{"id":{"repo_id":"njit","oai_identifier":"oai:digitalcommons.njit.edu:theses-1223"},"canonical_url":"https://search.dev.ndltd.org/etd/njit/oai:digitalcommons.njit.edu:theses-1223","repository":{"repo_id":"njit","name":"NJIT","base_url":"https://digitalcommons.njit.edu/do/oai/"},"display":{"title":"Characterizing alma for solar observation","abstract":"ALMA (Atacama Large Millimeter/submillimeter Array) is an antenna array of 66 antennas located in northern Chile at 5000 meters altitude. It is the largest ground-based array operated at millimeter/submillimeter wavelengths. In this thesis, the advantages of using ALMA for solar observation are presented, together with the introduction of a campaign to commission ALMA for solar observations. Observation modes of the solar campaign are reviewed in Chapter 2. Methods for constructing images from single dish data as well as the procedure for processing interferometer data, including calibration and imaging, are given in Chapter 3. The CLEAN algorithm that is used for producing images is also discussed in this chapter. Examples of processed images, both for single dish and interferometer, are shown in Chapter 4. In the final Chapter 5, a discussion about what remains to be done to create the observing tool and define observing modes for future ALMA solar campaign is provided.","abstract_html":"ALMA (Atacama Large Millimeter/submillimeter Array) is an antenna array of 66 antennas located in northern Chile at 5000 meters altitude. It is the largest ground-based array operated at millimeter/submillimeter wavelengths. In this thesis, the advantages of using ALMA for solar observation are presented, together with the introduction of a campaign to commission ALMA for solar observations. Observation modes of the solar campaign are reviewed in Chapter 2. Methods for constructing images from single dish data as well as the procedure for processing interferometer data, including calibration and imaging, are given in Chapter 3. The CLEAN algorithm that is used for producing images is also discussed in this chapter. Examples of processed images, both for single dish and interferometer, are shown in Chapter 4. In the final Chapter 5, a discussion about what remains to be done to create the observing tool and define observing modes for future ALMA solar campaign is provided.","abstract_has_math":false,"creators":["Chai, Yi"],"institution":null,"degree_name":"Master of Science in Applied Physics - (M.S.)","degree_level":null,"degree_discipline":"Physics","degree_department":null,"school":null,"contributors":["Dale E. Gary","Haimin Wang","Andrew Gerrard"],"advisors":[],"committee_chairs":[],"committee_members":[],"year":2015,"date_issued":"2015-05-31T07:00:00Z","date_published":"2015-05-31T07:00:00Z","updated_at":"2026-07-24T03:22:34Z","subjects":["Atacama Large Millimeter/submillimeter Array","Solar observation","Other Physics"],"languages":[],"rights":[],"rights_urls":[],"identifier_entries":[]},"links":{"outbound_url":"https://digitalcommons.njit.edu/theses/224","outbound_label":"Repository record","outbound_source":"dc:identifier"},"metadata_groups":[{"id":"people","label":"People","entries":[{"key":"dc:contributor","label":"Contributor","values":["Dale E. 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It is the largest ground-based array operated at millimeter/submillimeter wavelengths. In this thesis, the advantages of using ALMA for solar observation are presented, together with the introduction of a campaign to commission ALMA for solar observations. Observation modes of the solar campaign are reviewed in Chapter 2. Methods for constructing images from single dish data as well as the procedure for processing interferometer data, including calibration and imaging, are given in Chapter 3. The CLEAN algorithm that is used for producing images is also discussed in this chapter. Examples of processed images, both for single dish and interferometer, are shown in Chapter 4. In the final Chapter 5, a discussion about what remains to be done to create the observing tool and define observing modes for future ALMA solar campaign is provided."]},{"key":"dc:title","label":"Title","values":["Characterizing alma for solar observation"]}]}],"canonical_facts":{"dc:contributor":["Dale E. Gary","Haimin Wang","Andrew Gerrard"],"dc:creator":["Chai, Yi"],"dc:description.abstract":["ALMA (Atacama Large Millimeter/submillimeter Array) is an antenna array of 66 antennas located in northern Chile at 5000 meters altitude. It is the largest ground-based array operated at millimeter/submillimeter wavelengths. In this thesis, the advantages of using ALMA for solar observation are presented, together with the introduction of a campaign to commission ALMA for solar observations. Observation modes of the solar campaign are reviewed in Chapter 2. Methods for constructing images from single dish data as well as the procedure for processing interferometer data, including calibration and imaging, are given in Chapter 3. The CLEAN algorithm that is used for producing images is also discussed in this chapter. Examples of processed images, both for single dish and interferometer, are shown in Chapter 4. In the final Chapter 5, a discussion about what remains to be done to create the observing tool and define observing modes for future ALMA solar campaign is provided."],"dc:identifier":["https://digitalcommons.njit.edu/theses/224"],"dc:subject":["Atacama Large Millimeter/submillimeter Array","Solar observation","Other Physics"],"dc:title":["Characterizing alma for solar observation"],"dc:type":["Thesis"],"thesis:degree_discipline":["Physics"],"thesis:degree_name":["Master of Science in Applied Physics - (M.S.)"]},"updated_at":"2026-07-24T03:22:34Z"}