Ion composition in a noctilucent cloud

Ion composition at mesospheric altitudes was measured and compared between high and mid-latitude sites under summer daytime conditions. Rocket-borne measurements were made with pumped quadrupole ion mass spectrometers. The mid-latitude data were obtained at Wallops Island, Virginia on June 30, 1973,...

Full description

Bibliographic Details
Main Authors: Witt, G., Goldberg, R. A.
Format: Other/Unknown Material
Language:unknown
Published: 1976
Subjects:
Online Access:http://hdl.handle.net/2060/19760021638
id ftnasantrs:oai:casi.ntrs.nasa.gov:19760021638
record_format openpolar
spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19760021638 2023-05-15T17:04:13+02:00 Ion composition in a noctilucent cloud Witt, G. Goldberg, R. A. Unclassified, Unlimited, Publicly available Jul 1, 1976 application/pdf http://hdl.handle.net/2060/19760021638 unknown Document ID: 19760021638 Accession ID: 76N28726 http://hdl.handle.net/2060/19760021638 No Copyright CASI GEOPHYSICS NASA-TM-X-71161 X-912-76-133 1976 ftnasantrs 2019-07-21T11:04:48Z Ion composition at mesospheric altitudes was measured and compared between high and mid-latitude sites under summer daytime conditions. Rocket-borne measurements were made with pumped quadrupole ion mass spectrometers. The mid-latitude data were obtained at Wallops Island, Virginia on June 30, 1973, at 1510 LMT. Large quantities of hydronium cluster ions were observed through 109+, with maximum concentrations at 55+ and 73+. Also, cluster ions of nitric oxide were observed through 84+. The high latitude launch occurred at Kiruna, Sweden on August 2, 1973, at 0700 LMT following visual sighting of a noctilucent cloud on the prior evening. The data near mesopause shows cluster ions, but also a preponderance of heavy ions between 90 and 145 AMU, with groupings 18 AMU apart but unrelated to the more typical cluster ions. One possible set of consistent identifications leads to iron and iron oxide hydrates. These results may suggest the presence of metallic particulates and ions which form hydrated clusters ions. Other/Unknown Material Kiruna NASA Technical Reports Server (NTRS) Kiruna
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic GEOPHYSICS
spellingShingle GEOPHYSICS
Witt, G.
Goldberg, R. A.
Ion composition in a noctilucent cloud
topic_facet GEOPHYSICS
description Ion composition at mesospheric altitudes was measured and compared between high and mid-latitude sites under summer daytime conditions. Rocket-borne measurements were made with pumped quadrupole ion mass spectrometers. The mid-latitude data were obtained at Wallops Island, Virginia on June 30, 1973, at 1510 LMT. Large quantities of hydronium cluster ions were observed through 109+, with maximum concentrations at 55+ and 73+. Also, cluster ions of nitric oxide were observed through 84+. The high latitude launch occurred at Kiruna, Sweden on August 2, 1973, at 0700 LMT following visual sighting of a noctilucent cloud on the prior evening. The data near mesopause shows cluster ions, but also a preponderance of heavy ions between 90 and 145 AMU, with groupings 18 AMU apart but unrelated to the more typical cluster ions. One possible set of consistent identifications leads to iron and iron oxide hydrates. These results may suggest the presence of metallic particulates and ions which form hydrated clusters ions.
format Other/Unknown Material
author Witt, G.
Goldberg, R. A.
author_facet Witt, G.
Goldberg, R. A.
author_sort Witt, G.
title Ion composition in a noctilucent cloud
title_short Ion composition in a noctilucent cloud
title_full Ion composition in a noctilucent cloud
title_fullStr Ion composition in a noctilucent cloud
title_full_unstemmed Ion composition in a noctilucent cloud
title_sort ion composition in a noctilucent cloud
publishDate 1976
url http://hdl.handle.net/2060/19760021638
op_coverage Unclassified, Unlimited, Publicly available
geographic Kiruna
geographic_facet Kiruna
genre Kiruna
genre_facet Kiruna
op_source CASI
op_relation Document ID: 19760021638
Accession ID: 76N28726
http://hdl.handle.net/2060/19760021638
op_rights No Copyright
_version_ 1766058282888200192