Issue |
A&A
Volume 577, May 2015
|
|
---|---|---|
Article Number | A94 | |
Number of page(s) | 5 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/201425406 | |
Published online | 08 May 2015 |
Research Note
Ground-based search for lightning in Jupiter with GTC/OSIRIS fast photometry and tunable filters
1
Instituto de Astrofísica de Andalucía, IAA-CSIC,
PO Box 3004
18080
Granada
Spain
e-mail:
aluque@iaa.es
2
Instituto de Astrofísica de Canarias (IAC),
Vía Láctea s/n
38200, La Laguna,
Spain
3 Departamento de Astrofísica, Universidad de La Laguna, Spain
Received: 26 November 2014
Accepted: 7 March 2015
Context. Lightning flashes in Jupiter have been observed by spacecraft orbiting the planet, but so far, they have escaped optical detection from Earth. However, theoretical estimations suggest that these flashes may be detectable by a large telescope if they can be distinguished from the much more intense background of reflected sunlight from the dayside of the planet that is visible from Earth.
Aims. Here we attempt such a detection with the 10.4 m Gran Telescopio de Canarias (GTC) telescope.
Methods. To increase the signal-to-background ratio of Jovian lightning flashes in the dayside, we used the recently commissioned fast-photometry modes of the GTC together with a tunable narrowband filter centered on the hydrogen Hα line. The observations were then tested to determine whether they contain statistically significant deviations from the expected noise and instrumental artifacts.
Results. Our results are consistent with the null hypothesis that lightning flashes were not detected.
Key words: planets and satellites: atmospheres / planets and satellites: gaseous planets / methods: statistical
© ESO, 2015
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