Cite abstracts as Author(s) (2006), Title, Eos Trans. AGU, 87(36), Jt. Assem. Suppl., Abstract xxxxx-xx
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withers
HR: 11:10h
AN: U52A-02
TI: Effects of Solar Flares on Earth and Mars
AU: * Mendillo, M
EM: mendillo@bu.edu
AF: Boston University
Center for Space Physics, 725 Commonwealth Avenue, Boston, MA 02215
United States
AU: Withers, P
EM: withers@bu.edu
AF: Boston University
Center for Space Physics, 725 Commonwealth Avenue, Boston, MA 02215
United States
AB:
Flares on the Sun have long been known to cause changes in the
Earth's ionosphere. At other planets, ionospheric observations
are far less common, and certainly not continuous, making the detection
of short-lived flare effects not easy to demonstrate. The Mars Global
Surveyor (MGS) radio science experiment has now made 4896 measurements
of the electron density profiles at Mars since 1998; recent analyses have
shown large electron density enhancements to be due unambiguously to flares.
In this paper, we will review briefly the types of flare effects seen in the
Earth's ionosphere, and relate them to the EUV and X-ray flare emissions that cause
enhancements to the F-layer's total electron content (TEC) and to the E-layer's peak density, respectively.
We will contrast these with effects now being seen at Mars,
assessing both TEC variations and changes in Mars' secondary ionospheric layer.
The different roles of ionization by photo-electrons at the two planets are major
factors in understanding solar-terrestrial-martian relationships.
DE: 6207 Comparative planetology
DE: 6225 Mars
DE: 2400 IONOSPHERE (6929)
DE: 2435 Ionospheric disturbances
DE: 2479 Solar radiation and cosmic ray effects
SC: Union [U]
MN: 2006 Joint Assembly