Abstract
The total mass of several quiescent prominences observed in EUV by the AIA instrument on board SDO, in soft X-rays by XRT on Hinode and in H and CaII H by the SLS and HSFA spectrographs of the Ond?rejov observatory, was estimated. Values of asymmetry of coronal emissivity obtained during the mass computations are compared with those estimated from 193Å intensities measured at the disk edge and just above the limb. © 2013 International Astronomical Union.
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Schwartz, P., Heinzel, P., Kotrč, P., Fárník, F., Kupryakov, Y. A., DeLuca, E. E., & Golub, L. (2013). Total mass loading of prominences estimated from their multi-spectral observations. In Proceedings of the International Astronomical Union (Vol. 8, pp. 458–459). Cambridge University Press. https://doi.org/10.1017/S174392131301154X
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