E.

AU - Homeier, D.

PY - 2011

Y1 - 2011

N2 - Theoretical arguments and observations suggest that the atmospheres of Brown Dwarfs and planets are very dynamic on chemical and on physical time scales. The modelling of such substellar atmospheres has, hence, been much more demanding than initially anticipated. This Splinter(1) has combined new developments in atmosphere modelling, with novel observational techniques, and new challenges arising from planetary and space weather observations.

AB - Theoretical arguments and observations suggest that the atmospheres of Brown Dwarfs and planets are very dynamic on chemical and on physical time scales. The modelling of such substellar atmospheres has, hence, been much more demanding than initially anticipated. This Splinter(1) has combined new developments in atmosphere modelling, with novel observational techniques, and new challenges arising from planetary and space weather observations.

M3 - Conference contribution

SN - 978-1-58381-776-6

SP - 403

EP - 414

BT - 16th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun

A2 - JohnsKrull, CMJ

A2 - Browning, MK

A2 - West, AA

PB - Astronomical Society of the Pacific

CY - San Francisco

T2 - 16th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun

Y2 - 28 August 2010 through 3 September 2010

ER -

Aspects of Multi-Dimensional Modelling of Substellar Atmospheres

Abstract

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