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18 April 2024
 
  » arxiv » astro-ph/0504110

 Article overview


Chandra Observation of an X-ray Flare at Saturn: Evidence for Direct Solar Control on Saturn's Disk X-ray Emissions
Anil Bhardwaj ; Ronald F. Elsner ; J. Hunter Waite Jr ; G. Randall Gladstone ; Thomas E. Cravens ; Peter G. Ford ;
Date 5 Apr 2005
Journal Astrophys.J. 624 (2005) L121-L124
Subject astro-ph
AbstractSaturn was observed by Chandra ACIS-S on 20 and 26-27 January 2004 for one full Saturn rotation (10.7 hr) at each epoch. We report here the first observation of an X-ray flare from Saturn’s non-auroral (low-latitude) disk, which is seen in direct response to an M6-class flare emanating from a sunspot that was clearly visible from both Saturn and Earth. Saturn’s disk X-ray emissions are found to be variable on time scales of hours to weeks to months, and correlated with solar F10.7 cm flux. Unlike Jupiter, X-rays from Saturn’s polar (auroral) region have characteristics similar to those from its disk. This report, combined with earlier studies, establishes that disk X-ray emissions of the giant planets Saturn and Jupiter are directly regulated by processes happening on the Sun. We suggest that these emissions could be monitored to study X-ray flaring from solar active regions when they are on the far side and not visible to Near-Earth space weather satellites.
Source arXiv, astro-ph/0504110
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