Understanding the solar atmosphere through spectropolarimetric observations and synthetic data
Project/Area Number |
18K13596
|
Research Category |
Grant-in-Aid for Early-Career Scientists
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Allocation Type | Multi-year Fund |
Review Section |
Basic Section 16010:Astronomy-related
|
Research Institution | Japan Aerospace EXploration Agency |
Principal Investigator |
Noda Carlos 国立研究開発法人宇宙航空研究開発機構, 宇宙科学研究所, 国際トップヤングフェロー (70770303)
|
Project Period (FY) |
2018-04-01 – 2019-03-31
|
Project Status |
Discontinued (Fiscal Year 2018)
|
Budget Amount *help |
¥3,900,000 (Direct Cost: ¥3,000,000、Indirect Cost: ¥900,000)
Fiscal Year 2019: ¥1,690,000 (Direct Cost: ¥1,300,000、Indirect Cost: ¥390,000)
Fiscal Year 2018: ¥2,210,000 (Direct Cost: ¥1,700,000、Indirect Cost: ¥510,000)
|
Keywords | Polarimetry / Sun / Magnetism / Solar Polarimetry |
Outline of Annual Research Achievements |
The Kakenhi funding aims to support the work I started around 2016 to help in the development of the SCIP instrument (Katsukawa et al. in preparation). I am the Project Scientist of that instrument, and my main focus is to define the optimum design based on theoretical studies. I have produced a long list of publications, i.e. Quintero Noda et al. (2016, 2017a,b,c, 2018a,b), where step by step I have examined and determined the best instrumental configuration for our purposes, that is understanding the solar magnetism at the lower atmosphere.
Besides those theoretical studies, I wanted to help the SCIP team providing instrumentation. In this regard, as I mentioned in the Kakenhi proposal, the budget was aimed to purchase a scientific camera and additional optical elements. Thus, I bought the camera, and it is already installed in our lab. I am testing it, regarding efficiency, dark current... to verify that it meets our requirements. This camera will be used later this year, around April 2019, when testing the polarisers and different optical elements before installing the flight cameras (provided by an international partner on early 2020). Therefore, this Kakenhi budget is crucial for us because it will help us finalise the instrument on time (the expected flight is 2021) as we can test it while the final components are developed at other institutions. Finally, this grant complements the recently obtained Kakenhi S with reference 18H05234 that will cover the expenses of the rest of the elements and also the preparations for the flight.
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Report
(1 results)
Research Products
(6 results)