SuperDARN meteor wind data covering 1993 - 2023. These observations represent an average over approximately 80 - 120 km. X - radar boresight, Y - perpendicular (right, viewed from above). Supported by NSF #1934973 Collaborative Research: Super Dual Auroral Radar Network (SuperDARN) Operations, Research and Community Support. SuperDARN is an international collaboration operating ~35 high frequency (HF) radars deployed in the northern and southern hemispheres to measure ionospheric plasma circulation. Each partner institution secures funding and manages operations for their own facilities. The continued availability of SuperDARN data depends on the proper acknowledgment of data by its users. Guidelines for data acknowledgment are as follows: When data from an individual radar or radars are used, users must contact the principal investigator(s) of those radar(s) to obtain the appropriate acknowledgement information and to offer collaboration, where appropriate. Contact superdarn at jhuapl dot edu for information about this collection. For all usage of SuperDARN data, users are asked to include the following standard acknowledgment text: “The authors acknowledge the use of SuperDARN data. SuperDARN is a collection of radars funded by national scientific funding agencies of Australia, Canada, China, France, Italy, Japan, Norway, South Africa, United Kingdom and the United States of America.” While SuperDARN has an open data use policy, i.e., prior permission to access and analyse the data is not required, the data user is strongly encouraged to establish early contact with any Principal Investigator whose data are involved in the project to discuss the intended usage and collaboration. Data can be subject to limitations that are not immediately evident to users. In addition, some data are embargoed for use by designated Principal Investigators for a period of one year. SuperDARN and the organizations that contributed data must be acknowledged in all reports and publications that use SuperDARN data. The SuperDARN Executive Council must be notified before data are redistributed through another database. The data are not to be used for commercial purposes. If you have any questions about appropriate use of these data, contact any SuperDARN Principal Investigator.
", "publication_date": "2023-05-30", "publisher": "Zenodo", "resource_type": { "id": "dataset", "title": { "de": "Datensatz", "en": "Dataset" } }, "rights": [ { "description": { "en": "The Creative Commons Attribution license allows re-distribution and re-use of a licensed work on the condition that the creator is appropriately credited." }, "icon": "cc-by-icon", "id": "cc-by-4.0", "props": { "scheme": "spdx", "url": "https://creativecommons.org/licenses/by/4.0/legalcode" }, "title": { "en": "Creative Commons Attribution 4.0 International" } } ], "subjects": [ { "subject": "superdarn, aeronomy, mesosphere, thermosphere, cedar, meteor, wind, remote sensing, hf, radar, ionosphere" } ], "title": "SuperDARN meteor winds product (1993 - 2023)", "version": "2" }, "parent": { "access": { "owned_by": { "user": "270414" }, "settings": { "accept_conditions_text": null, "allow_guest_requests": false, "allow_user_requests": false, "secret_link_expiration": 0 } }, "communities": { "default": "f55b0eac-f9ba-449a-b93e-4abaa5754643", "entries": [ { "access": { "member_policy": "open", "members_visibility": "public", "record_submission_policy": "open", "review_policy": "open", "visibility": "public" }, "children": { "allow": false }, "created": "2016-07-07T00:56:48+00:00", "custom_fields": {}, "deletion_status": { "is_deleted": false, "status": "P" }, "id": "f55b0eac-f9ba-449a-b93e-4abaa5754643", "links": {}, "metadata": { "curation_policy": "A typical work for this community is one that would go into JGR: Space Physics, IEEE TGRS, AGU Earth and Space Science, the CEDAR Workshop or GEM workshop, AGU Fall Meeting SPA section, EGU, URSI or similar in geospace. Perhaps you have a dataset, program, notes, white paper, manuscript, abstract, etc. in this topic area.
\r\n\r\nPlease consider if your work is more oriented towards Astronomy. For example, if your work is about discovering exoplanets via Doppler spectroscopy of stellar spectrum, maybe it's more Astronomy-oriented. If your work is about aurora or magnetospheres of exoplanets, or even intergalactic magnetic fields, then perhaps it would belong in this community.
\r\n\r\nPlease feel free to send a note to the Space Physics curation team if you're not sure if your work fits here or you don't understand why a work was rejected. Note that rejected works still show in Zenodo, just not in this community.
\r\n", "page": "Space Physics: Aeronomy.
\r\n\r\nNote that this is not a general Astronomy, Cosmology, String Theory, et al group.
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