Jupiter in 1999/2000. II: Infrared wavelengths

Details Jupiter in 1999/2000. II: Infrared wavelengths Jupiter in 1999/2000. II: Infrared wavelengths

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003jbaa..113..136r&link_type=abstract

Journal of the British Astronomical Association, vol.113, no.3, p.136-140

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Several observers are now producing valuable images in the near-infrared methane absorption band, at the wavelength of 890nm. These images record high-altitude clouds and hazes. This article discusses the relative selectivity of the filters used by different observers, the features shown by them in 1999/2000, and the aspects that will be of interest for routine monitoring by methane images. These include the polar hoods, the equatorial zone, possibly erupting plume heads, anticyclonic ovals, and large scale disturbances of the major belts.

Affiliated with

Also associated with

No associations

Rating

Jupiter in 1999/2000. II: Infrared wavelengths does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Jupiter in 1999/2000. II: Infrared wavelengths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Jupiter in 1999/2000. II: Infrared wavelengths will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1867206