{"id":{"repo_id":"rice","oai_identifier":"oai:repository.rice.edu:1911/104067"},"canonical_url":"https://search.dev.ndltd.org/etd/rice/oai:repository.rice.edu:1911/104067","repository":{"repo_id":"rice","name":"Rice University","base_url":"https://repository.rice.edu/server/oai/request"},"display":{"title":"Correlation of the interplanetary magnetic field with auroral form and latitudinal position","abstract":"Hourly values of the interplanetary magnetic field were compared with photographs of the auroral zone taken by satellite. The photographs were first classified according to the level of auroral activity. It was found that there was a correlation between the north-south component of the magnetic field and the level of auroral activity. The level of activity was seen to increase as the field became more southerly. Measurements of the position of the equatorward and poleward edge of the aurora were also made. These measurements when correlated with the Ysm component of the intersm planetary magnetic field, indicate that the equatorward edge of the aurora moves in a direction antiparallel to the interplanetary magnetic field vector.","abstract_html":"Hourly values of the interplanetary magnetic field were compared with photographs of the auroral zone taken by satellite. The photographs were first classified according to the level of auroral activity. It was found that there was a correlation between the north-south component of the magnetic field and the level of auroral activity. The level of activity was seen to increase as the field became more southerly. Measurements of the position of the equatorward and poleward edge of the aurora were also made. These measurements when correlated with the Ysm component of the intersm planetary magnetic field, indicate that the equatorward edge of the aurora moves in a direction antiparallel to the interplanetary magnetic field vector.","abstract_has_math":false,"creators":["McConnaughhay, Mark Elliott"],"institution":"Rice University","degree_name":"Master of Science","degree_level":"Masters","degree_discipline":"Natural Sciences","degree_department":null,"school":null,"contributors":[],"advisors":["Dessler, A. J."],"committee_chairs":[],"committee_members":[],"year":1977,"date_issued":"1977","date_published":"1977","updated_at":"2026-07-24T04:10:36Z","subjects":[],"languages":["eng"],"rights":["Copyright is held by the author, unless otherwise indicated. Permission to reuse, publish, or reproduce the work beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder."],"rights_urls":[],"identifier_entries":[]},"links":{"outbound_url":"https://hdl.handle.net/1911/104067","outbound_label":"Handle","outbound_source":"dc:identifier.uri"},"metadata_groups":[{"id":"people","label":"People","entries":[{"key":"dc:contributor.advisor","label":"Advisor","values":["Dessler, A. 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These measurements when correlated with the Ysm component of the intersm planetary magnetic field, indicate that the equatorward edge of the aurora moves in a direction antiparallel to the interplanetary magnetic field vector."]},{"key":"dc:title","label":"Title","values":["Correlation of the interplanetary magnetic field with auroral form and latitudinal position"]}]}],"canonical_facts":{"dc:contributor.advisor":["Dessler, A. J."],"dc:creator":["McConnaughhay, Mark Elliott"],"dc:date.accessioned":["2018-12-18T21:16:57Z"],"dc:date.available":["2018-12-18T21:16:57Z"],"dc:date.issued":["1977"],"dc:description.abstract":["Hourly values of the interplanetary magnetic field were compared with photographs of the auroral zone taken by satellite. The photographs were first classified according to the level of auroral activity. It was found that there was a correlation between the north-south component of the magnetic field and the level of auroral activity. The level of activity was seen to increase as the field became more southerly. Measurements of the position of the equatorward and poleward edge of the aurora were also made. These measurements when correlated with the Ysm component of the intersm planetary magnetic field, indicate that the equatorward edge of the aurora moves in a direction antiparallel to the interplanetary magnetic field vector."],"dc:identifier.uri":["https://hdl.handle.net/1911/104067"],"dc:language.iso":["eng"],"dc:rights":["Copyright is held by the author, unless otherwise indicated. Permission to reuse, publish, or reproduce the work beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder."],"dc:title":["Correlation of the interplanetary magnetic field with auroral form and latitudinal position"],"dc:type":["Thesis"],"thesis:degree_discipline":["Natural Sciences"],"thesis:degree_level":["Masters"],"thesis:degree_name":["Master of Science"],"thesis:institution_name":["Rice University"]},"updated_at":"2026-07-24T04:10:36Z"}