Labrosse, Nicolas, Rodger, Andrew S., Radziszewski, Krzysztof, Rudawy, Paweł, Antolin, Patrick, Fletcher, Lyndsay, Levens, Peter J., Peat, Aaron W., Schmieder, Brigitte and Simões, Paulo J. A. (2022) First high resolution interferometric observation of a solar prominence with ALMA. Monthly Notices of the Royal Astronomical Society: Letters, 513 (1). L30-L34. ISSN 1745-3925
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Abstract
We present the first observation of a solar prominence at 84 − 116 GHz using the high resolution interferometric imaging of ALMA. Simultaneous observations in Hα from Białkaw Observatory and with SDO/AIA reveal similar prominence morphology to the ALMA observation. The contribution functions of 3 mm and Hα emission are shown to have significant overlap across a range of gas pressures. We estimate the maximum millimetre-continuum optical thickness to be τ3mm ≈ 2, and the brightness temperature from the observed Hα intensity. The brightness temperature measured by ALMA is ∼6000 − 7000 K in the prominence spine, which correlates well with the estimated brightness temperature for a kinetic temperature of 8000 K.
Item Type: | Article |
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Additional Information: | Funding information: We thank the referee for their comments. Support from STFC grants ST/T000422/1 (NL, LF), ST/N504075/1 (ASR), ST/K502005/1 (PJL) and ST/S505390/1 (AWP) is gratefully acknowledged. P.A. acknowledges STFC support from Ernest Rutherford Fellowship grant number ST/R004285/2. PJAS acknowledges support from CNPq (contract 307612/2019-8) and FAPESP (2013/24155-3). |
Uncontrolled Keywords: | Sun: filaments, prominences |
Subjects: | F300 Physics F500 Astronomy |
Department: | Faculties > Engineering and Environment > Mathematics, Physics and Electrical Engineering |
Depositing User: | Elena Carlaw |
Date Deposited: | 28 Mar 2022 14:38 |
Last Modified: | 10 May 2022 14:15 |
URI: | http://nrl.northumbria.ac.uk/id/eprint/48770 |
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