Abstrakti
The SUNRISE balloon-borne solar observatory consists of a 1m aperture Gregory telescope, a UV filter imager, an imaging vector polarimeter, an image stabilization system, and further infrastructure. The first science flight of SUNRISE yielded high-quality data that reveal the structure, dynamics, and evolution of solar convection, oscillations, and magnetic fields at a resolution of around 100 km in the quiet Sun. Here we describe very briefly the mission and the first results obtained from the SUNRISE data, which include a number of discoveries.
Alkuperäiskieli | Englanti |
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Otsikko | 4th Hinode Science Meeting : Unsolved Problems And Recent Insights |
Toimittajat | LRB Rubio, F Reale, M Carlsson |
Kustantaja | Astronomical Society of the Pacific |
Sivut | 143-154 |
Tila | Julkaistu - 2012 |
OKM-julkaisutyyppi | A4 Artikkeli konferenssijulkaisussa |
Tapahtuma | Hinode Science Meeting - Palermo, Italia Kesto: 11 lokak. 2010 → 15 lokak. 2010 Konferenssinumero: 4 |
Julkaisusarja
Nimi | ASP Conference series |
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Kustantaja | Astronomical Society of the Pacific |
Vuosikerta | 455 |
Conference
Conference | Hinode Science Meeting |
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Maa/Alue | Italia |
Kaupunki | Palermo |
Ajanjakso | 11/10/2010 → 15/10/2010 |