Uranus: Microwave Images

Observations of Uranus at wavelengths of 2 and 6 centimeters with the Very Large Array were made in 1980 and 1981. The resulting maps of brightness temperature show a subsolar symmetry at 2 centimeters but a near-polar symmetry at 6 centimeters. The 6-centimeter maps show an increase in temperature...

Full description

Bibliographic Details
Published in:Science
Main Authors: Jaffe, Walter J., Berge, Glenn L., Owen, Tobias, Caldwell, John
Format: Article in Journal/Newspaper
Language:English
Published: American Association for the Advancement of Science (AAAS) 1984
Subjects:
Online Access:http://dx.doi.org/10.1126/science.11541997
https://www.science.org/doi/pdf/10.1126/science.11541997
id craaas:10.1126/science.11541997
record_format openpolar
spelling craaas:10.1126/science.11541997 2024-06-09T07:48:26+00:00 Uranus: Microwave Images Jaffe, Walter J. Berge, Glenn L. Owen, Tobias Caldwell, John 1984 http://dx.doi.org/10.1126/science.11541997 https://www.science.org/doi/pdf/10.1126/science.11541997 en eng American Association for the Advancement of Science (AAAS) Science volume 225, issue 4662, page 619-621 ISSN 0036-8075 1095-9203 journal-article 1984 craaas https://doi.org/10.1126/science.11541997 2024-05-16T12:53:53Z Observations of Uranus at wavelengths of 2 and 6 centimeters with the Very Large Array were made in 1980 and 1981. The resulting maps of brightness temperature show a subsolar symmetry at 2 centimeters but a near-polar symmetry at 6 centimeters. The 6-centimeter maps show an increase in temperature from equator to pole with some evidence for a warm "ring" surrounding the north pole. The disk-average temperatures (147 ± 5 K and 230 ± 6 K at 2 and 6 centimeters, respectively) are distinctly lower than recently reported values; these results suggest that the secular increase in temperature reported during the last 15 years has been reversed. The variations in brightness temperature probably reflect variations in ammonia abundance in the planet's atmosphere, but the mechanism driving these variations is still unclear. Article in Journal/Newspaper North Pole AAAS Resource Center (American Association for the Advancement of Science) North Pole Science 225 4662 619 621
institution Open Polar
collection AAAS Resource Center (American Association for the Advancement of Science)
op_collection_id craaas
language English
description Observations of Uranus at wavelengths of 2 and 6 centimeters with the Very Large Array were made in 1980 and 1981. The resulting maps of brightness temperature show a subsolar symmetry at 2 centimeters but a near-polar symmetry at 6 centimeters. The 6-centimeter maps show an increase in temperature from equator to pole with some evidence for a warm "ring" surrounding the north pole. The disk-average temperatures (147 ± 5 K and 230 ± 6 K at 2 and 6 centimeters, respectively) are distinctly lower than recently reported values; these results suggest that the secular increase in temperature reported during the last 15 years has been reversed. The variations in brightness temperature probably reflect variations in ammonia abundance in the planet's atmosphere, but the mechanism driving these variations is still unclear.
format Article in Journal/Newspaper
author Jaffe, Walter J.
Berge, Glenn L.
Owen, Tobias
Caldwell, John
spellingShingle Jaffe, Walter J.
Berge, Glenn L.
Owen, Tobias
Caldwell, John
Uranus: Microwave Images
author_facet Jaffe, Walter J.
Berge, Glenn L.
Owen, Tobias
Caldwell, John
author_sort Jaffe, Walter J.
title Uranus: Microwave Images
title_short Uranus: Microwave Images
title_full Uranus: Microwave Images
title_fullStr Uranus: Microwave Images
title_full_unstemmed Uranus: Microwave Images
title_sort uranus: microwave images
publisher American Association for the Advancement of Science (AAAS)
publishDate 1984
url http://dx.doi.org/10.1126/science.11541997
https://www.science.org/doi/pdf/10.1126/science.11541997
geographic North Pole
geographic_facet North Pole
genre North Pole
genre_facet North Pole
op_source Science
volume 225, issue 4662, page 619-621
ISSN 0036-8075 1095-9203
op_doi https://doi.org/10.1126/science.11541997
container_title Science
container_volume 225
container_issue 4662
container_start_page 619
op_container_end_page 621
_version_ 1801380164078141440