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,...
Main Authors: | , |
---|---|
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 |