Discovery of diffuse aurora on Mars.

Autor: Schneider NM; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO 80303, USA. nick.schneider@lasp.colorado.edu., Deighan JI; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO 80303, USA., Jain SK; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO 80303, USA., Stiepen A; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO 80303, USA., Stewart AI; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO 80303, USA., Larson D; Space Sciences Lab, University of California, Berkeley, Berkeley, CA 94720, USA., Mitchell DL; Space Sciences Lab, University of California, Berkeley, Berkeley, CA 94720, USA., Mazelle C; Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, Toulouse, France. University Paul Sabatier, IRAP, CNRS, Toulouse, France., Lee CO; Space Sciences Lab, University of California, Berkeley, Berkeley, CA 94720, USA., Lillis RJ; Space Sciences Lab, University of California, Berkeley, Berkeley, CA 94720, USA., Evans JS; Computational Physics, Inc, Springfield, VA 22151, USA., Brain D; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO 80303, USA., Stevens MH; Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA., McClintock WE; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO 80303, USA., Chaffin MS; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO 80303, USA., Crismani M; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO 80303, USA., Holsclaw GM; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO 80303, USA., Lefevre F; Laboratoire Atmosphères, Milieux, Observations Spatiales, Institut Pierre Simon Laplace, Guyancourt, France., Lo DY; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA., Clarke JT; Center for Space Physics, Boston University, Boston, MA 02215, USA., Montmessin F; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA., Jakosky BM; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Boulder, CO 80303, USA.
Jazyk: angličtina
Zdroj: Science (New York, N.Y.) [Science] 2015 Nov 06; Vol. 350 (6261), pp. aad0313.
DOI: 10.1126/science.aad0313
Abstrakt: Planetary auroras reveal the complex interplay between an atmosphere and the surrounding plasma environment. We report the discovery of low-altitude, diffuse auroras spanning much of Mars' northern hemisphere, coincident with a solar energetic particle outburst. The Imaging Ultraviolet Spectrograph, a remote sensing instrument on the Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft, detected auroral emission in virtually all nightside observations for ~5 days, spanning nearly all geographic longitudes. Emission extended down to ~60 kilometer (km) altitude (1 microbar), deeper than confirmed at any other planet. Solar energetic particles were observed up to 200 kilo--electron volts; these particles are capable of penetrating down to the 60 km altitude. Given minimal magnetic fields over most of the planet, Mars is likely to exhibit auroras more globally than Earth.
(Copyright © 2015, American Association for the Advancement of Science.)
Databáze: MEDLINE